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| - | {{Nugget Badge
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| - | |title = High Resolution Temporal and Spatial Structure of a White Light Flare
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| - | |number = 299
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| - | |first_author = Vasyl Yurchyshyn
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| - | |second_author =
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| - | |publish_date = 30 April 2017
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| - | |description = The biggest solar telescope finds still smaller scales for white-light flaring - and more
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| - | {{Nugget Badge
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| - | |title = Multi-Instrument Solar Flare Observations II: A SC24 retrospective
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| - | |number = 298
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| - | |first_author = Ryan Milligan
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| - | |second_author = and Jack Ireland
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| - | |publish_date = 10 April 2017
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| - | |description = Retrospective searches for other useful observations of your favorite flare - how the widget did in Cycle 24
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| - | {{Nugget Badge
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| - | |title = Multi-Instrument Solar Flare Observations I: Solar Flare Finder
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| - | |number = 297
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| - | |first_author = Ryan Milligan
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| - | |second_author = and Kim Tolbert
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| - | |publish_date = 3 April 2017
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| - | |description = Retrospective searches for other useful observations of your favorite flare
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| - | |image = Icon297.png}}
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| - | {{Nugget Badge
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| - | |title = Suppression of Hydrogen Emission in an X-class White-light Solar Flare
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| - | |number = 296
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| - | |first_author = Ondřej Procházka
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| - | |second_author = and Ryan Milligan
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| - | |publish_date = 20 March 2017
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| - | |description = The absence of hydrogen emission lines in a white-light flare suggests an origin in the deep solar atmosphere.
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| - | |image = Icon296.png}}
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| - | {{Nugget Badge
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| - | |title = Radio Emissions from Double RHESSI TGFs
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| - | |number = 295
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| - | |first_author = Andrey Mezentsev
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| - | |second_author = and Thomas Gjesteland
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| - | |publish_date = 13 March 2017
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| - | |description = Lightning helps with microsecond timing calibrations, and is really interesting as a phenomenon of high-energy astrophysics.
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| - | |image = Icon295.png}}
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| - | {{Nugget Badge
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| - | |title = Edward Chupp
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| - | |number = 294
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| - | |first_author = RHESSI
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| - | |second_author =
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| - | |publish_date = 6 March 2017
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| - | |description =
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| - | {{Nugget Badge
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| - | |title = Pierre Kaufmann
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| - | |number = 293
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| - | |first_author = RHESSI
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| - | |second_author =
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| - | |publish_date = 19 February 2017
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| - | |description =
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| - | {{Nugget Badge
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| - | |title = RHESSI's 15th Anniversary
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| - | |number = 292
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| - | |first_author = Brian Dennis, Säm Krucker
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| - | |second_author = and Albert Shih
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| - | |publish_date = 13 February 2017
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| - | |description = RHESSI celebrates 15 years in orbit
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| - | |image = Icon292.png}}
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| - | {{Nugget Badge
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| - | |title = Hard X-ray Emission from Partially Occulted Solar Flares
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| - | |number = 291
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| - | |first_author = Frederic Effenberger
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| - | |second_author = and Fatima Rubio da Costa
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| - | |publish_date = 30 January 2017
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| - | |description = Systematic use of occultation lets us observe the corona in hard X-rays
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| - | |image = Icon291.png}}
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| - | {{Nugget Badge
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| - | |title = GOES Hard X-rays?
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| - | |number = 290
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| - | |first_author = Hugh Hudson, Janet Machol,
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| - | |second_author = and Rodney Viereck
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| - | |publish_date = 16 January 2017
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| - | |description = Solar minimum conditions reveal interesting properties of the GOES X-ray observations
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| - | |image = Icon290.png}}
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| - | {{Nugget Badge
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| - | |title = Syrovatskii's "constant density" approximation
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| - | |number = 289
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| - | |first_author = Hugh Hudson
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| - | |second_author = and Paulo Simões
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| - | |publish_date = 30 December 2016
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| - | |description = Remembering S.I. Syrovatskii; the relevance of the Shmeleva-Syrovatskii “constant density” approximation has been verified by modern high-resolution observations
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| - | |image = Icon289.png}}
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| - | {{Nugget Badge
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| - | |title = Statistical Link Between Electrons Emitting X-rays and Type III Radio Bursts
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| - | |number = 288
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| - | |first_author = Hamish Reid
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| - | |second_author = and Nicole Vilmer
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| - | |publish_date = 19 December 2016
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| - | |description = Correlations across the radio and X-ray spectra imply related populations of source electrons
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| - | |image = Icon288.jpg}}
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| - | {{Nugget Badge
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| - | |title = KW-Sun: The Konus/WIND Hard X-ray Solar Flare Database
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| - | |number = 287
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| - | |first_author = Alexandra Lysenko
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| - | |second_author = and the Konus/WIND Team
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| - | |publish_date = 20 November 2016
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| - | |description = A Hale Cycle's worth of hard X-ray and soft gamma-ray flare observations
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| - | |image = Icon287.png}}
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| - | {{Nugget Badge
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| - | |title = Microwave Emission from Twisted Magnetic Fields
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| - | |number = 286
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| - | |first_author = Mykola Gordovskyy
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| - | |second_author = and Philippa Browning
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| - | |publish_date = 13 November 2016
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| - | |description = The inherent magnetic twist of a flaring loop can be inferred from microwave polarization signatures.
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| - | |image = Icon286.png}}
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| - | {{Nugget Badge
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| - | |title = Spatio-Temporal Dynamics of Flare Hard X-ray Pulsations
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| - | |number = 285
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| - | |first_author = Ivan Zimovets,
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| - | |second_author = Sergey Kuznetsov, Alexander Morgachev, and Alexei Struminsky
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| - | |publish_date = 31 October 2016
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| - | |description = In pulsating flare energy release, the hard X-ray source peaks have different locations.
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| - | |image = Icon285.png}}
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| - | {{Nugget Badge
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| - | |title = Flare-induced Impulsive Sunspot Rotation caught in High Resolution
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| - | |number = 284
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| - | |first_author = Chang Liu
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| - | |second_author = and Haimin Wang
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| - | |publish_date = 24 October 2016
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| - | |description = The tail wags the dog - short time scales for coronal stresses on sunspot structure
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| - | |image = Icon284.png}}
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| - | {{Nugget Badge
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| - | |title = Hard X-ray Polarimetry from Tian Gong 2
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| - | |number = 283
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| - | |first_author = Wojtek Hajdas
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| - | |second_author =
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| - | |publish_date = 20 October 2016
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| - | |description = A novel hard X-ray polarimeter achieves solar "first light"
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| - | |image = Icon283.png}}
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| - | {{Nugget Badge
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| - | |title = A flare in the deep solar atmosphere
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| - | |number = 282
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| - | |first_author = Richard Schwartz
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| - | |second_author = and Hugh Hudson
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| - | |publish_date = 26 September 2016
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| - | |description = RHESSI recently spotted a very fast, very compact, and hot flare event in the deep atmosphere
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| - | |image = Icon_282.png}}
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| - | {{Nugget Badge
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| - | |title = To be or not to be - the role of projection effects in EUV imaging
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| - | |number = 281
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| - | |first_author = Karin Dissauer
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| - | |second_author = and Manuela Temmer
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| - | |publish_date = 16 August 2016
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| - | |description = Perspective matters - application of STEREO views to coronal dimming
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| - | |image = Icon281.png}}
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| - | {{Nugget Badge
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| - | |title = Solar flare neutrons observed on the ground and in space
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| - | |number = 280
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| - | |first_author = Alexander MacKinnon
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| - | |second_author =
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| - | |publish_date = 12 August 2016
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| - | |description = There has been dramatic progress in studying the Sun via its emission of energetic neutrons
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| - | |image = Icon280.png}}
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| - | {{Nugget Badge
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| - | |title = Unexpected intensity distributions of solar electrons in the heliosphere
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| - | |number = 279
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| - | |first_author = Andreas Klassen
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| - | |second_author = and the SEPT/STEREO team
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| - | |publish_date = 13 July 2016
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| - | |description = Solar energetic electrons may have complicated and informative distributions in the interplanetary medium
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| - | |image = Icon279.png}}
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| - | {{Nugget Badge
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| - | |title = Initiation of a type II radio burst without a CME
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| - | |number = 278
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| - | |first_author = Pankaj Kumar,
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| - | |second_author = Davina Innes, and Kyung-Suk Cho
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| - | |publish_date = 4 July 2016
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| - | |description = A global coronal shock wave without a CME driver
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| - | |image = Icon278.png}}
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| - | {{Nugget Badge
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| - | |title = Spotlessness returns
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| - | |number = 277
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| - | |first_author = Hugh Hudson
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| - | |second_author =
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| - | |publish_date = 27 June 2016
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| - | |description = The Sun had no spots for extended periods in June, 2016
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| - | |image = Icon277.png}}
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| - | {{Nugget Badge
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| - | |title = RHESSI has resumed operations
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| - | |number = 276
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| - | |first_author = Albert Shih,
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| - | |second_author = Brian Dennis and Säm Krucker
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| - | |publish_date = 20 June 2016
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| - | |description = A successful anneal and RHESSI continues to provide data
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| - | |image = Icon276.png}}
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| - | {{Nugget Badge
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| - | |title = Non-thermal recombination in solar flares and microflares
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| - | |number = 275
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| - | |first_author = Jeffrey Reep
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| - | |second_author = and John Brown
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| - | |publish_date = 6 June 2016
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| - | |description = A heretofore unrecognized emission mechanism for solar hard X-rays
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| - | |image = Icon275.png}}
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| - | {{Nugget Badge
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| - | |title = Data-driven radiative hydrodynamic modeling of SOL2014-03-29
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| - | |number = 274
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| - | |first_author = Fatima Rubio da Costa
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| - | |second_author =
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| - | |publish_date = 10 May 2016
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| - | |description = Intense pulses of energy modeled with RADYN
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| - | |image = Icon274.png}}
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| - | {{Nugget Badge
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| - | |title =Electron acceleration and hard X-ray emission from SOL2013-11-09
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| - | |number = 273
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| - | |first_author =Yuri Tsap
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| - | |second_author = and Galina Motorina
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| - | |publish_date = 5 May 2016
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| - | |description = Testing the thick-target model in an interesting flare
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| - | |image = Icon273.png}}
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| - | {{Nugget Badge
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| - | |title = Extreme events, stellar evolution, and magnetic reconnection
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| - | |number = 272
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| - | |first_author = Hugh Hudson
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| - | |second_author =
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| - | |publish_date = 30 April 2016
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| - | |description = Stellar activity measured by flare rates over the eons
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| - | |image = 272f3.jpg}}
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| - | {{Nugget Badge
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| - | |title = Radio polarization signatures in twisted flare loops
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| - | |number = 271
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| - | |first_author = Ivan Sharykin
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| - | |second_author = and Alexei Kuznetsov
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| - | |publish_date = 25 April 2016
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| - | |description = Flux-rope geometry via radio polarization signs
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| - | |image = Icon271.png}}
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| - | {{Nugget Badge
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| - | |title = An Unreported White-light Prominence
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| - | |number = 270
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| - | |first_author = Matt Penn
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| - | |second_author = and Hugh Hudson
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| - | |publish_date = 28 March 2016
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| - | |description = Massive flare ejecta observed visually
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| - | |image = Icon270.png}}
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| - | {{Nugget Badge
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| - | |title = RHESSI's 5th Anneal
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| - | |number = 269
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| - | |first_author = Albert Shih
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| - | |second_author = and Brian Dennis
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| - | |publish_date = 23 February 2016
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| - | |description = RHESSI has begun annealing its detectors, interrupting the flow of data for several weeks
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| - | |image = Icon269.png}}
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| - | {{Nugget Badge
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| - | |title = A new development in the Frost-Dennis paradigm
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| - | |number = 268
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| - | |first_author = Hugh Hudson,
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| - | |second_author = Melissa Pesce-Rollins, and Larisa Kashapova
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| - | |publish_date = 22 February 2016
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| - | |description = The Fermi/LAT long-duration events look like SOL1969-03-30
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| - | |image = Icon268.png}}
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| - | {{Nugget Badge
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| - | |title = When the Earth’s atmosphere becomes dynamic…
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| - | |number = 267
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| - | |first_author = Manuela Temmer,
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| - | |second_author = Sandro Krauss and Astrid Veronig
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| - | |publish_date = 13 February 2016
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| - | |description = The Earth's ionosphere reacts strongly to the occurrence of flares and CMEs
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| - | |image = Icon267.png}}
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| - | {{Nugget Badge
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| - | |title = Hard X-ray Directivity Measurements with STIX and MiSolFA
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| - | |number = 266
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| - | |first_author = Diego Casadei
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| - | |second_author = and Hugh Hudson
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| - | |publish_date = 7 December 2015
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| - | |description = Precise stereoscopic observations of hard X-rays can reveal electron beams
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| - | |image = Icon266.png}}
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| - | {{Nugget Badge
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| - | |title = On the Correlation of HXR and WL Emission in Solar Flares
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| - | |number = 265
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| - | |first_author = Matej Kuhar
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| - | |second_author =
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| - | |publish_date = 19 November 2015
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| - | |description = New data sharpen the correlations between hard X-rays and white light, but interesting questions remain open
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| - | |image = Icon265.png}}
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| - | {{Nugget Badge
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| - | |title = How to better determine the power in non-thermal electrons from observed X-ray spectra
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| - | |number = 264
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| - | |first_author = Eduard Kontar,
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| - | |second_author = Gordon Emslie, Natasha Jeffrey, and Nic Bian
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| - | |publish_date = 9 November 2015
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| - | |description = Incorporation of energy diffusion for electron transport helps with flare energetics
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| - | |image = Icon264.png}}
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| - | {{Nugget Badge
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| - | |title = Soft and Hard X-rays, Flares, and the Corona
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| - | |number = 263
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| - | |first_author = Hugh Hudson
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| - | |second_author =
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| - | |publish_date = 20 October 2015
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| - | |description = Behavior of the X-ray Sun at low activity levels
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| - | |image = Icon263.png}}
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| - | {{Nugget Badge
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| - | |title = Fine Structure in Flare Soft X-ray Light Curves
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| - | |number = 262
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| - | |first_author = Brian Dennis
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| - | |second_author = and Kim Tolbert
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| - | |publish_date = 21 September 2015
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| - | |description = A tool that we've had since 1976 now gives us surprisingly precise new information
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| - | |image = Icon262.png}}
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| - | {{Nugget Badge
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| - | |title = Photospheric Electric Fields and Energy Fluxes in the Eruptive Active Region NOAA 11158
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| - | |number = 261
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| - | |first_author = Maria Kazachenko
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| - | |second_author =
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| - | |publish_date = 14 September 2015
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| - | |description = Flares need magnetic energy. We can now measure its arrival as Poynting flux across the solar photosphere.
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| - | |image = Icon261.png}}
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| - | {{Nugget Badge
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| - | |title = RHESSI and General Relativity
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| - | |number = 260
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| - | |first_author = Bill Thompson
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| - | |second_author = and Hugh Hudson
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| - | |publish_date = 7 September 2015
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| - | |description = General-relativistic corrections to RHESSI source positions
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| - | |image = Icon260.png}}
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| - | {{Nugget Badge
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| - | |title = Return-current Model Spectra and Enhanced Plasma Resistivity
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| - | |number = 259
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| - | |first_author = Meriem Alaoui
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| - | |second_author = and Gordon Holman
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| - | |publish_date = 31 August 2015
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| - | |description = A basic return-current model matches RHESSI hard X-ray spectra and implies a need for anomalous resistivity
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| - | |image = Icon259.png}}
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| - | {{Nugget Badge
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| - | |title = High Energies in the Inner Heliosphere
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| - | |number = 258
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| - | |first_author = Hugh Hudson
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| - | |second_author =
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| - | |publish_date = 24 August 2015
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| - | |description = Cosmic rays measure the coronal magnetic field at the PFSS source surface itself
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| - | |image = Icon258.png}}
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| - | {{Nugget Badge
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| - | |title = A Two-ribbon White-light Flare Associated with a Failed Solar Eruption
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| - | |number = 257
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| - | |first_author = Xin CHENG
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| - | |second_author =
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| - | |publish_date = 13 July 2015
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| - | |description = The ONSET facility in Yunnan observes an interesting flare event
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| - | |image = Icon257.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = The Fastest Flare
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| - | |number = 256
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| - | |first_author = Hugh Hudson
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| - | |second_author = and Paulo Simões
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| - | |publish_date = 29 June 2015
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| - | |description = A GOES soft X-ray burst lasting less than one minute - with hard X-rays and white-light continuum
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| - | |image = Icon256.png}}
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| - | {{Nugget Badge
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| - | |title = High-energy Electrons and Electric Currents during a Flare
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| - | |number = 255
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| - | |first_author = Sophie Musset,
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| - | |second_author = Nicole Vilmer and Véronique Bommier
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| - | |publish_date = 22 June 2015
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| - | |description = Photospheric vertical currents linked to sites of electron acceleration in the corona
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| - | |image = Icon255.png}}
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| - | {{Nugget Badge
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| - | |title = High Dispersion Spectroscopy of solar-type superflare stars
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| - | |number = 254
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| - | |first_author = Yuta Notsu
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| - | |second_author =
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| - | |publish_date = 8 June 2015
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| - | |description = Researching the properties of Kepler's solar-type superflare stars
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| - | |image = Icon254.png}}
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| - | {{Nugget Badge
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| - | |title = "Superflares" on solar-type stars observed with Kepler
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| - | |number = 253
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| - | |first_author = Hiroyuki Maehara
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| - | |second_author =
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| - | |publish_date = 1 June 2015
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| - | |description = Flare energies 10-1000 times those of the most powerful solar flares
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| - | |image = Icon253.png}}
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| - | {{Nugget Badge
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| - | |title = EOVSA Coverage of a Recent Gamma-Ray Flare
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| - | |number = 252
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| - | |first_author = Dale Gary
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| - | |second_author = and Gregory Fleishman
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| - | |publish_date = 11 May 2015
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| - | |description = A recent gamma-ray flare observed with Owens Valley microwave imaging spectroscopy
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| - | |image = Icon252.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = Ionospheric Effects, Flare History, and Dick Donnelly
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| - | |number = 251
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| - | |first_author = Hugh Hudson
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| - | |second_author = and Peter Gallagher
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| - | |publish_date = 27 April 2015
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| - | |description = Recognizing the world’s largest X-ray detector, its ionosphere
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| - | |image = 251f3.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = RHESSI Detection of X-ray Emission from a Quiet-Sun Filament Eruption
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| - | |number = 250
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| - | |first_author =Gordon Holman
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| - | |second_author = and Adi Foord
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| - | |publish_date = 13 April 2015
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| - | |description = A RHESSI X-ray flare is detected outside an active region
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| - | |image = Icon250.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = Soft X-ray emission in kink-unstable coronal loops
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| - | |number = 249
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| - | |first_author = Rui Pinto,
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| - | |second_author = Nicole Vilmer, and Sacha Brun
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| - | |publish_date = 30 March 2015
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| - | |description = Kinking flux ropes can create flare emission, but their detection may be deceptive
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| - | |image = Icon249.png}}
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| - | {{Nugget Badge
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| - | |title = Daily solar mm-observations at Aalto University Metsähovi Radio Observatory
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| - | |number = 248
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| - | |first_author = Juha Kallunki
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| - | |second_author = and Minttu Uunila
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| - | |publish_date = 16 March 2015
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| - | |description = Systematic microwave and mm-wave solar observations from Finland
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| - | |image = Icon248.png}}
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| - | {{Nugget Badge
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| - | |title = Solar Physics during the March 2015 Solar Eclipse
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| - | |number = 247
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| - | |first_author = Hamish Reid
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| - | |second_author = and Hugh Hudson
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| - | |publish_date = 9 March 2015
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| - | |description = A total solar eclipse is coming on 2015 March 20, a good opportunity for many observatories
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| - | |image = Icon247.png}}
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| - | {{Nugget Badge
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| - | |title = Glasgow Callisto and CMEless type II bursts
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| - | |number = 246
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| - | |first_author = Peter Wakeford
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| - | |second_author = and Hugh Hudson
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| - | |publish_date = 16 February 2015
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| - | |description = The Glasgow Callisto telescope observes rare type II bursts without CME drivers
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| - | |image = Icon246.png}}
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| - | {{Nugget Badge
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| - | |title = Flare Heating by Mildly Non-thermal Particles
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| - | |number = 245
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| - | |first_author = Jeffrey Reep
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| - | |second_author =
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| - | |publish_date = 26 January 2015
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| - | |description = Sorting out nonthermal distributions via HYDRAD models
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| - | |image = Icon245.png}}
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| - | {{Nugget Badge
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| - | |title = Above-the-Looptop Sources
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| - | |number = 244
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| - | |first_author = Mitsuo Oka
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| - | |second_author = and Säm Krucker
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| - | |publish_date = 12 January 2015
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| - | |description = Electron distribution functions in coronal sources
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| - | |image = Icon244.png}}
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| - | {{Nugget Badge
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| - | |title = The IAU Solar Target Identifier - A Good Thing
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| - | |number = 243
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| - | |first_author = Hugh Hudson
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| - | |second_author = and John Leibacher
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| - | |publish_date = 29 December 2014
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| - | |description = Standardized names for flares help a lot
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| - | |image = Icon243.png}}
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| - | {{Nugget Badge
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| - | |title = The Low-High-Low Starting Frequency Trend in Groups of Type III Bursts
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| - | |number = 242
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| - | |first_author = Hamish Reid
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| - | |second_author =
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| - | |publish_date = 23 December 2014
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| - | |description = The type III radio bursts echo the pattern of flare energy release
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| - | |image = Icon242.png}}
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| - | {{Nugget Badge
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| - | |title = The Solar X-ray Limb II
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| - | |number = 241
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| - | |first_author = Marina Battaglia
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| - | |second_author = and Hugh Hudson
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| - | |publish_date = 24 November 2014
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| - | |description = X-raying the mass distribution at the limb of the Sun: the true solar radius
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| - | |image = Icon241.png}}
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| - | {{Nugget Badge
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| - | |title = Back from the Far Side
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| - | |number = 240
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| - | |first_author = Hugh Hudson
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| - | |second_author = and Greg Slater
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| - | |publish_date = 17 November 2014
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| - | |description = Active region 2192 has returned as 2209, still no CMEs
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| - | |image = Icon240.png}}
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| - | {{Nugget Badge
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| - | |title = A Record-Setting CMEless Flare
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| - | |number = 239
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| - | |first_author = Sam Freeland
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| - | |second_author = and Greg Slater
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| - | |publish_date = 27 October 2014
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| - | |description = Active region 2192 produced many huge flares, but no CMEs
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| - | |image = Icon239.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = The Formation of Kappa Distributions in Solar Flares
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| - | |number = 238
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| - | |first_author = Nicolas Bian
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| - | |second_author = and Duncan Stackhouse
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| - | |publish_date = 13 October 2014
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| - | |description = Kappa distributions may form naturally in certain flare environments
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| - | |image = Icon238.png}}
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| - | {{Nugget Badge
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| - | |title = The Balmer continuum observed from IRIS!
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| - | |number = 237
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| - | |first_author = Petr Heinzel
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| - | |second_author = and Lucia Kleint
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| - | |publish_date = 29 September 2014
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| - | |description = For the first time we have clear and direct observations of the Balmer continuum, from space
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| - | |image = Icon237.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = Energy goes up... but doesn't come back down! Coronal heating?
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| - | |number = 236
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| - | |first_author = Brian Welsch
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| - | |second_author =
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| - | |publish_date = 22 September 2014
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| - | |description = The Poynting flux responsible for coronal heating may have been spotted
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| - | |image = Icon236.png}}
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| - | {{Nugget Badge
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| - | |title = Which detectors can I use to analyze this flare?
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| - | |number = 235
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| - | |first_author = Brian Dennis
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| - | |second_author = and Kim Tolbert
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| - | |publish_date = 15 September 2014
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| - | |description = A new Browser feature helps to answer this question
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| - | |image = Icon235.png}}
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| - | {{Nugget Badge
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| - | |title = RHESSI Resumes Observations
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| - | |number = 234
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| - | |first_author = Albert Shih
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| - | |second_author = and Säm Krucker
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| - | |publish_date = 1 September 2014
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| - | |description = Back to normal, the anneal was a success
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| - | |image = Icon234.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = EUNIS Sees Pervasive Faint Fe XIX Emission: Evidence for Nanoflare Heating
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| - | |number = 233
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| - | |first_author = Jeff Brosius
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| - | |second_author =
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| - | |publish_date = 18 August 2014
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| - | |description = Faint emission at flare-like temperatures in a large coronal area
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| - | |image = Icon233.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = Octupolar out-of-plane magnetic field structure generation during magnetic reconnection
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| - | |number = 232
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| - | |first_author = Jan Graf von der Pahlen
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| - | |second_author = and David Tsiklauri
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| - | |publish_date = 11 August 2014
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| - | |description = A new characteristic marker of reconnection
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| - | |image = Icon232.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = Flare Observed by a Dozen Instruments
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| - | |number = 231
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| - | |first_author = Lucia Kleint
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| - | |second_author = and Kevin Reardon
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| - | |publish_date = 28 July 2014
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| - | |description = A wonderful flare observed by a grand set of instruments, including IRIS and IBIS
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| - | |image = Icon231.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = The Redistribution of Nonthermal Electron Energy
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| - | |number = 230
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| - | |first_author = Ryan Milligan
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| - | |second_author =
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| - | |publish_date = 14 July 2014
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| - | |description = Describing what we know about the dominant energy driving a solar flare
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| - | |image = Icon230.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = RHESSI is Annealing Now
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| - | |number = 229
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| - | |first_author = Albert Shih
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| - | |second_author = and Martin Fivian
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| - | |publish_date = 7 July2014
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| - | |description = A fourth repair job for RHESSI, smoothing out radiation damage
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| - | |image = Icon229.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = Mysteries of Flare/CME Initiation
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| - | |number = 228
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| - | |first_author = Shaun Bloomfield
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| - | |second_author = and Hugh Hudson
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| - | |publish_date = 8 June 2014
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| - | |description = Pairs of flares
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| - | |image = Icon228.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = Solar Cosmic Rays, Neutrons, and Fermi Gamma-Rays
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| - | |number = 227
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| - | |first_author = Hugh Hudson
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| - | |second_author = and Alec MacKinnon
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| - | |publish_date = 24 May 2014
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| - | |description = Exciting new solar high-energy observations
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| - | |image = Icon227.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = The 3D standard model for eruptive flares
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| - | |number = 226
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| - | |first_author = Miho Janvier
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| - | |second_author =
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| - | |publish_date = 10 May 2014
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| - | |description = Torus instability and slipping reconnection
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| - | |image = Icon226.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = Microwave Images of a Single-Loop Flare: Observations and Simulations
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| - | |number = 225
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| - | |first_author = Alexey Kuznetsov
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| - | |second_author = and Eduard Kontar
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| - | |publish_date = 28 April 2014
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| - | |description = A flare analysis making use of the new GX Simulator modeling software
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| - | |image = Icon225.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title =Abundances in Solar Flares
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| - | |number = 224
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| - | |first_author = Harry Warren
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| - | |second_author =
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| - | |publish_date = 21 April 2014
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| - | |description = Wrinkles in the FIP effect for flares
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| - | |image = Icon224.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title =Homing in on Flare Energy
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| - | |number = 223
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| - | |first_author = Hugh Hudson
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| - | |second_author = and Ryan Milligan
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| - | |publish_date = 14 April 2014
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| - | |description = Representing the spectral energy distribution of a flare
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| - | |image = Icon223.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title =Empirical Constructs and Cartoons
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| - | |number = 222
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| - | |first_author = Forrest Mozer
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| - | |second_author = and Hugh Hudson
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| - | |publish_date = 24 March 2014
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| - | |description = How our mental images may relate to what's really going on
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| - | |image = Icon222.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = Imaging Quasi-Periodic Oscillations in a Simple Flare
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| - | |number = 221
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| - | |first_author = Zongjun Ning
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| - | |second_author = and Hugh Hudson
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| - | |publish_date = 17 March 2014
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| - | |description = Time-series imaging spectroscopy in a B8 flare
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| - | |image = Icon221.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = A Wonderful Cycle 24 Flare
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| - | |number = 220
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| - | |first_author = Säm Krucker
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| - | |second_author = and Hugh Hudson
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| - | |publish_date = 3 March 2014
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| - | |description = There have been quite a few Cycle 24 X-class flares, and this was one of the nicest
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| - | |image = Icon220.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = Instantaneous Flare Properties
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| - | |number = 218
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| - | |first_author = Hugh Hudson
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| - | |second_author =
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| - | |publish_date = 10 February 2014
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| - | |description = Let's look at the derivative
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| - | |image = Icon218.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = Reflection of Coronal Global Waves
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| - | |number = 217
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| - | |first_author = Ines Kienreich
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| - | |second_author = and Hugh Hudson
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| - | |publish_date = 13 January 2014
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| - | |description = A homologous series of global coronal waves reflects at a coronal-hole boundary
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| - | |image = Icon217.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = Flare Coronal Rain
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| - | |number = 216
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| - | |first_author = Hugh Hudson
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| - | |second_author = and Säm Krucker
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| - | |publish_date = 23 December 2013
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| - | |description = Thermal collapse in flare loops seen in a wonderful new way
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| - | |image = Icon216.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = The HEROES Mission: High Energy Replicated Optics to Explore the Sun
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| - | |number = 215
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| - | |first_author = Steven Christe
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| - | |second_author = and Albert Shih
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| - | |publish_date = 16 December 2013
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| - | |description = Focusing optics to explore the high-energy Sun
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| - | |image = Icon215.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = CMEs on young, solar-type stars
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| - | |number = 214
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| - | |first_author = Alicia Aarnio
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| - | |second_author =
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| - | |publish_date = 9 December 2013
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| - | |description = Stellar flares and CMEs behave like solar ones
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| - | |image = Icon214.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = The 1859 Space Weather Event Revisited
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| - | |number = 213
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| - | |first_author = Ed Cliver
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| - | |second_author =
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| - | |publish_date = 25 November 2013
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| - | |description = Assessing the greatest space-weather events over the centuries
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| - | |image = Icon213.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = Hard X-ray Footpoint Asymmetry
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| - | |number = 212
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| - | |first_author = Ya-Hui YANG
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| - | |second_author =
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| - | |publish_date = 7 November 2013
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| - | |description = The behavior of conjugacy in flare footpoints
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| - | |image = Icon212.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = The Halloween Flares and Large-Scale Correlations
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| - | |number = 211
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| - | |first_author = Richard Schwartz
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| - | |second_author = and Hugh Hudson
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| - | |publish_date = 28 October 2013
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| - | |description = Flares bunch up strikingly
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| - | |image = Icon211.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = Scattering Polarization in Solar Flares
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| - | |number = 210
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| - | |first_author = Jiři Štěpán
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| - | |second_author = and Petr Heinzel
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| - | |publish_date = 21 October 2013
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| - | |description = Linear polarization produced by anisotropy, rather than particle-beam impact
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| - | |image = Icon210.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = The Flare that Time Forgot
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| - | |number = 209
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| - | |first_author = Paulo Simöes
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| - | |second_author = and Hugh Hudson
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| - | |publish_date = 13 October 2013
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| - | |description = A long-forgotten Masuda flare reappears
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| - | |image = Icon209.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = The Post-Burst Increase
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| - | |number = 208
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| - | |first_author = Hugh Hudson
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| - | |second_author =
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| - | |publish_date = 30 September 2013
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| - | |description = Tutorial on flare thermal sources seen in microwaves
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| - | |image = Icon208.png}}
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| - | {{Nugget Badge
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| - | |title = Peristaltic Shocks: a model
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| - | |number = 207
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| - | |first_author = Dana Longcope
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| - | |second_author = and Roger Scott
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| - | |publish_date = 16 September 2013
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| - | |description = Reconciling reconnection with high preflare coronal densities
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| - | |image = Icon207.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = Negative Microwave Bursts
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| - | |number = 206
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| - | |first_author = Victor Grechnev
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| - | |second_author = and Hugh Hudson
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| - | |publish_date = 3 September 2013
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| - | |description = Negative microwave bursts happen, in association with flares and "Hyder flares," and modern instrumentation makes them very interesting again
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| - | |image = Icon206.png}}
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| - | {{Nugget Badge
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| - | |title = Acceleration-region Densities
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| - | |number = 205
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| - | |first_author = Säm Krucker
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| - | |second_author = and Marina Battaglia
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| - | |publish_date = 6 August 2013
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| - | |description = Independent constraints on the densities of ions and non-thermal electrons reveal bulk acceleration
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| - | |image = Icon205.png}}
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| - | {{Nugget Badge
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| - | |title = Implosion and Oscillation
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| - | |number = 204
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| - | |first_author = Paulo Simões
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| - | |second_author = and Hugh Hudson
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| - | |publish_date = 29 July 2013
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| - | |description = The flare implosion originates in the lower atmosphere and involves GOES soft X-rays
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| - | |image = Icon204.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = Minoflares
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| - | |number = 203
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| - | |first_author = Iain Hannah
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| - | |second_author = and Hugh Hudson
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| - | |publish_date = 1 July 2013
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| - | |description = Earmarks of widespread energetic events in the solar atmosphere
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| - | |image = Icon203.png}}
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| - | {{Nugget Badge
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| - | |title = Mars Odyssey/HEND and RHESSI
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| - | |number = 202
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| - | |first_author = Vadim Vybornov
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| - | |second_author = and Michael A. Livshits
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| - | |publish_date = 9 June 2013
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| - | |description = An event from far behind the solar limb, observed at Mars
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| - | |image = Icon202.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = Hard X-rays in Descent
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| - | |number = 201
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| - | |first_author = Aidan O'Flannagain,
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| - | |second_author = John Brown and Peter Gallagher
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| - | |publish_date = 27 May 2013
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| - | |description = A novel test of the thick-target model
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| - | |image = Icon200.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = Too few? Too many?
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| - | |number = 200
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| - | |first_author = Paulo Simões
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| - | |second_author = and Eduard Kontar
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| - | |publish_date = 13 May 2013
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| - | |description = Too few electrons in the footpoints; too many electrons in the corona
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| - | |image = Icon201.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = A huge gamma-ray burst
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| - | |number = 199
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| - | |first_author = David Smith
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| - | |second_author = and André Csillaghy
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| - | |publish_date = 6 May 2013
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| - | |description = A wonderfully bright gamma-ray burst at Z = 0.34
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| - | |image = Icon199.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = Three-phase life leads to corpulent X-ray loops
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| - | |number = 198
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| - | |first_author = Natasha Jeffrey
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| - | |second_author = and Eduard Kontar
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| - | |publish_date = 15 April 2013
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| - | |description = RHESSI observations explore structural changes in flaring loops
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| - | |image = Icon198.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = Antipodal Flares
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| - | |number = 197
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| - | |first_author = B. Pecos
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| - | |second_author = and B. Paul
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| - | |publish_date = 1 April 2013
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| - | |description = Flares on a solar diameter suggest a new subatomic particle
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| - | |image = Icon197.png}}
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| - |
| |
| - | {{Nugget Badge
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| - | |title = Observational evidence for breakout reconnection
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| - | |number = 196
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| - | |first_author =Henry Aurass
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| - | |second_author = and Gordon Holman
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| - | |publish_date = 18 March 2013
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| - | |description = Coronal particle acceleration marks the eruption of a SEE
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| - | |image = Icon196.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = Burst-on-Tail (BOT)
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| - | |number = 195
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| - | |first_author = Alex Struminsky
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| - | |second_author = and Ivan Zimovets
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| - | |publish_date = 4 March 2013
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| - | |description = A "Burst-on-Tail" (BOT) phenomenon
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| - | |image = Icon195.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = Electron re-acceleration and HXR emission
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| - | |number = 194
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| - | |first_author = Heather Ratcliffe
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| - | |second_author = and Marian Karlický
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| - | |publish_date =18 February 2013
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| - | |description = Can wave-particle interactions solve the electron number problem?
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| - | |image = Icon194.png}}
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| - | {{Nugget Badge
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| - | |title = Passages of Electron Beams
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| - | |number = 193
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| - | |first_author = Bin Chen
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| - | |second_author = and Tim Bastian
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| - | |publish_date =11 February 2013
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| - | |description = New VLA capability for imaging spectroscopy shows several remarkable features of type III bursts
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| - | |image = Icon193.png}}
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| - | {{Nugget Badge
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| - | |title = Kappa Distribution
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| - | |number = 192
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| - | |first_author = Mitsuo Oka
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| - | |second_author =
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| - | |publish_date =21 January 2013
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| - | |description = A simpler function fits both thermal and nonthermal RHESSI spectral ranges
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| - | |image = Icon192.jpg}}
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| - | {{Nugget Badge
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| - | |title = Hard X-ray Spikes Observed by RHESSI
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| - | |number = 191
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| - | |first_author = Jiong Qiu
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| - | |second_author =
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| - | |publish_date =7 January 2013
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| - | |description = New software allows RHESSI to study rapid time variations
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| - | |image = Icon191.png}}
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| - | {{Nugget Badge
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| - | |title = Flare Productivity
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| - | |number = 190
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| - | |first_author = Hugh Hudson
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| - | |second_author = and Lyndsay Fletcher
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| - | |publish_date =27 December 2012
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| - | |description = An anomalous change in flare productivity per active region
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| - | |image = Icon190.png}}
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| - | {{Nugget Badge
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| - | |title = FOXSI Success
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| - | |number = 189
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| - | |first_author = Lindsay Glesener
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| - | |second_author = and Säm Krucker
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| - | |publish_date =27 December 2012
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| - | |description = The FOXSI rocket soars, and a flare occurs on schedule
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| - | |image = Icon189.png}}
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| - | {{Nugget Badge
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| - | |title = "Impulse Response Flares" and Gamma Rays
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| - | |number = 188
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| - | |first_author = Stephen White
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| - | |second_author = and Hugh Hudson
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| - | |publish_date =13 November 2012
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| - | |description = A simplifying paradigm may describe acceleration to the highest energies in flares
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| - | |image = Icon188.png}}
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| - | {{Nugget Badge
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| - | |title = Glasgow Callisto optimistic: first light comes in focus
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| - | |number = 187
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| - | |first_author = Heather Ratcliffe
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| - | |second_author = and Eduard Kontar
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| - | |publish_date =29 October 2012
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| - | |description = The Glasgow Callisto radio observatory is on line
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| - | |image = Icon187.png}}
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| - | {{Nugget Badge
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| - | |title = Photospheric Temperature Gradient
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| - | |number = 186
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| - | |first_author = Martin Fivian
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| - | |second_author = and Hugh Hudson
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| - | |publish_date =22 October 2012
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| - | |description = RHESSI observes the photosphere with exquisite precision
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| - | |image = Icon186.png}}
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| - | {{Nugget Badge
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| - | |title = Energy Partition in Large Solar Eruptive Events
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| - | |number = 185
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| - | |first_author = Gordon Emslie
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| - | |second_author = and Brian Dennis
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| - | |publish_date =5 October 2012
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| - | |description = Where the flare energy comes from, and where it goes to.
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| - | |image = Icon185.png}}
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| - | {{Nugget Badge
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| - | |title = New TGFs Found in the RHESSI Data
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| - | |number = 184
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| - | |first_author = Thomas Gjesteland
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| - | |second_author = and Nikolai Østgaard
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| - | |publish_date =10 September 2012
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| - | |description = RHESSI sees many, many gamma-ray flashes from lightning
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| - | |image = Icon184.png}}
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| - | {{Nugget Badge
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| - | |title = The RHESSI Flare Catalog
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| - | |number = 183
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| - | |first_author = Jim McTiernan
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| - | |second_author = and Hugh Hudson
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| - | |publish_date = 29 August 2012
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| - | |description = The Catalog is a powerful and easy-to-use access tool for the RHESSI flare observations
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| - | |image = Icon183.png}}
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| - | {{Nugget Badge
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| - | |title = RHESSI Catches Gamma-Ray Bursts
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| - | |number = 182
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| - | |first_author = Jakub Ripa
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| - | |second_author =
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| - | |publish_date = 15 August 2012
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| - | |description = RHESSI catches gamma-ray bursts, and they come in three flavors
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| - | |image = Icon182.jpg}}
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| - | {{Nugget Badge
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| - | |title = Dense Loop Flares
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| - | |number = 181
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| - | |first_author = Jingnan Guo
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| - | |second_author = and Gordon Emslie
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| - | |publish_date =6 August 2012
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| - | |description = Direct electron mapping teaches us about the structure of electron acceleration in flares
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| - | |image = Icon181.png}}
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| - | {{Nugget Badge
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| - | |title = The Slowest Flare
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| - | |number = 180
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| - | |first_author = Sam Freeland
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| - | |second_author = and Hugh Hudson
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| - | |publish_date =23 July 2012
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| - | |description = A flare with an exceptionally slow rise phase, more than 5 hours in GOES 1-8 A soft X-rays
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| - | |image = Icon180.png}}
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| - | {{Nugget Badge
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| - | |title = Dimmings and Sustained Gamma-Ray Events
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| - | |number = 179
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| - | |first_author = Hugh Hudson
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| - | |second_author = and Nicola Omodei
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| - | |publish_date =25 June 2012
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| - | |description = Coronal disruptions reveal themselves as depletions and gamma-ray emissions
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| - | |image = Icon179.png}}
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| - | {{Nugget Badge
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| - | |title = Flare Nimbus
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| - | |number = 178
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| - | |first_author = Susan McKenna-Lawlor
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| - | |second_author =
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| - | |publish_date =14 June 2012
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| - | |description = The Flare Nimbus, its history and significance
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| - | |image = Icon178.jpg}}
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| - | {{Nugget Badge
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| - | |title = RHESSI and the Transit of Venus I
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| - | |number = 177
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| - | |first_author = Hugh Hudson
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| - | |second_author = and Martin Fivian
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| - | |publish_date =1 June 2012
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| - | |description = RHESSI prepares for the June 5/6 Venus transit
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| - | |image = Icon177.jpg}}
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| - | {{Nugget Badge
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| - | |title = Time Profiles of Solar Flare Densities
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| - | |number = 176
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| - | |first_author = Ryan Milligan
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| - | |second_author = and Michael Kennedy
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| - | |publish_date =21 May 2012
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| - | |description = Density-diagnostic line ratios in EVE spectra
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| - | |image = Icon176.png}}
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| - | {{Nugget Badge
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| - | |title = Solar energetic electron events over one solar cycle
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| - | |number = 175
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| - | |first_author = Linghua Wang
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| - | |second_author =
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| - | |publish_date =7 May 2012
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| - | |description = The statistics of SEP electrons
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| - | |image = Icon175.png}}
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| - | {{Nugget Badge
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| - | |title = A Shocking Type II
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| - | |number = 174
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| - | |first_author = Hazel Bain,
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| - | |second_author = Säm Krucker and Lyndsay Glesener
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| - | |publish_date =30 April 2012
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| - | |description = The properties of global coronal waves sorted out
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| - | |image = icon174.png}}
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| - | {{Nugget Badge
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| - | |title = RHESSI and IRIS
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| - | |number = 173
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| - | |first_author = Hugh Hudson
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| - | |second_author =
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| - | |publish_date =16 April 2012
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| - | |description = Flare gold at the foot of the rainbow
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| - | |image = icon173.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = A New Day Dawns
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| - | |number = 172
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| - | |first_author = Dale Gary
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| - | |second_author =
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| - | |publish_date =26 March 2012
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| - | |description = Soon, true microwave imaging spectroscopy
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| - | |image = icon172.png}}
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| - | {{Nugget Badge
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| - | |title = An Fe Cascade
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| - | |number = 171
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| - | |first_author = Hugh Hudson
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| - | |second_author =
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| - | |publish_date =12 March 2012
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| - | |description = Iron everywhere in the EVE spectra
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| - | |image = icon171.png}}
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| - | {{Nugget Badge
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| - | |title = Do slow waves trigger pulsations in two-ribbon flares? An observational search
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| - | |number = 170
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| - | |first_author = A. Inglis
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| - | |second_author = and B. Dennis
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| - | |publish_date = 27 February 2012
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| - | |description = Slow waves, QPPs, and hard X-rays
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| - | |image = icon170.png}}
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| - | {{Nugget Badge
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| - | |title = RHESSI's Tenth Anniversary
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| - | |number = 169
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| - | |first_author = B. Dennis
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| - | |second_author = and R. Lin
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| - | |publish_date = 15 February 2012
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| - | |description = On RHESSI's tenth, a top-ten discovery list
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| - | |image = icon169.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = Supra-Arcade Downflows
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| - | |number = 168
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| - | |first_author = S. Savage
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| - | |second_author = and D. McKenzie
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| - | |publish_date = 23 January 2012
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| - | |description = A re-interpretation of the famous SAD tadpoles
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| - | |image = icon168.png}}
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| - | {{Nugget Badge
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| - | |title = Flare Observations of the EUV Continua
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| - | |number = 167
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| - | |first_author = R. Milligan
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| - | |second_author =
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| - | |publish_date = 16 January 2012
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| - | |description = The flare EUV continua now routinely observed
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| - | |image = icon167.png}}
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| - | {{Nugget Badge
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| - | |title = No Hard X-rays from Comet Lovejoy
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| - | |number = 166
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| - | |first_author = H. Hudson
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| - | |second_author = and P. Saint-Hilaire
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| - | |publish_date = 19 December 2011
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| - | |description = An amazing sungrazing comet, but not detectable at high energies
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| - | |image = icon166.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = Modelling spatially resolved X-ray polarization
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| - | |number = 165
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| - | |first_author = N. Jeffrey
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| - | |second_author = and E. Kontar
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| - | |publish_date = 12 December 2011
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| - | |description = Spatial distribution of X-ray polarization, and its implications
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| - | |image = icon165.png}}
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| - |
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| - | {{Nugget Badge
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| - | |title = Slowly but surely towards the huge amount of energy II
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| - | |number = 164
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| - | |first_author = S. Kołomański
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| - | |second_author = and T. Mrozek
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| - | |publish_date = 28 November 2011
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| - | |description = Analysis of the huge energies of loop-top sources in flares
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| - | |image = icon164.png}}
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| - | {{Nugget Badge
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| - | |title = X-ray and H-alpha Flare Impulses
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| - | |number = 163
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| - | |first_author = K. Radziszewski
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| - | |second_author = and P. Rudawy
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| - | |publish_date = 14 November 2011
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| - | |description = Strikingly precise correlations of H-alpha kernels and hard X-ray bursts
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| - | |image = icon163.jpg}}
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| - |
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| - | {{Nugget Badge
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| - | |title = Slowly but surely towards the huge amount of energy I
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| - | |number = 162
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| - | |first_author = Urszula Bąk-Stęślicka
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| - | |second_author = and Tomasz Mrozek, Sylwester Kołomański
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| - | |publish_date = 31 October 2011
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| - | |description = The energetics of "slow LDEs"
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| - | |image = icon162.png}}
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| - | {{Nugget Badge
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| - | |title = Quasi-Periodic Pulsations: Fermi/GBM Results
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| - | |number = 161
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| - | |first_author = David Gruber
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| - | |second_author = and Pawel Lachowicz
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| - | |publish_date = 24 October 2011
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| - | |description = Dealing with red noise
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| - | |image = icon161.png}}
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| - | {{Nugget Badge
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| - | |title = A Flare in 3D
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| - | |number = 160
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| - | |first_author = Hugh Hudson
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| - | |second_author = and Juan Carlos Martinez Oliveros
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| - | |publish_date = 10 October 2011
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| - | |description = Solar astrometry in 3D
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| - | |image = icon160.gif}}
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| - | {{Nugget Badge
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| - | |title = Solar Max Arrives
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| - | |number = 159
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| - | |first_author = Hugh Hudson
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| - | |second_author = and Richard Schwartz
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| - | |publish_date = 28 September 2011
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| - | |description = Seven X-class flares already in 2011
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| - | |image = icon159.png}}
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| - | {{Nugget Badge
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| - | |title = Two-stage SEE Shows Reconnection
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| - | |number = 158
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| - | |first_author = Yang Su
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| - | |second_author = and Brian Dennis
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| - | |publish_date = 8 September 2011
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| - | |description = Reconnection late in a flare
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| - | |image = icon158.png}}
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| - | {{Nugget Badge
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| - | |title = Scattered Light: Inverse Compton Scattering and Coronal Hard X-ray Sources
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| - | |number = 157
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| - | |first_author = B. Chen
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| - | |second_author = and T. S. Bastian
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| - | |publish_date = 17 August 2011
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| - | |description = Inverse Compton radiation - gaining momentum
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| - | |image = icon157.png}}
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| - | {{Nugget Badge
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| - | |title = X-ray, EUV & WL emission heights observed by RHESSI & SDO
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| - | |number = 156
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| - | |first_author = Marina Battaglia
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| - | |second_author = and Eduard Kontar
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| - | |publish_date = 24 July 2011
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| - | |description = A first - the relative height of hard X-ray and white-light flare sources
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| - | |image = icon156.png}}
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| - | {{Nugget Badge
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| - | |title = Hard X-rays and Sympathy
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| - | |number = 155
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| - | |first_author = Hugh Hudson
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| - | |second_author =
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| - | |publish_date = 13 July 2011
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| - | |description = A hard X-ray spike elicits a sympathetic response
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| - | |image = icon155.png}}
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| - | {{Nugget Badge
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| - | |title = Suzaku Microflares
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| - | |number = 154
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| - | |first_author = S. Ishikawa
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| - | |second_author =
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| - | |publish_date = 30 June 2011
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| - | |description = Microflares too have powerful particle acceleration
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| - | |image = icon154.png}}
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| - | {{Nugget Badge
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| - | |title = Acceleration without Heating
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| - | |number = 153
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| - | |first_author = G. Fleishman &
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| - | |second_author = E. Kontar
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| - | |publish_date = 13 June 2011
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| - | |description = Strong hard X-rays and weak soft X-rays - breaking the paradigm?
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| - | |image = icon153.png}}
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| - | {{Nugget Badge
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| - | |title = DIY spectroscopy: Analyzing AIA diffraction patterns
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| - | |number = 152
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| - | |first_author = C. L. Raftery &
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| - | |second_author = S. Krucker
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| - | |publish_date = 30 May 2011
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| - | |description = Imaging spectroscopy in the EUV, at AIA resolution
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| - | |image = icon152.png}}
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| - | {{Nugget Badge
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| - | |title = EVE/ESP and the Neupert Effect
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| - | |number = 151
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| - | |first_author = H. Hudson
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| - | |second_author =
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| - | |publish_date = 9 May 2011
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| - | |description = The Neupert Effect works, sort of, in a limb gamma-ray flare
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| - | |image = icon151.png}}
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| - | {{Nugget Badge
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| - | |title = Decimetric pulsations and coronal X-ray sources
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| - | |number = 150
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| - | |first_author = A. Benz,
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| - | |second_author = M. Battaglia, and N. Vilmer
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| - | |publish_date = 18 April 2011
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| - | |description = Radio pulsations may illuminate a strongly non-radial current sheet
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| - | |image = icon150.png}}
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| - | {{Nugget Badge
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| - | |title = The Alfven Speed above a Sunspot, and Gamma-rays
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| - | |number = 149
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| - | |first_author = H. Hudson
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| - | |second_author = and L. Fletcher
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| - | |publish_date = 12 April 2011
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| - | |description = Flare effects in sunspot umbrae
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| - | |image = icon149.png}}
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| - | {{{Nugget Badge
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| - | |title = Slow Magnetoacoustic Waves in Two-Ribbon Flares
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| - | |number = 148
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| - | |first_author = V. Nakariakov
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| - | |second_author = and I. Zimovets
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| - | |publish_date = 17 March 2011
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| - | |description = Wave dynamics explains arcade development
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| - | |image = icon148.png}}
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| - | {{Nugget Badge
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| - | |title = First Sunquake of Solar Cycle 24 Observed by Solar Dynamics Observatory
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| - | |number = 147
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| - | |first_author = A. G. Kosovichev
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| - | |second_author =
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| - | |publish_date = 7 March 2011
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| - | |description = An X-class flare - and a sunquake
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| - | |image = icon147.png}}
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| - | {{Nugget Badge
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| - | |title = M is for Magnifique Part Deux
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| - | |number = 146
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| - | |first_author = Steven Christe
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| - | |second_author = and Andrew Inglis
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| - | |publish_date = 22 February 2011
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| - | |description = A type II radio burst but no CME and introducing a new way to search for waves in SDO. (CORRECTION There is a CME!)
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| - | |image = icon146.png}}
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| - | {{Nugget Badge
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| - | |title = At last, the EUV Spectrum
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| - | |number = 145
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| - | |first_author = Hugh Hudson
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| - | |second_author =
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| - | |publish_date = 8 February 2011
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| - | |description = The main flare radiated energy is not in the EUV
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| - | |image = icon145.png}}
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| - | {{Nugget Badge
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| - | |title = Black and White Flares
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| - | |number = 144
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| - | |first_author = Juan Carlos Martinez Oliveros
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| - | |second_author = and Charles Lindsey
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| - | |publish_date = 24 January 2011
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| - | |description = HMI sees a black-light flare (?)
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| - | |image = icon144.png}}
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| - | {{Nugget Badge
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| - | |title = The Flares of the RHESSI Monograph
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| - | |number = 143
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| - | |first_author = Hugh Hudson
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| - | |second_author = and Gordon Emslie
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| - | |publish_date = 11 January 2011
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| - | |description = The top ten RHESSI flares thus far
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| - | |image = icon143.png}}
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| - | {{Nugget Badge
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| - | |title = Brilliant Timing
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| - | |number = 142
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| - | |first_author = Säm Krucker
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| - | |second_author = and Hugh Hudson
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| - | |publish_date = 20 December 2010
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| - | |description = Hinode and RHESSI observations strain the credibility of the thick-target model
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| - | |image = icon142.png}}
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| - | {{Nugget Badge
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| - | |title = M is for Magnifique
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| - | |number = 141
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| - | |first_author = Steven Christe
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| - | |second_author = and Andrew Inglis
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| - | |publish_date = 6 December 2010
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| - | |description = RHESSI and SDO see a remarkable flare
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| - | |image = icon141.png}}
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