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"Impulse Response Flares" and Gamma Rays"Superflares" on solar-type stars observed with Kepler2000
200120022005 RHESSI Science Nuggets
2006 RHESSI Science Nuggets2007 RHESSI Science Nuggets2008 RHESSI Science Nuggets
2009 RHESSI Science Nuggets2010 RHESSI Science Nuggets2011 RHESSI Science Nuggets
2012-05-29 Lunar Occultation2012-05-30 SAS observation of Venus Transit 20122012-06-22 Browser tips
2012-10-31 Elemental Abundances2012-10-31 GOES M9 Flare2012-12-12 Detector 4 Segmented
2012 RHESSI Science Nuggets2013-02-27 Detector 2 Front Slow Threshold Changes2013-03-13 Detector 2 spectral behavior
2013-03-20 Partial Segmentation and Splitting of the Annihilation Line2013-04-17 Detector 9 weirdness
2013-05 X flares2013-06-05 Cryocooler balancing2013-06-05 Detector 9 update
2013-06-12 Spin rate anomalies2013-06-19 Spin rates and detector temperatures2013-08-14 May 13 EMDs
2013-08-21 Kappa distribution in 2013 May 12 flare2013-08-28 HMI/RHESSI 2012 Nov 20 flare
2013 RHESSI Science Nuggets2014 RHESSI Science Nuggets2015 RHESSI Science Nuggets
2016 RHESSI Science Nuggets2017 RHESSI Science Nuggets2018 RHESSI Science Nuggets
2019 RHESSI Science Nuggets3D Magnetic Reconnection at a Coronal Null Point3pow - Triple Power Law
A (The?) 3D standard model for eruptive flaresA Bad Time for Flares but a Good Time for DebrisA Cool Star Flare Reveals an Unexpectedly Hot Emission Component
A Curious Sunspot Group in 2018A Flare in 3DA Lasso Model for Solar Gamma-ray Events
A New Day DawnsA Pion EventA Record-Setting CMEless Flare
A STEREO/RHESSI Flare at Solar MinimumA Shocking Type IIA Solar Hard X-Ray Halo: Exploring the Quiet Sun 2
A Sunspot from Cycle 25 for sureA Two-ribbon White-light Flare Associated with a Failed Solar EruptionA Wonderful Cycle 24 Flare
A flare in the deep solar atmosphereA hard wee flare observed with RHESSI and Hinode/XRTA huge gamma-ray burst
A lasso model for gamma raysA last best active regionA myriad of microflares
A new development in the Frost-Dennis paradigmA remarkable, but confused, coronal hard X-ray sourceA solar X-ray dentist mirror
A tiny white-light flareAbove-the-Looptop SourcesAbundances in Solar Flares
Acceleration-region DensitiesAcceleration of fast halo CMEs & synchronized flare HXR burstsAcceleration without Heating
Albedo and the modification of RHESSI resultsAll RHESSI Science NuggetsAlphabetic List of Data Access Commands
Alternatives to IDLAn Alternative View of the Masuda FlareAn Fe Cascade
An Unreported White-light ProminenceAn energetic pre-flare
An energetic pre-flare: electron distributions in magnetic reconnection outflowsAn energetic pre-flare and kappa electron distribution in magnetic reconnection outflowAnisotropy of RHESSI hard X-ray emission
AnnealingAnnealing RHESSI for the first timeAnnihilation of Positrons
Antipodal FlaresAre stellar flares like solar flares?At last, the EUV Spectrum
AttenuatorsAttitude Control SystemAwesome Stellar Flare Spectra
BARREL Balloon Observations and HistoryBack from the Far SideBastille Day 2017
Bastille day encore 2005Birth of a dense flaring loopBlack and White Flares
Blind Image AnalysisBlue-wing enhancement of the Mg II h and k lines in a flareBouncing Thick-Target Coronal X-Ray Sources
Bpow - Broken Power LawBrilliant TimingBroken-up hard X-ray spectra found for a loop-top source during a solar limb flare
Browse the RHESSI data!Burst-on-Tail (BOT)But there was a bigger one
CMEless FlaresCMEs on young, solar-type starsCORONAS/SPIRIT Mg XII and Nanoflares
Chree Analysis for FlaresChromospheric Plasma Parameters
CleanClean and UV Smooth Images Changing Image CentersCloudy SolarSoftware
Collapsing TrapsComplementary Data AccessConfined Flares versus Eruptive Flares
Coronal Hard X-ray Sources RevisitedCoronal gamma-ray sources in giant solar flaresCoronal hard X-rays and gamma-rays
Coronal implosionCoronal nanoflares powered by footpoint reconnectionCreate Article
Creating a Spectrum File Using the HESSI GUICryocooler
Cycle 24Cycle 24 - don't panic yet!Cycle 24 - time to panic
Cycle 24 Flares BeginCycle 24 has begunCycle 25 Strikes Again
DIB-table-2015-May-27DIB Table
DIB table 2015-Sep-23DIB table 2015 Aug 25DIB table 2015 Aug 5
DIB table 2015 Sep 22DIB table 2016-May-12DIB table 2016-May-4
DIY spectroscopy: Analyzing AIA diffraction patternsDaily solar mm-observations at Aalto University Metsähovi Radio ObservatoryData-driven radiative hydrodynamic modeling of SOL2014-03-29
DecimationDecimetric pulsations and coronal X-ray sourcesDense Loop Flares
Detector 1Detector 1 anneal 2012Detector 2
Detector 2 anneal 2012Detector 3Detector 3 anneal 2012
Detector 4Detector 4 anneal 2012Detector 5
Detector 5 anneal 2012Detector 6Detector 6 anneal 2012
Detector 7Detector 7 anneal 2012Detector 8
Detector 8 anneal 2012Detector 9Detector 9 anneal 2012
Detector Source CentroidsDetectors
Dimmings and Sustained Gamma-Ray Events
Dips and WavesDissauer et al. (2016)
Do Kepler Superflare Stars Really Include Slowly Rotating Sun-like Stars?Do slow waves trigger pulsations in two-ribbon flares? An observational searchDo solar decimetric spikes originate in coronal X-ray sources?
Double Coronal Hard X-ray SourceDouble Coronal X-ray and Microwave Sources Associated With A Magnetic Breakout Solar Eruption
Drm mod - Pseudo function for fine tuning RHESSI DRM parametersDynamic Processes of the Moreton Wave on 2014 March 29EIT Waves - Cadence issues
EOVSA Coverage of a Recent Gamma-Ray FlareEUNIS Sees Pervasive Faint Fe XIX Emission: Evidence for Nanoflare HeatingEVE-RHESSI DEM Models and the Low-energy Cutoff for Nonthermal Electrons
EVE/ESP and the Neupert EffectEVE Observations of Flare FootpointsEdward Chupp
Electric Current Neutralization and Solar Eruption in Active RegionsElectron Scattering in the Flaring CoronaElectron acceleration and hard X-ray emission from SOL2013-11-09
Electron beam anisotropy during precipitation info a flaring atmosphereElectron re-acceleration and HXR emissionElementary Flares
Emission LinesEmpirical Constructs and CartoonsEnergy Partition in Large Solar Eruptive Events
Energy goes up... but doesn't come back down! Coronal heating?Energy goes up... but doesn't come back down! Photospheric energy drives atmospheric heatingExploring the Quiet Sun 1
Extreme events, stellar evolution, and magnetic reconnectionFOXSI-2 LaunchFOXSI Success
Faculae and microflaresFast electron recombination: a neglected HXR sourceFast electrons relaxing
Fe XIX and Pervasive Nanoflare HeatingFine Structure in Flare Soft X-ray Light CurvesFirst Sunquake of Solar Cycle 24 Observed by Solar Dynamics Observatory
Fit function componentsFitting a new detectorFitting multiple intervals
Flare-induced Impulsive Sunspot Rotation caught in High ResolutionFlare Coronal RainFlare Heating by Mildly Non-thermal Particles
Flare Loop AsymmetriesFlare NimbusFlare Observations of the EUV Continua
Flare Observed by a Dozen InstrumentsFlare Plasma Abundances - New X-ray ObservationsFlare Productivity
Footpoint motions and what we can learn from themFree-bound continuum: basicsGOES Hard X-rays?
Gamma rays and Doppler shiftsGdlGlasgow Callisto and CMEless type II bursts
Glasgow Callisto optimistic: first light comes in focusGridsGround Stations
HESSI and Type III Radio BurstsHard X-ray Directivity Measurements with STIX and MiSolFAHard X-ray Emission along H-alpha Ribbons
Hard X-ray Emission from Partially Occulted Solar FlaresHard X-ray Footpoint AsymmetryHard X-ray Polarimetry from Tian Gong 2
Hard X-ray Pulsations in FlaresHard X-ray Spikes Observed by RHESSIHard X-rays and Sympathy
Hard X-rays from a jet?Hard X-rays in DescentHarmonic Oscillations
Hessi color table
High-energy Electrons and Electric Currents during a FlareHigh Dispersion Spectroscopy of solar-type superflare starsHigh Energies in the Inner Heliosphere
High Resolution Temporal and Spatial Structure of a White Light FlareHigh Temperatures in Active RegionsHighly significant detection of solar neutrons
Hinode/SOT Observations of Flare RibbonsHistory of Solar OblatenessHoming in on Flare Energy
Homologous CME/flares from AR 12371Homologous White Light Solar FlaresHow does RHESSI make images?
How to better determine the power in non-thermal electrons from observed X-ray spectraHow to correctly determine the power in non-thermal electrons from observed X-ray spectraHsi flare list fill: How the RHESSI Flare List is Generated
Hunting for Hidden Tiny FlaresIDLDE 7.1 or 7.1.1 PatchIDL Command: vso files
IDL Command: vso prepIDL Command: vso searchImage
Imaging - First StepsImaging Quasi-Periodic Oscillations in a Simple FlareImaging Techniques: Tips, Tricks, and Issues
Imaging through visibility interpolation: uv-smoothImplosion and Oscillation
Initiation of a type II radio burst without a CMEInstantaneous Flare PropertiesInverse Compton X-rays from relativistic flare leptons
Ionospheric Effects, Flare History, and Dick DonnellyIs the coronal magnetic field braiding?John Brown and the thick-target model
Joint MinXSS and RHESSI Flare X-ray Spectra between 1 and 15 keVJust how bursty is X-ray data?KW-Sun: The Konus/WIND Hard X-ray Solar Flare Database
Kappa DistributionKernels and RibbonsKristian Birkeland
Late-phase particle accelerationLine - GaussianLinear Polarization in H-alpha Flares
Localized Microwave and EUV Bright Structures in an Eruptive ProminenceLog for tohban anomaliesM Dwarf Flare Spectra in the Near-UV from the Hubble Space Telescope
M is for MagnifiqueM is for Magnifique Part DeuxMagnetic fields in active regions
Main PageMajor Flare Watch EvaluationMars Odyssey/HEND and RHESSI
Masuda flareMicroflares in SectorsMicrowave Emission from Twisted Magnetic Fields
Microwave Images of a Single-Loop Flare: Observations and SimulationsMicrowave Imaging Spectroscopy of Flares is HereMinXSS and RHESSI measure flare spectra over 1-15 keV
MinoflaresModelling spatially resolved X-ray polarizationMulti-Instrument Solar Flare Observations I: Solar Flare Finder
Multi-Instrument Solar Flare Observations II: A SC24 retrospectiveMulti-thermal delays
Multiple Regions of Shock-accelerated Particles during a Solar Coronal Mass EjectionMysteries of Flare/CME InitiationNarrowband radio signal correlated with early hard X-ray flux during a microflare
Negative Microwave BurstsNeutron Production in Solar FlaresNeutron starquake shakes RHESSI
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