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- 21:29, 13 February 2012 (diff | hist) Do slow waves trigger pulsations in two-ribbon flares? An observational search
- 21:29, 13 February 2012 (diff | hist) Do slow waves trigger pulsations in two-ribbon flares? An observational search
- 21:27, 13 February 2012 (diff | hist) N File:Pulse cartoon ainglis v5.jpg (Cartoon showing the progression of slow waves along a two-ribbon arcade.) (top)
- 21:25, 13 February 2012 (diff | hist) N Do slow waves trigger pulsations in two-ribbon flares? An observational search (Created page with " ===Introduction=== A recent study by Nakariakov & Zimovets (2011), which was the subject of a recent RHESSI nugget, suggested that quasi-periodic pulsations (QPP) might be exp...")
- 20:35, 17 February 2011 (diff | hist) m M is for Magnifique Part Deux
- 20:28, 17 February 2011 (diff | hist) m M is for Magnifique Part Deux
- 20:27, 17 February 2011 (diff | hist) m M is for Magnifique Part Deux
- 20:15, 17 February 2011 (diff | hist) M is for Magnifique Part Deux
- 19:42, 17 February 2011 (diff | hist) M is for Magnifique Part Deux
- 19:37, 17 February 2011 (diff | hist) N File:Nugget maps.jpg (top)
- 16:17, 15 February 2011 (diff | hist) M is for Magnifique Part Deux
- 16:11, 15 February 2011 (diff | hist) N File:Rhessi goes 16 oct 2010.jpg (top)
- 21:19, 14 February 2011 (diff | hist) M is for Magnifique Part Deux
- 19:30, 14 February 2011 (diff | hist) M is for Magnifique Part Deux
- 19:26, 14 February 2011 (diff | hist) N File:Cor map1600.jpg (top)
- 19:25, 14 February 2011 (diff | hist) N File:Cor map304.jpg (top)
- 19:24, 14 February 2011 (diff | hist) N File:Cor map171.jpg (top)
- 19:14, 14 February 2011 (diff | hist) m M is for Magnifique Part Deux
- 19:13, 14 February 2011 (diff | hist) M is for Magnifique Part Deux
- 19:10, 14 February 2011 (diff | hist) N File:Ribbon 171 304.jpg (top)
- 18:59, 14 February 2011 (diff | hist) M is for Magnifique Part Deux
- 19:40, 30 November 2010 (diff | hist) m M is for Magnifique (→Intro to AIA)
- 17:01, 30 November 2010 (diff | hist) M is for Magnifique (→Intro to AIA)
- 16:46, 30 November 2010 (diff | hist) M is for Magnifique (→Intro to AIA)
- 16:44, 30 November 2010 (diff | hist) N File:Sdo wavelengths.png
- 16:37, 30 November 2010 (diff | hist) M is for Magnifique
- 15:16, 14 July 2010 (diff | hist) N Talk:Harmonic Oscillations (New page: We are still investigating the effect we are reporting on in this Nugget, and it grows more interesting by the day. It in fact turns out that for the flare of 6th November 2004, the modula...) (top)
- 08:46, 18 May 2009 (diff | hist) m Hard X-ray Pulsations in Flares
- 10:52, 15 May 2009 (diff | hist) m Hard X-ray Pulsations in Flares
- 10:46, 15 May 2009 (diff | hist) Hard X-ray Pulsations in Flares
- 10:43, 15 May 2009 (diff | hist) Hard X-ray Pulsations in Flares
- 10:37, 15 May 2009 (diff | hist) Hard X-ray Pulsations in Flares
- 10:36, 15 May 2009 (diff | hist) Hard X-ray Pulsations in Flares
- 10:33, 15 May 2009 (diff | hist) Hard X-ray Pulsations in Flares
- 10:31, 15 May 2009 (diff | hist) Hard X-ray Pulsations in Flares
- 10:26, 15 May 2009 (diff | hist) Hard X-ray Pulsations in Flares
- 09:51, 15 May 2009 (diff | hist) Hard X-ray Pulsations in Flares
- 09:40, 15 May 2009 (diff | hist) Hard X-ray Pulsations in Flares
- 09:38, 15 May 2009 (diff | hist) Hard X-ray Pulsations in Flares
- 09:36, 15 May 2009 (diff | hist) Hard X-ray Pulsations in Flares
- 09:24, 15 May 2009 (diff | hist) Hard X-ray Pulsations in Flares
- 09:21, 15 May 2009 (diff | hist) Hard X-ray Pulsations in Flares
- 09:17, 15 May 2009 (diff | hist) Hard X-ray Pulsations in Flares
- 09:06, 15 May 2009 (diff | hist) N File:Nugget6.png (top)
- 09:05, 15 May 2009 (diff | hist) N File:Nugget5.png (top)
- 09:05, 15 May 2009 (diff | hist) N File:Nugget4.png (top)
- 09:04, 15 May 2009 (diff | hist) N File:Nugget3.png (top)
- 09:04, 15 May 2009 (diff | hist) N File:Nugget2.png (top)
- 09:03, 15 May 2009 (diff | hist) N File:Nugget1.png (top)
- 08:54, 15 May 2009 (diff | hist) N Hard X-ray Pulsations in Flares (New page: '''Introduction''' For several decades astronomers have observed curious oscillations and pulsations in the emission from solar flares. Collectively these are usually known as "quasi-peri...)
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