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- 10:05, 8 July 2014 (diff | hist) The Redistribution of Nonthermal Electron Energy (→Conclusions)
- 10:04, 8 July 2014 (diff | hist) The Redistribution of Nonthermal Electron Energy (→Flare Energies)
- 10:00, 8 July 2014 (diff | hist) The Redistribution of Nonthermal Electron Energy (→Conclusions)
- 09:59, 8 July 2014 (diff | hist) The Redistribution of Nonthermal Electron Energy
- 09:54, 8 July 2014 (diff | hist) N File:20110215 lam flam.png (top)
- 09:53, 8 July 2014 (diff | hist) N File:20110215 flam.png (top)
- 16:32, 7 July 2014 (diff | hist) The Redistribution of Nonthermal Electron Energy
- 16:32, 7 July 2014 (diff | hist) The Redistribution of Nonthermal Electron Energy
- 16:30, 7 July 2014 (diff | hist) The Redistribution of Nonthermal Electron Energy
- 16:22, 7 July 2014 (diff | hist) The Redistribution of Nonthermal Electron Energy
- 16:20, 7 July 2014 (diff | hist) The Redistribution of Nonthermal Electron Energy
- 16:14, 7 July 2014 (diff | hist) N File:20110215 lam flam log.png (top)
- 16:13, 7 July 2014 (diff | hist) N File:20110215 lam flam linear.png (top)
- 16:10, 7 July 2014 (diff | hist) The Redistribution of Nonthermal Electron Energy
- 16:01, 7 July 2014 (diff | hist) The Redistribution of Nonthermal Electron Energy
- 15:55, 7 July 2014 (diff | hist) N File:Hsi eve aia sot ltc v4.png (top)
- 15:49, 7 July 2014 (diff | hist) The Redistribution of Nonthermal Electron Energy
- 15:47, 7 July 2014 (diff | hist) The Redistribution of Nonthermal Electron Energy
- 15:44, 7 July 2014 (diff | hist) N File:Chianti flare spec coverage.png (top)
- 15:43, 7 July 2014 (diff | hist) The Redistribution of Nonthermal Electron Energy
- 15:41, 7 July 2014 (diff | hist) N The Redistribution of Nonthermal Electron Energy (Created page with " Introduction It is widely accepted that the hard X-ray emission that RHESSI observes come from thick-target interactions between accelerated electrons and the dense chromosphere...")
- 15:26, 21 May 2012 (diff | hist) m Time Profiles of Solar Flare Densities
- 15:25, 21 May 2012 (diff | hist) m Time Profiles of Solar Flare Densities
- 15:23, 21 May 2012 (diff | hist) m Time Profiles of Solar Flare Densities
- 14:01, 21 May 2012 (diff | hist) m Time Profiles of Solar Flare Densities
- 13:57, 21 May 2012 (diff | hist) m Time Profiles of Solar Flare Densities
- 13:55, 21 May 2012 (diff | hist) m Time Profiles of Solar Flare Densities
- 13:53, 21 May 2012 (diff | hist) m Time Profiles of Solar Flare Densities
- 13:39, 21 May 2012 (diff | hist) File:Eve density fe xxi 20110809 nugget.png (uploaded a new version of "File:Eve density fe xxi 20110809 nugget.png") (top)
- 13:29, 21 May 2012 (diff | hist) Time Profiles of Solar Flare Densities
- 10:19, 21 May 2012 (diff | hist) Time Profiles of Solar Flare Densities
- 10:18, 21 May 2012 (diff | hist) Time Profiles of Solar Flare Densities
- 10:16, 21 May 2012 (diff | hist) Time Profiles of Solar Flare Densities
- 10:12, 21 May 2012 (diff | hist) Time Profiles of Solar Flare Densities
- 10:07, 21 May 2012 (diff | hist) Time Profiles of Solar Flare Densities
- 10:02, 21 May 2012 (diff | hist) N File:Eve density fe xxi 20110809 nugget.png (Electron density profiles from three Fe XXI line ratios during the X6.9 class flare on 2011 August 9. The top panel shows the GOES lightcurves for the event in the 0.5-4 and 1-8A channels, while the bottom three panels show the electron density time profi)
- 10:01, 21 May 2012 (diff | hist) N File:Eve flare lines.png (Plot of the 8-16 nm portion of the EVE spectra prior to the start of the X6.9 flare that occurred on 9 August 2011 (black curve) and at the SXR peak (red curve). Lines formed from transitions of highly-ionized iron are noted.) (top)
- 09:59, 21 May 2012 (diff | hist) N Time Profiles of Solar Flare Densities (Created page with "== Introduction == Solar flares are generally thought of as increases in X-ray luminosity on the Sun due to an increase in the temperature and density of the coronal plasma. The...")
- 14:06, 13 January 2012 (diff | hist) Flare Observations of the EUV Continua
- 13:59, 13 January 2012 (diff | hist) Flare Observations of the EUV Continua
- 13:48, 13 January 2012 (diff | hist) Flare Observations of the EUV Continua
- 13:32, 13 January 2012 (diff | hist) N File:Eve hsi goes plot.png (Top panel: lightcurves of free-free, free-bound, and bound-bound emission as observed by EVE during the 15 February 2011 flare. The vertical dashed lines in each panel denote the time of peak emission in each band. Also shown is the GOES 0.1-0.8 nm lightc) (top)
- 13:31, 13 January 2012 (diff | hist) Flare Observations of the EUV Continua
- 13:29, 13 January 2012 (diff | hist) File:Sample eve chianti flare spec.png (top)
- 13:28, 13 January 2012 (diff | hist) N File:Sample eve chianti flare spec.png (A sample of the EUV spectra from 6.5-105 nm taken with both the MEGS-A and MEGS-B components of EVE near the peak of the X2.2 flare that occurred on 15 February 2011. The locations of the recombination edges at 22.8, 50.4, and 91.2 nm are noted. Synthetic)
- 13:26, 13 January 2012 (diff | hist) N Flare Observations of the EUV Continua (Created page with " == Introduction == It has long been known that the bulk of the energy deposited in the chromosphere by non-thermal electrons during solar flares is re-radiated in the form of c...")
- 14:26, 24 March 2010 (diff | hist) Particle Acceleration due to a Plasmoid-Looptop Collision
- 14:25, 24 March 2010 (diff | hist) Particle Acceleration due to a Plasmoid-Looptop Collision
- 14:17, 24 March 2010 (diff | hist) Particle Acceleration due to a Plasmoid-Looptop Collision
- 14:15, 24 March 2010 (diff | hist) Particle Acceleration due to a Plasmoid-Looptop Collision
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