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- 11:05, 24 April 2023 (diff | hist) m Did a Solar Flare Accelerate all the Ambient Electrons in the Coronal Acceleration Region?... (Changed /cc to cm<sup>-3</sup>) (top)
- 19:43, 5 August 2022 (diff | hist) m Fifty-year Anniversary of the First Detection of Gamma rays from a Solar Flare (→Conclusion: Minor punctuation changes.)
- 19:35, 5 August 2022 (diff | hist) m Fifty-year Anniversary of the First Detection of Gamma rays from a Solar Flare (→Solar γ rays: Deleted "particularly.")
- 19:33, 5 August 2022 (diff | hist) m Fifty-year Anniversary of the First Detection of Gamma rays from a Solar Flare (→Introduction: Caption revised.)
- 13:28, 1 October 2018 (diff | hist) m Coronal Hard X-ray Sources Revisited (→Results for Multiple Flares: Minor edits)
- 19:40, 28 September 2018 (diff | hist) m Coronal Hard X-ray Sources Revisited (→Example Flare - 14/15 April 2002: Added Ref. [4])
- 19:16, 28 September 2018 (diff | hist) m Coronal Hard X-ray Sources Revisited (→Results for Multiple Flares: Added Ref. 2,3,4,5,6.)
- 17:32, 28 September 2018 (diff | hist) m Coronal Hard X-ray Sources Revisited (→Source Length Determination: No change)
- 17:30, 28 September 2018 (diff | hist) m Coronal Hard X-ray Sources Revisited (→Source Length Determination: Delta D)
- 17:25, 28 September 2018 (diff | hist) m Coronal Hard X-ray Sources Revisited (→References: Edited Ref. 6.)
- 17:23, 28 September 2018 (diff | hist) m Coronal Hard X-ray Sources Revisited (→Introduction: Added links to Refs. 2,3,4,5,6.)
- 17:20, 28 September 2018 (diff | hist) m Coronal Hard X-ray Sources Revisited (→References: Added References 2 - 6)
- 14:32, 28 September 2018 (diff | hist) m Coronal Hard X-ray Sources Revisited (→Results for Multiple Flares: Removed Figures 1 - 6 and edited text)
- 14:20, 28 September 2018 (diff | hist) m Coronal Hard X-ray Sources Revisited (→Example Flare - 14/15 April 2002: Moved Figure 4, 5, and 6)
- 14:01, 28 September 2018 (diff | hist) m Coronal Hard X-ray Sources Revisited (→Example Flare - 14/15 April 2002: Moved Figure 3)
- 13:58, 28 September 2018 (diff | hist) m Coronal Hard X-ray Sources Revisited (→Example Flare - 14/15 April 2002: Moved Figure 2)
- 13:53, 28 September 2018 (diff | hist) m Coronal Hard X-ray Sources Revisited (→Example Flare - 14/15 April 2002: Moved Figure 1)
- 21:52, 26 September 2018 (diff | hist) m Coronal Hard X-ray Sources Revisited (→Example Flare - 14/15 April 2002: Added more text)
- 19:13, 26 September 2018 (diff | hist) m Coronal Hard X-ray Sources Revisited (→Example Flare - 14/15 April 2002: Added text)
- 22:16, 21 September 2018 (diff | hist) m Coronal Hard X-ray Sources Revisited (→Example Flare - 14/15 April 2002: Added Figures and text)
- 21:47, 21 September 2018 (diff | hist) File:Mem njit FW50M dLvsdD 20-30.jpg (uploaded a new version of "File:Mem njit FW50M dLvsdD 20-30.jpg": Changes in position (DeltaD) and length (DeltaL measured at 50% of the peak intensity) between 20 to 30 keV for the coronal sources for the 6 flares and 12 time intervals used) (top)
- 21:44, 21 September 2018 (diff | hist) N File:Mem njit FW50M dLvsdD 20-30.jpg (Changes in position (DeltaD) and length (DeltaL measured at 50% of the peak intensity) between 20 to 30 keV for the coronal sources for the 6 flares and 12 time intervals used in the study.)
- 21:29, 21 September 2018 (diff | hist) N File:Mem njit event3 dist.jpg.jpg (Energy dependence of the distance, D, between the peak in coronal flux in the 20-22 keV image and the peak at other energies. The solid lines show linear fits to the data points from 10 to 20 keV and 20 to 30 keV, and the indicated values of DeltaD are th) (top)
- 21:18, 21 September 2018 (diff | hist) N File:Mem njit event3 fwhm arc2.jpg (Coronal source length measured along the loop spine plotted vs. photon energy. The lengths were determined as the distances between the positions at which the intensity along the arc dropped to 75% (blue), 50% (orange), and 20% (red) of the peak value in ) (top)
- 21:06, 21 September 2018 (diff | hist) N File:Mem njit event3 gaussfit arc2.jpg (Normalized X-ray intensity vs. distance measured along the loop spine that pass through the coronal source peak location at each energy Color-coded points for each energy show the intensities at each pixel along the arc in the image. The curves are the su) (top)
- 20:27, 21 September 2018 (diff | hist) N File:Im 15april2002 000000to000500 hsi memnjit 12to25to50kev d3456.jpg (RHESSI 12 - 25 keV image (color-coded according to the color bar in units of photons cm^2 s^1 arcsec^2) overlaid with 25 - 50 keV contours (5, 10, 30, 50, 70, and 90% of the peak value) for the 5-min. interval from 00:00 to 00:05 UT made using the MEM NJI) (top)
- 22:29, 17 September 2018 (diff | hist) m Coronal Hard X-ray Sources Revisited (Added Figures 1 and 2)
- 22:24, 17 September 2018 (diff | hist) N File:Sp 15april2002 000000to000500 hsi mtpow thick2 albedo 5to60keV d4f.jpg (RHESSI count flux spectrum for the five-minute time interval shown in Figure 1. The black histogram is the background-subtracted count flux in the front segment of Detector #4. The red histogram is the function that was fitted to the data between 6 and 5) (top)
- 22:00, 17 September 2018 (diff | hist) N File:Lc 15April2002 hsi ql.jpg (RHESSI light curves for the flare on 15 April 2002. The color-coded curves are for the five indicated energy ranges. Counts from the front segments of all detectors except for detectors #2 and #7 were summed and divided by the summed live times and the t) (top)
- 21:30, 17 September 2018 (diff | hist) N Coronal Hard X-ray Sources Revisited (Initialization and Introduction)
- 23:41, 5 February 2018 (diff | hist) m MinXSS and RHESSI measure flare spectra over 1-15 keV (→Introduction: Added link to Ref.1. Do we reall need a reference to the RHESSI paper here?)
- 23:39, 5 February 2018 (diff | hist) m MinXSS and RHESSI measure flare spectra over 1-15 keV (→Joint observations of solar flares: Changed link to Ref. 1 to Ref.2. There is currently no link to Ref.1. I will add it to the first section.)
- 23:36, 5 February 2018 (diff | hist) m MinXSS and RHESSI measure flare spectra over 1-15 keV (→Conclusions: Minor editorial changes.)
- 23:21, 5 February 2018 (diff | hist) MinXSS and RHESSI measure flare spectra over 1-15 keV (→Joint observations of solar flares: Editorial changes. Moved all but the first sentence from figure caption to the main body of text. Corrected RHESSI's spectral range from 620 keV to 6 to 20 keV)
- 22:56, 5 February 2018 (diff | hist) m MinXSS and RHESSI measure flare spectra over 1-15 keV (→Introduction: Minor editorial changes. Added the number of RHESSI flares)
- 14:39, 3 March 2017 (diff | hist) m Edward Chupp (Minor edit)
- 22:49, 2 March 2017 (diff | hist) Nm Edward Chupp (Initital draft)
- 22:08, 2 March 2017 (diff | hist) N File:EdChupp.jpg (Edward Chupp Emeritus Professor Department of Physics, Professor Space Science Center (EOS) Physics) (top)
- 14:24, 15 February 2017 (diff | hist) m RHESSI's 15th Anniversary (Removed ",a highly successful SMEX mission," and made other minor changes)
- 15:42, 17 June 2016 (diff | hist) m RHESSI has resumed operations (Text changes)
- 14:06, 31 March 2016 (diff | hist) m An Unreported White-light Prominence (Removed RHESSI comment from caption of Fig. 1.)
- 23:17, 20 September 2015 (diff | hist) m User talk:Bdennis (→SOL2002-07-23: Changed 00:28 to ~00:29) (top)
- 23:15, 20 September 2015 (diff | hist) m User talk:Bdennis (→Introduction)
- 23:13, 20 September 2015 (diff | hist) m User talk:Bdennis (→Introduction: Added attenuator note in Figure 1 caption)
- 20:48, 20 September 2015 (diff | hist) m User talk:Bdennis (Corrected Section on SOL2015-03-11)
- 22:13, 18 September 2015 (diff | hist) m User talk:Bdennis (→SOL2013-10-23: Edited EVE/ESP link and other text)
- 21:57, 18 September 2015 (diff | hist) m User talk:Bdennis (→Introduction: Moved Figure 1 and reformated links to previous Nuggets)
- 21:52, 18 September 2015 (diff | hist) m User talk:Bdennis (Renumbered all references & changed Figure discussions in text)
- 21:18, 18 September 2015 (diff | hist) m User talk:Bdennis (→Introduction: Changed references to Figure 1)
- 19:48, 18 September 2015 (diff | hist) m User talk:Bdennis (→Conclusions: Renumbered references)
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