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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)
- 19:45, 18 September 2015 (diff | hist) m User talk:Bdennis (→Introduction: Edited text and renumbered references)
- 19:41, 18 September 2015 (diff | hist) m User talk:Bdennis (→References: Added Chamberlin reference and renumbered)
- 19:17, 18 September 2015 (diff | hist) m User talk:Bdennis (→SOL2015-: Edited header)
- 19:07, 18 September 2015 (diff | hist) m User talk:Bdennis (→References: Added Caspi et al.)
- 19:01, 18 September 2015 (diff | hist) m User talk:Bdennis (→Conclusions: Added text)
- 21:51, 17 September 2015 (diff | hist) m User talk:Bdennis
- 21:50, 17 September 2015 (diff | hist) m User talk:Bdennis (→References: Added Nakariakov reference)
- 21:22, 17 September 2015 (diff | hist) m User talk:Bdennis (→Conclusion: Added Conclusions)
- 20:57, 17 September 2015 (diff | hist) m User talk:Bdennis (→Introduction: Added links and names of previous Nuggets)
- 20:51, 17 September 2015 (diff | hist) m User talk:Bdennis (→SOL2013-10-23)
- 20:49, 17 September 2015 (diff | hist) m User talk:Bdennis
- 20:46, 17 September 2015 (diff | hist) m User talk:Bdennis (→SOL2013-10-23: New Figure 3)
- 20:40, 17 September 2015 (diff | hist) N File:Lc 28Oct2013 0152to0214 hsi 50to100keV GOESderiv EVEderiv.jpg (RHESSI, GOES, and EVE/ESP light curves for flare on 28 October 2013) (top)
- 20:37, 17 September 2015 (diff | hist) m User talk:Bdennis (Added links to EVE/ESP)
- 19:47, 17 September 2015 (diff | hist) m User talk:Bdennis (→Observations: Divided text by flare)
- 19:39, 17 September 2015 (diff | hist) m User talk:Bdennis (→Observations: Added link to EVE/ESP)
- 19:34, 17 September 2015 (diff | hist) m User talk:Bdennis (→Introduction: Added link to teh Neupert Effect)
- 19:25, 17 September 2015 (diff | hist) m User talk:Bdennis (→Observations: Added text)
- 18:00, 17 September 2015 (diff | hist) m User talk:Bdennis (→Observations)
- 17:56, 17 September 2015 (diff | hist) m User talk:Bdennis (→Observations: Superscripts)
- 16:05, 17 September 2015 (diff | hist) m User talk:Bdennis (→Heading 1: New Figure 2)
- 15:33, 17 September 2015 (diff | hist) N File:Lc 23July2002 0018to0035 hsi countflux 4s 6to1000keV d1 GOESderiv.jpg (RHESSI hard X-ray light curve and time derivative of GOES soft X-ray light curve of flare on 23 July 2002.) (top)
- 15:29, 17 September 2015 (diff | hist) m User talk:Bdennis (→Introduction: References to Figure 1)
- 15:08, 17 September 2015 (diff | hist) m User talk:Bdennis (→Introduction: GOES IDL Users Guide)
- 18:50, 10 September 2015 (diff | hist) m User talk:Bdennis (QPP links)
- 16:13, 10 September 2015 (diff | hist) m User talk:Bdennis (Figure 4)
- 16:10, 10 September 2015 (diff | hist) N File:Lc 11Mar2015161140to1700 GOES13&15deriv crosscorrelation.jpg (Time derivative of GOES 13 and 15 light curves with cross correlation plots for selected time intervals.)
- 16:08, 10 September 2015 (diff | hist) m User talk:Bdennis (Figure 3)
- 16:04, 10 September 2015 (diff | hist) N File:Lc 11Mar2015161140to1700 GOES13&15deriv.jpg (GOES13&15 Light curves for flare starting at 16:20 UT on 11 march 2015 (SOL2015-03-11).)
- 15:59, 10 September 2015 (diff | hist) m User talk:Bdennis (References)
- 15:37, 10 September 2015 (diff | hist) m User talk:Bdennis
- 15:32, 10 September 2015 (diff | hist) m User talk:Bdennis (Ref. 1)
- 15:25, 10 September 2015 (diff | hist) m User talk:Bdennis (Figures 1 and 2)
- 15:15, 10 September 2015 (diff | hist) m User talk:Bdennis (Figure 1)
- 15:01, 10 September 2015 (diff | hist) N File:Lc 28Oct3013 0152to0210 hsi 25to50to100to300keV GOES15deriv.jpg (RHESSI 25 to 300 keV and GOES time derivative light curves for flare at 01:52 UT on 28 October 2013.) (top)
- 21:59, 9 September 2015 (diff | hist) N File:Lc 23July2002 0017to0036 GOES logflux logderivative.jpg (GOES Flux and time derivative light curves for 23 July 2002) (top)
- 21:49, 9 September 2015 (diff | hist) m User talk:Bdennis
- 21:45, 9 September 2015 (diff | hist) m User talk:Bdennis
- 21:43, 9 September 2015 (diff | hist) m User talk:Bdennis
- 21:41, 9 September 2015 (diff | hist) Nm User talk:Bdennis (Introduction and Outline)
- 22:36, 11 September 2014 (diff | hist) m Which detectors can I use to analyze this flare? (Kim's typo finds corrected)
- 18:48, 11 September 2014 (diff | hist) m Which detectors can I use to analyze this flare? (Made Albert's changes and cleaned up references)
- 16:14, 11 September 2014 (diff | hist) m Which detectors can I use to analyze this flare? (Added References)
- 22:10, 10 September 2014 (diff | hist) m Which detectors can I use to analyze this flare? (Minor edits. Added last sentence.)
- 21:24, 10 September 2014 (diff | hist) m Which detectors can I use to analyze this flare? (Minor edits)
- 21:06, 10 September 2014 (diff | hist) m Which detectors can I use to analyze this flare? (→A1 Attenuator State (thin attenuators): Minor)
- 21:03, 10 September 2014 (diff | hist) m Which detectors can I use to analyze this flare? (→A1 Attenuator State (thin attenuators): Minor)
- 21:56, 9 September 2014 (diff | hist) m Which detectors can I use to analyze this flare? (Edited text and added Conclusions)
- 19:28, 9 September 2014 (diff | hist) m Which detectors can I use to analyze this flare? (→A0 Attenuator State (no attenuators): Minor edits)
- 18:33, 9 September 2014 (diff | hist) m Which detectors can I use to analyze this flare? (→Description of Plots: Minor edits)
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