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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)
- 16:02, 9 September 2014 (diff | hist) m Which detectors can I use to analyze this flare? (Figure 1 removed and figures renumbered)
- 15:36, 9 September 2014 (diff | hist) m Which detectors can I use to analyze this flare? (→Introduction: Added link to .png files)
- 15:21, 9 September 2014 (diff | hist) m Which detectors can I use to analyze this flare? (→Description of Plots)
- 15:10, 9 September 2014 (diff | hist) m Which detectors can I use to analyze this flare? (→Introduction: Edited text)
- 14:34, 9 September 2014 (diff | hist) m Which detectors can I use to analyze this flare? (→A0 Attenuator State (no attenuators): Edited text)
- 14:19, 9 September 2014 (diff | hist) m Which detectors can I use to analyze this flare? (→Description of Plots: Edited text.)
- 22:50, 8 September 2014 (diff | hist) m Which detectors can I use to analyze this flare? (Consolidated discussion of three attenuator states)
- 22:37, 8 September 2014 (diff | hist) m Which detectors can I use to analyze this flare? (Added a fourth plot, renumbered figures, and edited text)
- 21:21, 8 September 2014 (diff | hist) m Which detectors can I use to analyze this flare? (Added a fourth plot and renumbered figures)
- 21:08, 8 September 2014 (diff | hist) N File:Hsi sepdet spectrum 20140903 133928to134028.png (Kim's latest version) (top)
- 21:01, 8 September 2014 (diff | hist) File:Hsi sepdet spectrum 20050120 065040to065140.png (uploaded a new version of "File:Hsi sepdet spectrum 20050120 065040to065140.png": Kim's latest version) (top)
- 20:59, 8 September 2014 (diff | hist) File:Hsi sepdet spectrum 20140903 025128to025228.png (uploaded a new version of "File:Hsi sepdet spectrum 20140903 025128to025228.png": Kim's latest version) (top)
- 20:56, 8 September 2014 (diff | hist) File:Hsi sepdet spectrum 20140502 005436to005536.png (uploaded a new version of "File:Hsi sepdet spectrum 20140502 005436to005536.png": Kim's latest version.) (top)
- 14:41, 8 September 2014 (diff | hist) m Which detectors can I use to analyze this flare? (Added link to K-shell decays rates)
- 22:28, 5 September 2014 (diff | hist) m Which detectors can I use to analyze this flare? (Added Example 2)
- 21:30, 5 September 2014 (diff | hist) N File:Hsi sepdet spectrum 20140903 025128to025228.png (Count flux and photon spectra for all individual detector front segments for flare on 03 September 2014.)
- 21:23, 5 September 2014 (diff | hist) m Which detectors can I use to analyze this flare? (Added text and bolded detector names)
- 17:00, 5 September 2014 (diff | hist) m Which detectors can I use to analyze this flare? (Added text)
- 16:02, 5 September 2014 (diff | hist) m Which detectors can I use to analyze this flare? (Added bullets)
- 15:53, 5 September 2014 (diff | hist) m Which detectors can I use to analyze this flare? (Added Nugget template and links)
- 21:43, 4 September 2014 (diff | hist) m Which detectors can I use to analyze this flare? (Added text)
- 16:01, 4 September 2014 (diff | hist) m Which detectors can I use to analyze this flare? (Added text)
- 13:36, 4 September 2014 (diff | hist) m Which detectors can I use to analyze this flare? (Added text and Figure 2)
- 13:15, 4 September 2014 (diff | hist) N File:Hsi sepdet spectrum 20050120 065040to065140.png (All detector front segment count and photon flux spectra during big X-class flare on 20 January 2005.)
- 22:51, 3 September 2014 (diff | hist) m Which detectors can I use to analyze this flare? (Added text.)
- 22:33, 3 September 2014 (diff | hist) Which detectors can I use to analyze this flare? (Added Figure 1)
- 22:29, 3 September 2014 (diff | hist) N File:Hsi sepdet spectrum 20140502 005436to005536.png (Individual detector count and photon flux spectra.)
- 22:09, 3 September 2014 (diff | hist) N Which detectors can I use to analyze this flare? (Started a Nugget)
- 21:43, 28 July 2014 (diff | hist) m Flare Observed by a Dozen Instruments (→Conclusions)
- 12:54, 15 July 2014 (diff | hist) m The Redistribution of Nonthermal Electron Energy (→Conclusions: Two typo errors)
- 16:21, 6 July 2014 (diff | hist) m RHESSI is Annealing Now (→The current anneal: Added reference to Fermi GBM.)
- 16:08, 6 July 2014 (diff | hist) m RHESSI is Annealing Now (→Introduction: Chnaged "room temperature" to "about 100 degrees Centigrade.")
- 21:18, 1 May 2014 (diff | hist) m Tohban (→Tohban Context Tool: Added link to daily SOH plots page.)
- 21:03, 1 May 2014 (diff | hist) Annealing (Edited text, corrected and added anneal dates and times and link to all offpoint and anneal times.) (top)
- 20:08, 1 May 2014 (diff | hist) Tohban (Added links to Categories and 1-day Averages pages)
- 22:18, 5 October 2012 (diff | hist) m Energy Partition in Large Solar Eruptive Events (Reformatted table)
- 22:14, 5 October 2012 (diff | hist) m Energy Partition in Large Solar Eruptive Events (→Data Reduction)
- 22:04, 5 October 2012 (diff | hist) m Energy Partition in Large Solar Eruptive Events (→Data Reduction: Minor tweaks)
- 21:47, 5 October 2012 (diff | hist) m Energy Partition in Large Solar Eruptive Events (→Introduction)
- 21:45, 5 October 2012 (diff | hist) m Energy Partition in Large Solar Eruptive Events (Minor tweaks.)
- 21:20, 14 February 2012 (diff | hist) m RHESSI's Tenth Anniversary (→RHESSI's Scientific Legacy: Added link to "High-energy Apsects of Solar Flares.")
- 20:56, 14 February 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Number 7: HXR Flare Ribbons: Removed "[" from Fletcher reference.)
- 20:51, 14 February 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Number 1: Discovery of Gamma-ray Footpoint Structures: Edited figure caption.)
- 20:50, 14 February 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Number 8: Location of Superhot X-ray source: Edited text.)
- 20:38, 14 February 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Number 2: Energy Content & Spectrum of Flare Energetic Electrons: Edited text. Replaced Holman et al. (2011) with Holman et al. (2003).)
- 20:18, 14 February 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Number 1: Discovery of Gamma-ray Footpoint Structures: Edited text.)
- 15:43, 13 February 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Flare Discoveries: "Discoveries" to "Contributions")
- 15:38, 13 February 2012 (diff | hist) m RHESSI's Tenth Anniversary (→The Flare Discoveries: Minor)
- 20:47, 9 February 2012 (diff | hist) m RHESSI's Tenth Anniversary (→RHESSI's Scientific Legacy: Added references)
- 20:29, 9 February 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Extras: removed this section)
- 20:27, 9 February 2012 (diff | hist) m RHESSI's Tenth Anniversary (→RHESSI's Scientific Legacy: Removed reference to "a RHESSI inspired monograph.")
- 20:22, 9 February 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Nonthermal Emissions from the Corona: combined text - simplified references.)
- 20:20, 9 February 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Nonthermal Emissions from the Corona: combined text - simplified references.)
- 23:33, 8 February 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Non-flare Related Items: Minor)
- 23:29, 8 February 2012 (diff | hist) m RHESSI's Tenth Anniversary (→RHESSI's Scientific Legacy: minor)
- 20:26, 8 February 2012 (diff | hist) m RHESSI's Tenth Anniversary (→RHESSI's Scientific Legacy: Rearranged order of list and rewrote opeing section)
- 15:23, 6 February 2012 (diff | hist) m RHESSI's Tenth Anniversary (→RHESSI's Scientific Legacy: Added section on Energy Content & Spectrum of Flare Energetic Electrons)
- 15:14, 6 February 2012 (diff | hist) N File:Massoneetal2 2004.jpg (Source electron flux spectra corresponding to the angle θo, the angle between the observer and the electron beam direction, for the electrons filling a semi-angle of α about the beam direction. Thus, α = 180 is an isotropic electron distribution. (Mass) (top)
- 15:11, 6 February 2012 (diff | hist) N File:Massoneetal1 2004.jpg (X-ray photon flux spectra for the time interval (01:39:04–01:39:48 UT) during the 2002 August 21 flare. This spectrum was obtained by processing the RHESSI count spectrum through the SPEX software on the Solar Software tree and is robust in the count/ph) (top)
- 20:06, 5 February 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Imaging the Acceleration Region: Bulk Energization: Added references)
- 19:34, 5 February 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Imaging the Acceleration Region: Bulk Energization: Added figure)
- 19:29, 5 February 2012 (diff | hist) N File:Kruckeretal2011.jpg (Example of X-ray imaging of a limb flare. The dark green line is the optical solar limb. The thermal flare loop is shown in red. A single HXR source visible at the limb (in blue) is identified as a footpoint with the second footpoint occulted behind the l) (top)
- 19:20, 5 February 2012 (diff | hist) m RHESSI's Tenth Anniversary (Added section on Imaging the Acceleration Region: Bulk Energization)
- 19:14, 5 February 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Nonthermal Emissions from the Corona: Minor)
- 19:13, 5 February 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Coronal hard X-rays sources: Replaced text and references)
- 18:59, 5 February 2012 (diff | hist) m RHESSI's Tenth Anniversary (Replaced Multiple Footpoints section with HXR Ribbons Section)
- 18:52, 5 February 2012 (diff | hist) N File:HXRFlareRibbons.jpg (Hard X-ray (green contours) and white light (G band) imaging of a flare ribbon. The left image shows the two ribbons. On the right is an enlargement of the brightest part of the southern ribbon (from Krucker et al. 2011).) (top)
- 18:40, 5 February 2012 (diff | hist) m RHESSI's Tenth Anniversary (Replaced gamma-ray imaging and Dopplar line shifts sections with new combined section and moved it to the top)
- 22:07, 4 February 2012 (diff | hist) m RHESSI's Tenth Anniversary (Added horizontal lines and alternated figures, left and right.)
- 21:32, 4 February 2012 (diff | hist) m RHESSI's Tenth Anniversary (Added microflare locations figure and references)
- 19:54, 4 February 2012 (diff | hist) N File:Christeetal2008.jpg (Flare positions as observed plotted on the solar disk. Positions were found by finding the centroid of back-projection images. Flares are concentrated in the active region bands.) (top)
- 19:49, 4 February 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Microflares and the Quiet Sun: Added text and Christe et al. reference.)
- 19:29, 4 February 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Location of Superhot X-ray source: Added image, text, and reference.)
- 19:09, 4 February 2012 (diff | hist) N File:Caspi&Lin2010.jpg (X-ray spectrum and image of the 2002 July 23 X4.8 flare. Photon flux spectra (black), model fit (Fe and Fe-Ni lines: olive; super-hot: brown; hot: magenta; non-thermal: green; total model: blue), and normalized residuals during the RHESSI SXR peak (~00:31) (top)
- 22:58, 3 February 2012 (diff | hist) m RHESSI's Tenth Anniversary (→RHESSI's Scientific Legacy: Text for Microflares section and "trnasient" changed to "terrestrial.")
- 23:25, 1 February 2012 (diff | hist) m RHESSI's Tenth Anniversary (→RHESSI's Scientific Legacy: Added link to Nugget #71 & reference to Ji et al.)
- 23:16, 1 February 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Coincidence of flare impulsive phase with CME acceleration: Added figure, references, and text)
- 22:54, 1 February 2012 (diff | hist) File:Temmeretal2010.jpg (uploaded a new version of "File:Temmeretal2010.jpg": CME kinematics of the 2008 March 25 M1.7 flare/CME event. Top to bottom: CME distance, velocity, and acceleration against time together with the background-subtracted flare HXR flux (red, ) (top)
- 22:50, 1 February 2012 (diff | hist) N File:Temmeretal2010.jpg (CME kinematics of the 2008 March 25 M1.7 flare/CME event. Top to bottom: CME distance, velocity, and acceleration against time together with the background-subtracted flare HXR flux (red, log scale). The gray bar with the letter ‘N’ indicates the time)
- 22:23, 1 February 2012 (diff | hist) m RHESSI's Tenth Anniversary (→RHESSI's Scientific Legacy: various minor text edits.)
- 22:06, 1 February 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Transient Gamma-ray Flashes (TGFs): added Smith et al. reference.)
- 21:15, 1 February 2012 (diff | hist) m RHESSI's Tenth Anniversary (→RHESSI's Scientific Legacy: Added new link to image)
- 21:13, 1 February 2012 (diff | hist) N File:Dwyer&Smith2005.jpg (Accumulated spectrum of 85 RHESSI TGFs, with theoretical relativistic-runaway spectra. The only difference between the models is the altitude of the average TGF, which is constrained to be between roughly 15 and 21 km.) (top)
- 20:56, 1 February 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Transient Gamma-ray Flashes (TGFs): Corrected link to image)
- 20:52, 1 February 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Magnetar timing and spectroscopy: Added link to nugget and 2nd reference)
- 20:27, 1 February 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Transient Gamma-ray Flashes (TGFs): Edited text)
- 23:49, 31 January 2012 (diff | hist) m RHESSI's Tenth Anniversary (→RHESSI's Scientific Legacy: Added link to nugget #14)
- 23:43, 31 January 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Transient Gamma-ray Flashes (TGFs): Added link to nugget and figure)
- 23:14, 31 January 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Coronal hard X-rays sources: added link to nugget)
- 23:12, 31 January 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Microflares and the Quiet Sun: Added link to nugget)
- 22:22, 31 January 2012 (diff | hist) m RHESSI's Tenth Anniversary (Added text to the Twin coronal sources and the initial downward motion sections.)
- 21:58, 31 January 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Photosphere as a dentist's mirror: Added figure from Kontar and Brown (2006))
- 21:49, 31 January 2012 (diff | hist) N File:Kontar&Brown2006.jpg (Bottom: Recovered mean electron flux spectra (thick lines) for the 2002 August 20 flare (accumulation time interval 08:25:20–08:25:40 UT) for the downward-directed (solid line) and observer-directed (dashed line) fluxes with corresponding errors (thin l) (top)
- 21:38, 31 January 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Photosphere as a dentist's mirror)
- 15:43, 31 January 2012 (diff | hist) m RHESSI's Tenth Anniversary (→RHESSI's Scientific Legacy)
- 14:59, 31 January 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Magnetar timing and spectroscopy)
- 14:54, 31 January 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Solar Oblateness)
- 14:51, 31 January 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Different X-ray and gamma-ray source locations)
- 14:47, 31 January 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Broadened 511-keV positron annihilation line)
- 14:41, 31 January 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Different X-ray and gamma-ray source locations)
- 14:37, 31 January 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Coronal hard X-rays sources)
- 02:56, 30 January 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Initial downward motion of X-ray sources)
- 02:52, 30 January 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Initial downward motion of X-ray sources)
- 02:48, 30 January 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Double Coronal X-ray Sources)
- 02:46, 30 January 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Double Coronal X-ray Sources)
- 02:24, 30 January 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Solar Oblateness)
- 02:20, 30 January 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Magnetar timing and spectroscopy)
- 02:19, 30 January 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Magnetar timing and spectroscopy)
- 02:12, 30 January 2012 (diff | hist) N File:Hurleyetal 1 2005.jpg (a: RHESSI 20−100-keV X-ray time history plotted with 0.5-s resolution. The flare began with an intense spike followed by the oscillatory phase. Inset, time history of the precursor with 8-ms resolution. b: Spectral blackbody temperature versus time de) (top)
- 01:29, 30 January 2012 (diff | hist) N File:Hurleyetal2005.jpg (An exceptionally bright flare from SGR 1806−20 and the origins of short-duration γ-ray bursts Hurley et al. Time-averaged counts in the tail phase of the giant flare, compared with the ‘trapped fireball’ model. Zero corresponds to 77,280 s UT. The) (top)
- 19:16, 29 January 2012 (diff | hist) m RHESSI's Tenth Anniversary (→RHESSI's Scientific Legacy)
- 18:42, 29 January 2012 (diff | hist) File:Fivianetal2008.jpg (uploaded a new version of "File:Fivianetal2008.jpg": Comparison of oblateness measurements from space. Here, we compare the RHESSI oblateness measurement, representing data from 29 June to 24 September 2004 (red crosses), with the best earli) (top)
- 18:37, 29 January 2012 (diff | hist) N File:Fivianetal2008.jpg (Comparison of oblateness measurements from space. Here, we compare the RHESSI oblateness measurement, representing data from 29 June to 24 September 2004 (red crosses), with the best earlier values, namely the balloon-borne Solar Disk Sextant (SDS) experi)
- 18:11, 29 January 2012 (diff | hist) m RHESSI's Tenth Anniversary (→RHESSI's Scientific Legacy)
- 18:00, 29 January 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Share et al. (2004))
- 17:45, 29 January 2012 (diff | hist) N File:Shareetal2004.jpg (RHESSI count spectra of the solar 511 keV annihilation line (instrumentally broadened) derived by subtracting bremsstrahlung and nuclear contributions during the 2003 October 28 flare when the solar line was broad (11:06–11:16 UT) and narrow (11:18–11) (top)
- 17:38, 29 January 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Share et al. (2004))
- 19:03, 24 January 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Krucker et al.)
- 18:51, 24 January 2012 (diff | hist) N File:Kruckeretal2008.jpg (Images taken during the flare on January 20, 2005 at the peak time at 06:43:32 to 06:46:40 UTC (left), and during the decay phase at 06:50:00 to 06:55:01 UTC (right). Both figures show a TRACE 1,600Å image taken at 06:45:11 UTC overplotted with 12–15 k) (top)
- 17:33, 24 January 2012 (diff | hist) N File:CaspiLin2010.jpg (Photon flux spectra (black), model fit (Fe and Fe–Ni lines: olive; super-hot: brown; hot: magenta; non-thermal: green; total model: blue), and normalized residuals during the RHESSI SXR peak of the flare on 2002-Jul-23 at ∼00:31:30 UT, when the super-) (top)
- 23:34, 23 January 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Sui and Holman (2003))
- 23:31, 23 January 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Hurford et al. (2003, 2006))
- 23:03, 23 January 2012 (diff | hist) N File:Hurfordetal2006.jpg (Fig. 2.—Overlay of the 50%, 70%, and 90% contours of 35� resolution gamma-ray images made with RMCs 6and 9 on a TRACE 195 Angstrom image of the 2003 October 28 flare. The red plus signs indicate 200–300 keV footpoint locations for successive adjacen) (top)
- 19:11, 23 January 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Caspi and Lin (2009?))
- 19:04, 23 January 2012 (diff | hist) m RHESSI's Tenth Anniversary (→Sui and Holman (2003))
- 19:01, 23 January 2012 (diff | hist) N File:SuiHolmanDennis2004.jpg (Altitude History of the coronal� X-ray source observed during the 2002 April 14–15 Flare. The source altitude initially decreased by 10 - 20% for the first ~3 minutes of the flare, and then increased at a speed of up to 40 km/s that is correlated with) (top)
- 18:41, 23 January 2012 (diff | hist) m RHESSI's Tenth Anniversary (→RHESSI's Scientific Legacy)
- 18:17, 23 January 2012 (diff | hist) N RHESSI's Tenth Anniversary (Starting the 10th Anniversary Nugget)
- 18:14, 23 January 2012 (diff | hist) N File:SuiHolman2003.jpg (Twin coronal X-ray sources with footpoints and presumptive location of energy release site indicated.) (top)
- 19:51, 9 September 2011 (diff | hist) m Two-stage SEE Shows Reconnection (→Authors: Modified Yang Su's location)
- 18:11, 9 September 2011 (diff | hist) File:LightCurves 08March2011.jpg (uploaded a new version of "File:LightCurves 08March2011.jpg": RHESSI 25 - 50 keV light curve corrected) (top)
- 18:10, 9 September 2011 (diff | hist) File:LightCurves 08March2011.jpg (uploaded a new version of "File:LightCurves 08March2011.jpg": RHESSI 25 - 50 keV light curve corrected)
- 21:52, 22 August 2011 (diff | hist) m Two-stage SEE Shows Reconnection (→Magnetic Reconnection: Added link to STEREO image.)
- 21:43, 22 August 2011 (diff | hist) N File:Stereo 195 2005UT.jpg (Image from STEREO_B in the 195 Angstrom passband with the disk visible from the earth to the left of the line marked "RHESSI limb.") (top)
- 21:27, 22 August 2011 (diff | hist) m Two-stage SEE Shows Reconnection (→Magnetic Reconnection: Added reference to STEREO image.)
- 20:44, 22 August 2011 (diff | hist) m Two-stage SEE Shows Reconnection (→Introduction: A Two-Stage SEE: Modified Fig. 1 caption to include EVE data and order of light curves.)
- 20:32, 22 August 2011 (diff | hist) m File:LightCurves 08March2011.jpg (Added reference to the EVE irradiance curves in this knew figure. Change the spacecraft name order to better reflect order of the curves in the figure.)
- 20:27, 22 August 2011 (diff | hist) m Two-stage SEE Shows Reconnection (→Introduction: A Two-Stage SEE: Add reference to EVE irradiance curves in Fig. 1)
- 20:08, 22 August 2011 (diff | hist) File:LightCurves 08March2011.jpg (uploaded a new version of "File:LightCurves 08March2011.jpg": Added EVE irradiance light curves. Improved RHESSI 25 - 50 keV light curve.)
- 19:52, 22 August 2011 (diff | hist) m Two-stage SEE Shows Reconnection (→Authors Notes: Minor changes)
- 19:50, 22 August 2011 (diff | hist) m Two-stage SEE Shows Reconnection (→Authors Notes: Added Brian Dennis and changed order)
- 19:44, 22 August 2011 (diff | hist) m Two-stage SEE Shows Reconnection (→References: Need link to Woods et al. paper but it is not yet on line.)
- 19:28, 22 August 2011 (diff | hist) m Two-stage SEE Shows Reconnection (→Magnetic Reconnection: Added link to movie)
- 16:53, 7 August 2011 (diff | hist) m Two-stage SEE Shows Reconnection (Minor editing)
- 16:12, 7 August 2011 (diff | hist) m Two-stage SEE Shows Reconnection (Added AIA Image and references)
- 15:52, 7 August 2011 (diff | hist) File:AIA 131 200622 bw.jpg (uploaded a new version of "File:AIA 131 200622 bw.jpg") (top)
- 15:49, 7 August 2011 (diff | hist) N File:AIA 131 200622 bw.jpg (Still from AIA movie in the 131 Angstrom passband at 20:06:22 UT showing the remarkable similarity to the classical picture of X-point magnetic reconnection.)
- 15:47, 7 August 2011 (diff | hist) m Two-stage SEE Shows Reconnection (Added figure caption.)
- 15:42, 7 August 2011 (diff | hist) m File:LightCurves 08March2011.jpg (Added a sentence about T and EM.)
- 15:37, 7 August 2011 (diff | hist) m Two-stage SEE Shows Reconnection (Added light curves plot)
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