All public logs
From RHESSI Wiki
Combined display of all available logs of RHESSI Wiki. You can narrow down the view by selecting a log type, the user name (case-sensitive), or the affected page (also case-sensitive).(Latest | Earliest) View (newer 50 | older 50) (20 | 50 | 100 | 250 | 500)- 21:47, 21 September 2018 Bdennis (Talk | contribs) 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 in the study.)
- 21:44, 21 September 2018 Bdennis (Talk | contribs) uploaded "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 Bdennis (Talk | contribs) uploaded "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)
- 21:18, 21 September 2018 Bdennis (Talk | contribs) uploaded "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 )
- 21:06, 21 September 2018 Bdennis (Talk | contribs) uploaded "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)
- 20:27, 21 September 2018 Bdennis (Talk | contribs) uploaded "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)
- 22:24, 17 September 2018 Bdennis (Talk | contribs) uploaded "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)
- 22:00, 17 September 2018 Bdennis (Talk | contribs) uploaded "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)
- 22:08, 2 March 2017 Bdennis (Talk | contribs) uploaded "File:EdChupp.jpg" (Edward Chupp Emeritus Professor Department of Physics, Professor Space Science Center (EOS) Physics )
- 20:40, 17 September 2015 Bdennis (Talk | contribs) uploaded "File:Lc 28Oct2013 0152to0214 hsi 50to100keV GOESderiv EVEderiv.jpg" (RHESSI, GOES, and EVE/ESP light curves for flare on 28 October 2013)
- 15:33, 17 September 2015 Bdennis (Talk | contribs) uploaded "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.)
- 16:10, 10 September 2015 Bdennis (Talk | contribs) uploaded "File:Lc 11Mar2015161140to1700 GOES13&15deriv crosscorrelation.jpg" (Time derivative of GOES 13 and 15 light curves with cross correlation plots for selected time intervals.)
- 16:04, 10 September 2015 Bdennis (Talk | contribs) uploaded "File:Lc 11Mar2015161140to1700 GOES13&15deriv.jpg" (GOES13&15 Light curves for flare starting at 16:20 UT on 11 march 2015 (SOL2015-03-11).)
- 15:01, 10 September 2015 Bdennis (Talk | contribs) uploaded "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.)
- 21:59, 9 September 2015 Bdennis (Talk | contribs) uploaded "File:Lc 23July2002 0017to0036 GOES logflux logderivative.jpg" (GOES Flux and time derivative light curves for 23 July 2002)
- 21:08, 8 September 2014 Bdennis (Talk | contribs) uploaded "File:Hsi sepdet spectrum 20140903 133928to134028.png" (Kim's latest version)
- 21:01, 8 September 2014 Bdennis (Talk | contribs) uploaded a new version of "File:Hsi sepdet spectrum 20050120 065040to065140.png" (Kim's latest version)
- 20:59, 8 September 2014 Bdennis (Talk | contribs) uploaded a new version of "File:Hsi sepdet spectrum 20140903 025128to025228.png" (Kim's latest version)
- 20:56, 8 September 2014 Bdennis (Talk | contribs) uploaded a new version of "File:Hsi sepdet spectrum 20140502 005436to005536.png" (Kim's latest version.)
- 21:30, 5 September 2014 Bdennis (Talk | contribs) uploaded "File:Hsi sepdet spectrum 20140903 025128to025228.png" (Count flux and photon spectra for all individual detector front segments for flare on 03 September 2014.)
- 13:15, 4 September 2014 Bdennis (Talk | contribs) uploaded "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.)
- 22:29, 3 September 2014 Bdennis (Talk | contribs) uploaded "File:Hsi sepdet spectrum 20140502 005436to005536.png" (Individual detector count and photon flux spectra.)
- 15:14, 6 February 2012 Bdennis (Talk | contribs) uploaded "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)
- 15:11, 6 February 2012 Bdennis (Talk | contribs) uploaded "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)
- 19:29, 5 February 2012 Bdennis (Talk | contribs) uploaded "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)
- 18:52, 5 February 2012 Bdennis (Talk | contribs) uploaded "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).)
- 19:54, 4 February 2012 Bdennis (Talk | contribs) uploaded "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.)
- 19:09, 4 February 2012 Bdennis (Talk | contribs) uploaded "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)
- 22:54, 1 February 2012 Bdennis (Talk | contribs) 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, log scale). The gray bar with the letter ‘N’ indicates the time)
- 22:50, 1 February 2012 Bdennis (Talk | contribs) uploaded "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)
- 21:13, 1 February 2012 Bdennis (Talk | contribs) uploaded "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.)
- 21:49, 31 January 2012 Bdennis (Talk | contribs) uploaded "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)
- 02:12, 30 January 2012 Bdennis (Talk | contribs) uploaded "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)
- 01:29, 30 January 2012 Bdennis (Talk | contribs) uploaded "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)
- 18:42, 29 January 2012 Bdennis (Talk | contribs) 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 earlier values, namely the balloon-borne Solar Disk Sextant (SDS) experi)
- 18:37, 29 January 2012 Bdennis (Talk | contribs) uploaded "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)
- 17:45, 29 January 2012 Bdennis (Talk | contribs) uploaded "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 (11:18–1)
- 18:51, 24 January 2012 Bdennis (Talk | contribs) uploaded "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)
- 17:33, 24 January 2012 Bdennis (Talk | contribs) uploaded "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-)
- 23:03, 23 January 2012 Bdennis (Talk | contribs) uploaded "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)
- 19:01, 23 January 2012 Bdennis (Talk | contribs) uploaded "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)
- 18:14, 23 January 2012 Bdennis (Talk | contribs) uploaded "File:SuiHolman2003.jpg" (Twin coronal X-ray sources with footpoints and presumptive location of energy release site indicated.)
- 18:11, 9 September 2011 Bdennis (Talk | contribs) uploaded a new version of "File:LightCurves 08March2011.jpg" (RHESSI 25 - 50 keV light curve corrected)
- 18:10, 9 September 2011 Bdennis (Talk | contribs) uploaded a new version of "File:LightCurves 08March2011.jpg" (RHESSI 25 - 50 keV light curve corrected)
- 21:43, 22 August 2011 Bdennis (Talk | contribs) uploaded "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.")
- 20:08, 22 August 2011 Bdennis (Talk | contribs) uploaded a new version of "File:LightCurves 08March2011.jpg" (Added EVE irradiance light curves. Improved RHESSI 25 - 50 keV light curve.)
- 15:52, 7 August 2011 Bdennis (Talk | contribs) uploaded a new version of "File:AIA 131 200622 bw.jpg"
- 15:49, 7 August 2011 Bdennis (Talk | contribs) uploaded "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.)
- 15:32, 7 August 2011 Bdennis (Talk | contribs) uploaded "File:LightCurves 08March2011.jpg" (AIA, GOES, RHESSI light curves of the 2-stage SEE on 8 March 2011.)
- 23:14, 29 December 2009 Bdennis (Talk | contribs) uploaded "File:Lc 021004tp021008 clean chisqvsiter gain0p1 64x8arcsec 12to25kev d789.jpg" (Plot with chi-squared test enabled in Clean. Time interval 21 April 2002 02:10:04 to 02:10:08 UT.)