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This special page shows all uploaded files. By default the last uploaded files are shown at top of the list.

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File list
 

Date Name User ascSize Description Versions
02:18, 14 April 200999_Blank.png (file)Lsvalgaard218 B 1
08:24, 22 August 201820f2.png (file)Hhudson710 B 1
20:44, 23 July 2014Test.jpg (file)JanGrafvonderPahlen727 B 1
08:24, 22 August 201820f1.png (file)Hhudson2 KB 1
08:25, 22 August 201820f7.png (file)Hhudson2 KB 1
11:03, 5 November 2008Icon_85.jpg (file)Hhudson2 KB (Sobel-filtered white-light image constructed from one month's worth of RHESSI aspect-camera data.)1
11:14, 12 November 2008Icon_80.jpg (file)Hhudson2 KB (Gauguin's view of the McClymont Jerk)1
23:42, 11 September 200939_amplitudes_and_phases.png (file)Schriste4 KB (Visibility amplitudes and phases derived from the stacked counts in Figure 2d. Roll bins #3,4 & 5 taken from the three selected regions are shown in the same colors as the previous figure.)1
11:09, 15 April 2014Icon223.png (file)Hhudson4 KB 1
08:24, 22 August 201820f3.png (file)Hhudson4 KB 1
09:49, 15 February 2010Plot_314MHz.png (file)Haurass4 KB 1
13:21, 5 November 2008Icon_81.jpg (file)Hhudson4 KB (Solar centroid locations of thousands of X-ray microflares observed by RHESSI. )1
21:48, 2 January 2020Eqn3.jpg (file)Amackinnon5 KB 2
13:17, 5 November 2008Icon_82.jpg (file)Hhudson5 KB 1
20:38, 15 September 2017306e1.png (file)Hhudson5 KB 1
08:25, 22 August 201820f8.png (file)Hhudson5 KB 1
03:16, 25 November 2011Icon164.png (file)Hhudson5 KB 2
15:15, 23 May 2009Icon102.png (file)Hhudson5 KB 2
18:57, 21 December 2011Cryo_current_20111215.png (file)Jmctiernan5 KB (RHESSI cryocooler current for two days, 2011-12-15 and 2011-12-16)1
13:51, 30 September 2013Icon208.png (file)Hhudson5 KB (A cartoon from Kosugi (1985) showing the possibility of gyroresonance contributions to the post-flare loops comprising a microwave thermal source of the PBI/GRF type.)1
23:41, 11 September 200939_modulated_counts.png (file)Schriste5 KB (RHESSI modulation profile. The green vertical lines mark the boundaries of spacecraft rotations, (units of 360 degrees) and the red tick marks indicate the roll bins selected for phase-bin stacking. Three sets of rollbins are identified by the colors blue)1
13:14, 5 November 2008Icon_83.jpg (file)Hhudson5 KB 1
10:53, 3 January 2020Eqn5.jpg (file)Amackinnon5 KB 1
23:40, 11 September 200939_energy-binned_pulse_hts.png (file)Schriste5 KB (Energy-binned pulse heights.)1
03:46, 5 January 2010Hessi_dets_test_hi_ct1b.png (file)Jmctiernan5 KB (D1 sensitivity relative to background-subtracted GOES)1
03:36, 6 January 2009Icon92.jpg (file)Schriste5 KB 1
00:18, 10 February 2011Hsi_flare_list_split_flare_sm.png (file)Jmctiernan5 KB (Inside hsi_flare_list_fill, demonstration of temp_split_flare on extra-smoothed data)1
23:44, 9 February 2011Hsi_flare_list_split_flare.png (file)Jmctiernan5 KB (Inside hsi_flare_list_fill, demonstration of temp_split_flare results)1
23:42, 11 September 200939_stacked_counts_3_rbins.png (file)Schriste6 KB ( Stacked roll bins #3,4 & 5 taken from the three selected regions shown in corresponding colors in the previous figure.)1
23:49, 9 February 2011Hsi_flare_list_simple_flare.png (file)Jmctiernan6 KB (Inside hsi_flare_list_fill, a simple flare finding.)1
13:38, 28 September 2010Icon136.jpg (file)Hhudson6 KB (Courtesy MDI)1
08:13, 11 March 2015Sunant_flux_20140610.png (file)JuhaKallunki6 KB (MRO solar antenna measurement on 20140610)1
01:53, 23 December 2008Icon91.png (file)Schriste6 KB 1
09:34, 23 October 2012RhessiLightcurve.png (file)HeatherRatcliffe6 KB (RHESSI Lightcurves for the second Glasgow Callisto event )1
14:30, 13 July 2011Icon155.png (file)Hhudson6 KB (A hard X-ray spike elicits a sympathetic response)1
23:47, 9 February 2011Hsi_flare_list_mult_flare.png (file)Jmctiernan6 KB (Inside hsi_flare_list_fill, an orbit with lots of flares, which will need splitting.)2
00:29, 22 December 2009Hessi_dets_test_ct24.png (file)Jmctiernan6 KB (Ratio of Rhessi counts for detector 1 to GOES Hi channel flux, for twos samples of flares.)1
10:42, 22 January 2009Icon93.jpg (file)Hhudson6 KB 1
10:37, 20 March 2014Icon221.png (file)Hhudson6 KB 1
23:12, 13 March 200997_jmm_Ppr2008_f4.png (file)Jmctiernan6 KB (RHESSI versus GOES T, for the first 7 months of the mission.)1
14:30, 5 November 2019Icon363.png (file)Hhudson6 KB 1
21:01, 7 June 2011153f1.png (file)Hhudson6 KB (Upper, GOES soft X-rays, and lower, RHESSI hard X-rays. Note that there is no soft X-ray counterpart of the burst.)1
10:03, 3 September 2015260f2.png (file)Hhudson6 KB 1
23:39, 11 September 200939_triangle_waveform.png (file)Schriste6 KB (Ideal hard X-ray grid response (solid curve), with its associated fundamental sinusoid (dashed curve).)1
00:25, 22 December 2009Hessi_dets_test_ct14.png (file)Jmctiernan6 KB (Ratio of RHESSI Detector 1 counts versus both GOES channels versus time)1
19:08, 6 September 2019Ppr2019_nugget_20110213_chi2.png (file)Jmctiernan6 KB (Chi^2 versus cutoff energy E_c, coronal (black), photospheric (red) abundance)1
15:22, 28 September 2009111Icon.jpg (file)Hhudson6 KB (A five-hour RHESSI integration at 4-8 keV starting some 9 hours after a C-class flare and CME eruption.)1
15:26, 28 September 2009Icon111.jpg (file)Hhudson6 KB (With an extremely deep integration, RHESSI may have detected X-rays from the base of a post-CME current sheet.)1
03:05, 5 January 2010Hessi_dets_test_ct1b.png (file)Jmctiernan7 KB (Time averaged RHESSI - background subtracted GOES data.)1
03:03, 5 January 2010Hessi_dets_test_ctb.png (file)Jmctiernan7 KB (Relative sensitivity for sample with ok background-subtracted GOES Hi data.)1

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