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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 20 | older 20) (20 | 50 | 100 | 250 | 500)- 21:53, 31 October 2008 Schriste (Talk | contribs) uploaded "File:RHESSI countrate 21042002.jpg" (RHESSI 100-200 keV counting rate (top panel) and 100 – 200 keV/50 – 100 keV hardness ratio (bottom panel) for the second peak of the 2002 April 21 solar flare.)
- 21:52, 31 October 2008 Schriste (Talk | contribs) uploaded "File:Yohkoh countrate 06051998.jpg" (Yohkoh ~100-200 keV counting rate (top panel) and ~100 – 200 keV/~50 – 100 keV hardness ratio (bottom panel) for the second peak of the 1998 May 6 solar flare. )
- 21:49, 31 October 2008 Schriste (Talk | contribs) uploaded "File:RHESSI countrate 02112003.jpg" (RHESSI 100-200 keV counting rate (top panel) and 100 – 200 keV/50 – 100 keV hardness ratio for the 2003 November 02 solar flare.)
- 21:47, 31 October 2008 Schriste (Talk | contribs) uploaded "File:Yohkoh countrate 15042001.jpg" (Yohkoh counting rate in ~100-200 keV counting rate (top panel) and ~100 – 200 keV/~50 – 100 keV hardness ratio for the 2001 April 15 solar flare.)
- 21:44, 31 October 2008 Schriste (Talk | contribs) uploaded "File:Yohkoh countrate 08142000.jpg" (Yohkoh counting rate for the 14 July 2000 events in ~100-200 keV (top panel) and ~100 – 200 keV/~50 – 100 keV hardness ratio (bottom panel) for the 2000 July 14 solar flare.)
- 19:37, 22 October 2008 Schriste (Talk | contribs) uploaded "File:XRS fip models.jpg" (FIP bias vs. FIP for two different models of coronal abundances used by CHIANTI and for the XRS-measured values for Fe, Ca, Si, and S averaged over five ~M-class flares.)
- 19:36, 22 October 2008 Schriste (Talk | contribs) uploaded "File:XRS line spectrum 01072007.jpg" (Continuum and line contributions to the measured XRS count-rate spectrum. The black curve is the best fit to the XRS count-rate spectrum and the colored lines are the contributions from the continuum and the line complexes from the different elements, as )
- 19:34, 22 October 2008 Schriste (Talk | contribs) uploaded "File:XRS fit spectrum 01072007.jpg" (MESSENGER XRS spectrum with CHIANTI thermal best-fits. Blue histogram: background-subtracted X-ray count-rate spectrum measured with XRS at the time of peak temperature during the flare starting at 14:30 UT on 1 June 2007. Green and yellow curves: CHIANTI)
- 19:32, 22 October 2008 Schriste (Talk | contribs) uploaded "File:XRS lightcurve.jpg" (X-ray light curves measured with XRS in four energy bands for the flare starting at 14:30 UT on 1 June 2007. Note that the lower energies show the typical later peak times and longer decay times compared to the higher energies.)
- 19:30, 22 October 2008 Schriste (Talk | contribs) uploaded "File:MESSENGER spacecraft.jpg" (Artist's impression of MESSENGER in orbit about Mercury, showing the sunshade on which the XRS solar monitor is mounted.)
- 01:12, 21 October 2008 Schriste (Talk | contribs) uploaded "File:Spikes Xray time delay.jpg"
- 01:08, 21 October 2008 Schriste (Talk | contribs) uploaded "File:Pulsation Xray time delay.jpg"
- 01:04, 21 October 2008 Schriste (Talk | contribs) uploaded "File:Radio Spectrum 08142008.jpg" (The event of August 14, 2004 observed by the Phoenix-2 radio spectrometer (top) and the RHESSI X-ray satellite (bottom). The event was selected for detailed analysis. The radio spectrum was cleaned from interference and shows a decimetric pulsation. The X)
- 16:02, 16 October 2008 Schriste (Talk | contribs) uploaded "File:SPHINX photo.jpg" (Photograph of the SphinX instrument ready for delivery to the CORONAS-PHOTON spacecraft)
- 01:32, 16 October 2008 Schriste (Talk | contribs) uploaded "File:Attitude control subsystem.gif" (A diagram of the RHESSI attitude control subsystem)
- 01:28, 16 October 2008 Schriste (Talk | contribs) uploaded "File:Hessi ras.jpg" (Image of the RHESSI Roll Angle System.)
- 01:15, 16 October 2008 Schriste (Talk | contribs) uploaded "File:Cryocooler.gif" (Photograph of the RHESSI cryocooler)
- 16:58, 15 October 2008 Schriste (Talk | contribs) uploaded "File:SPHINX schematic.jpg" (Schematic of the SphinX instrument. Sunlight is incident from the top via the input apertures which are 5 degree collimators. The X-rays are detected by Si PIN detectors, 20 mm2, manufactured by Amptek (USA). )
- 16:57, 15 October 2008 Schriste (Talk | contribs) uploaded "File:SPHINX simulated spectra.jpg" (Simulated X-ray spectra in the 0-12 keV range for a solar coronal plasma with temperatures 5, 10, and 25 MK. Chief line features are identified by element symbols. The spectral resolution approximately matches that expected for the SphinX detectors. )
- 16:55, 15 October 2008 Schriste (Talk | contribs) uploaded "File:CORONAS signing.jpg" (Professor Janusz Sylwester (Polish Academy of Sciences, Wroclaw, Poland: right) signs the protocol with Professor Yury Kutov of the Moscow Engineering--Physical Institute, Project Scientist of CORONAS-Photon, Warsaw, April 2006. )