Upload log
From RHESSI Wiki
Below is a list of the most recent file uploads. See the gallery of new files for a more visual overview.(Latest | Earliest) View (newer 50 | older 50) (20 | 50 | 100 | 250 | 500)- 20:51, 5 January 2009 Lfletcher (Talk | contribs) uploaded "File:Pixons 041002.png" (RHESSI image of the 4-October-2008 event, made with grids 1,3,4,5,6 between 25-50keV. The Pixons algorithm was used.)
- 20:37, 5 January 2009 Lfletcher (Talk | contribs) uploaded "File:Wlmodel2.png" (TRACE WL image at the peak of the 4-Oct-2002 flare)
- 01:53, 23 December 2008 Schriste (Talk | contribs) uploaded "File:Icon91.png"
- 20:29, 22 December 2008 Schriste (Talk | contribs) uploaded "File:Solar Cycle 24 Schedule.jpg" (Layout of the working groups at the Solar24 meeting. )
- 18:28, 22 December 2008 Schriste (Talk | contribs) uploaded "File:Sunspot Numbers.png" (This figure summarizes the 400 years of regular sunspot number observations. This figure was prepared by Robert A. Rohde and is part of the Global Warming Art project.)
- 15:06, 22 December 2008 Hhudson (Talk | contribs) uploaded "File:Icon91.jpg"
- 14:07, 22 December 2008 Hhudson (Talk | contribs) uploaded "File:Solar24.jpg" (Variation of the radio index [http://www.hia-iha.nrc-cnrc.gc.ca/drao/solar_e.html F10.7] over its recorded history, which began in 1947. As a crude measure of cycle length, this plot locates each cycle by noting when this index passes through 80 SFU (one )
- 17:32, 10 December 2008 Schriste (Talk | contribs) uploaded "File:Solar Cycle 24 Poster.jpg" (Meeting poster for the Solar Cycle 24 meeting in Napa.)
- 17:57, 1 December 2008 Schriste (Talk | contribs) uploaded "File:Icon90.jpg" (Arthur Compton in inverse.)
- 17:05, 1 December 2008 Hhudson (Talk | contribs) uploaded "File:Icon90.png" (Inverse Compton scattering is really the same thing as regular Compton scattering, from the physicist's point of view)
- 18:18, 24 November 2008 Pmallik (Talk | contribs) uploaded a new version of "File:ICposi.jpg"
- 18:13, 24 November 2008 Pmallik (Talk | contribs) uploaded a new version of "File:ICelec.jpg"
- 17:43, 24 November 2008 Pmallik (Talk | contribs) uploaded "File:Inversecompton.jpg"
- 17:42, 24 November 2008 Pmallik (Talk | contribs) uploaded "File:Invsersecompton.jpg"
- 17:37, 24 November 2008 Pmallik (Talk | contribs) uploaded "File:ICposi.jpg"
- 17:24, 24 November 2008 Pmallik (Talk | contribs) uploaded "File:ICelec.jpg"
- 20:55, 17 November 2008 Schriste (Talk | contribs) uploaded "File:Icon89.png" (Arthur Compton holding the dip.)
- 15:50, 13 November 2008 Schriste (Talk | contribs) uploaded "File:Histogram of dip as function of index.png" (Histogram showing the percentage of flares with a dip as a function of spectral index γ )
- 15:48, 13 November 2008 Schriste (Talk | contribs) uploaded "File:Histogram of dip as function of heliocentric angle.png" (Histogram of the 18 events with a significant dip as a function of μ, the cosine of the heliocentric angle of the flare.)
- 15:45, 13 November 2008 Schriste (Talk | contribs) uploaded "File:Electron Spectrum for 01Apr2004.png" (Plot of electron distribution spectrum for the 1 April 2004 23:00 UTC solar flare. The blue line denotes the uncorrected electron spectrum and the green line denotes the electron spectrum after correction for albedo. Both lines are plotted with 1σ error )
- 11:14, 12 November 2008 Hhudson (Talk | contribs) uploaded "File:Icon 80.jpg" (Gauguin's view of the McClymont Jerk)
- 13:21, 5 November 2008 Hhudson (Talk | contribs) uploaded "File:Icon 81.jpg" (Solar centroid locations of thousands of X-ray microflares observed by RHESSI. )
- 13:17, 5 November 2008 Hhudson (Talk | contribs) uploaded "File:Icon 82.jpg"
- 13:14, 5 November 2008 Hhudson (Talk | contribs) uploaded "File:Icon 83.jpg"
- 11:07, 5 November 2008 Hhudson (Talk | contribs) uploaded a new version of "File:Icon 84.jpg" (A view of MESSENGER's accommodation of the X-ray Spectrometer instrument.)
- 11:03, 5 November 2008 Hhudson (Talk | contribs) uploaded "File:Icon 85.jpg" (Sobel-filtered white-light image constructed from one month's worth of RHESSI aspect-camera data.)
- 11:00, 5 November 2008 Hhudson (Talk | contribs) uploaded "File:Icon 84.jpg" (Thumbnail of an optical image constructed from the linear CCDs of RHESSI's SAS. This is probably a one-month integration, shown via the Sobel high-pass filter to have residuals due to sunspots.)
- 22:24, 4 November 2008 Schriste (Talk | contribs) uploaded "File:Icon 86.jpg"
- 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. )
- 18:26, 3 October 2008 Wikisysop (Talk | contribs) uploaded "File:RHESSI optical images icon.png" (Icon for RHESSI optical images Nugget)
- 00:36, 3 October 2008 Wikisysop (Talk | contribs) uploaded "File:RHESSI may image.gif" (RHESSI visible light image of the Sun for the month of May, 2003.)