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)- 23:42, 11 September 2009 Schriste (Talk | contribs) uploaded "File:39 stacked counts 3 rbins.png" ( Stacked roll bins #3,4 & 5 taken from the three selected regions shown in corresponding colors in the previous figure.)
- 23:41, 11 September 2009 Schriste (Talk | contribs) uploaded "File:39 modulated counts.png" (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)
- 23:40, 11 September 2009 Schriste (Talk | contribs) uploaded "File:39 energy-binned pulse hts.png" (Energy-binned pulse heights.)
- 23:40, 11 September 2009 Schriste (Talk | contribs) uploaded "File:39 time-tagged pulse hts.png" (Time-tagged pulse heights.)
- 23:39, 11 September 2009 Schriste (Talk | contribs) uploaded "File:39 triangle waveform.png" (Ideal hard X-ray grid response (solid curve), with its associated fundamental sinusoid (dashed curve).)
- 23:17, 20 July 2009 Schriste (Talk | contribs) uploaded a new version of "File:Icon106.jpg" (The quiet Sun.)
- 19:09, 6 July 2009 Schriste (Talk | contribs) uploaded a new version of "File:Icon105.jpg"
- 19:13, 14 May 2009 Schriste (Talk | contribs) uploaded "File:101 sbs1.png"
- 17:27, 11 May 2009 Schriste (Talk | contribs) uploaded "File:Icon101b.png"
- 19:26, 15 April 2009 Schriste (Talk | contribs) uploaded "File:Spd mtg logo 2009.png" (Meeting logo for the 2009 SPD meeting in Boulder, Colorado.)
- 17:35, 30 March 2009 Schriste (Talk | contribs) uploaded "File:Icon98.jpg" (The Chree Medal and Prize)
- 17:24, 30 March 2009 Schriste (Talk | contribs) uploaded a new version of "File:98flare tsi.jpg"
- 20:40, 2 March 2009 Schriste (Talk | contribs) uploaded "File:Icon96.png" (EMT)
- 19:42, 2 March 2009 Schriste (Talk | contribs) uploaded "File:Microflare EMT.png" ( Microflare temperature against emission measure. The correlation plot is the microflares in this study with black plus signs representing the results of a previous RHESSI study ( Battaglia et al. 2005). The dashed straight line rep- resents the corre)
- 20:39, 16 February 2009 Schriste (Talk | contribs) uploaded "File:Icon95.png" (The diagram of an implosion. (courtesy of wikipedia))
- 20:52, 5 February 2009 Schriste (Talk | contribs) uploaded "File:92 lc.png" (Lightcurves of various flare emissions. Left, GOES soft X-rays and RHESSI hard/soft X-rays; right, TRACE EUV and Nobeyama microwave data.)
- 20:51, 5 February 2009 Schriste (Talk | contribs) uploaded "File:92 confus big.png" (A "confusogram" packed with information about the four time slices (on rows) and four RHESSI energy ranges (on columns, with different colors: 6-12, 12-20, 20-30, and 30-50 keV). The rightmost column shows all RHESSI energies overlaid.)
- 20:50, 5 February 2009 Schriste (Talk | contribs) uploaded "File:92 norh.png" (Left: Nobeyama 17 GHz and 34 GHz (black and blue) and RHESSI 30-50 keV (red) contours overlaid on the TRACE image at Time Slice 2. Note the extension of the blue (high-frequency radio) contours in the direction of the jet. Right: contour map of radio spec)
- 03:36, 6 January 2009 Schriste (Talk | contribs) uploaded "File:Icon92.jpg"
- 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.)
- 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.)
- 02:11, 10 December 2008 Schriste (Talk | contribs) moved RHESSI Wiki:Users to Solar Cycle 24 Group B (Should not be editing this page.)
- 17:57, 1 December 2008 Schriste (Talk | contribs) uploaded "File:Icon90.jpg" (Arthur Compton in inverse.)
- 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 )
- 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. )