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- 00:31, 12 September 2009 (diff | hist) Simulating Images
- 00:30, 12 September 2009 (diff | hist) Drm mod - Pseudo function for fine tuning RHESSI DRM parameters
- 00:29, 12 September 2009 (diff | hist) Selecting Background for RHESSI Spectra (top)
- 00:29, 12 September 2009 (diff | hist) Fitting a new detector
- 00:28, 12 September 2009 (diff | hist) Fit function components (top)
- 00:28, 12 September 2009 (diff | hist) Fitting multiple intervals
- 00:27, 12 September 2009 (diff | hist) Line - Gaussian
- 00:27, 12 September 2009 (diff | hist) OSPEX Users Guide
- 00:27, 12 September 2009 (diff | hist) Vth - Variable Thermal
- 00:26, 12 September 2009 (diff | hist) Thick2 - Thick Target Bremsstrahlung Version 2
- 00:26, 12 September 2009 (diff | hist) Thick - Thick Target Bremsstrahlung
- 00:25, 12 September 2009 (diff | hist) Thin - Thin Target Bremsstrahlung
- 00:24, 12 September 2009 (diff | hist) Template:Infobox Nugget
- 00:24, 12 September 2009 (diff | hist) Template:Infobox Nugget
- 00:23, 12 September 2009 (diff | hist) EIT Waves - Cadence issues
- 00:22, 12 September 2009 (diff | hist) Cycle 24 - time to panic
- 00:22, 12 September 2009 (diff | hist) Creating a Spectrum File Using the HESSI GUI
- 00:21, 12 September 2009 (diff | hist) Confined Flares versus Eruptive Flares
- 00:21, 12 September 2009 (diff | hist) Bpow - Broken Power Law
- 00:20, 12 September 2009 (diff | hist) m 3pow - Triple Power Law
- 00:04, 12 September 2009 (diff | hist) RHESSI Visibilities (→Visibilities à la Fourier: fixed spelling error)
- 00:02, 12 September 2009 (diff | hist) Confined Flares versus Eruptive Flares
- 00:02, 12 September 2009 (diff | hist) Confined Flares versus Eruptive Flares
- 00:01, 12 September 2009 (diff | hist) m Confined Flares versus Eruptive Flares
- 00:01, 12 September 2009 (diff | hist) m RHESSI Visibilities
- 00:00, 12 September 2009 (diff | hist) m RHESSI Visibilities
- 23:57, 11 September 2009 (diff | hist) RHESSI Visibilities (added figures)
- 23:52, 11 September 2009 (diff | hist) RHESSI Visibilities
- 23:52, 11 September 2009 (diff | hist) m RHESSI Visibilities
- 23:43, 11 September 2009 (diff | hist) Main Page
- 23:42, 11 September 2009 (diff | hist) N File:39 ed.gif (Observed visibility amplitudes (blue crosses) for a flare interval as a function of subcollimator (SC=1-9) and position angle (PA=0-180°) of the grids. Each of the 9 vertical panels shows the amplitude as a function of PA for one subcollimator (labeled b) (top)
- 23:42, 11 September 2009 (diff | hist) N File:39 amplitudes and phases.png (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.) (top)
- 23:42, 11 September 2009 (diff | hist) N 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.) (top)
- 23:41, 11 September 2009 (diff | hist) N 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) (top)
- 23:40, 11 September 2009 (diff | hist) N File:39 energy-binned pulse hts.png (Energy-binned pulse heights.) (top)
- 23:40, 11 September 2009 (diff | hist) N File:39 time-tagged pulse hts.png (Time-tagged pulse heights.) (top)
- 23:39, 11 September 2009 (diff | hist) N File:39 triangle waveform.png (Ideal hard X-ray grid response (solid curve), with its associated fundamental sinusoid (dashed curve).) (top)
- 23:38, 11 September 2009 (diff | hist) RHESSI Visibilities (added links)
- 23:31, 11 September 2009 (diff | hist) N RHESSI Visibilities (New page: == Visibilities à la Fourier == RHESSI is a Fourier imager, which means that it obtains amplitudes and phases (a.k.a. "visibilities") of the X-ray image modulations. This particular choi...)
- 19:34, 19 August 2009 (diff | hist) m Temp (added info box and category)
- 21:56, 18 August 2009 (diff | hist) Main Page
- 21:56, 18 August 2009 (diff | hist) Main Page
- 21:56, 18 August 2009 (diff | hist) Main Page
- 21:54, 18 August 2009 (diff | hist) Temp (→Solar activity associated to particle acceleration)
- 21:54, 18 August 2009 (diff | hist) N Temp (New page: == Introduction == Solar relativistic particle events or Ground Level Enhancements (GLEs) are the relativistic counterparts of solar energetic particle (SEP) events. They are detected by ...)
- 21:53, 18 August 2009 (diff | hist) Main Page
- 22:39, 7 August 2009 (diff | hist) EIT Waves - Cadence issues
- 22:38, 7 August 2009 (diff | hist) N Faculae and microflares (New page: In this nugget, we consider the RHESSI aspect sensors. Though their job is to provide aspect measurements, those measurements can be scientifically interesting in their own right. The RHES...)
- 22:31, 7 August 2009 (diff | hist) EIT Waves - Cadence issues
- 22:25, 7 August 2009 (diff | hist) N EIT Waves - Cadence issues (New page: Introduction Globally propagating coronal disturbances as observed by the SOHO/EIT telescope are known as "EIT waves". They are spectacular events, observed in the EUV, in which structure...)
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