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• Flare Plasma Abundances - New X-ray Observations
  ...]. This should not be a problem during the decay phase of a flare when any plasma is likely to be in thermal equilibrium but may be an issue during the impul ... Broadly speaking, the intensity of a line from a particular element for a plasma with a given emission measure and temperature is directly proportional to t
  10 KB (1,613 words) - 16:22, 22 August 2018

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• Flare Plasma Abundances - New X-ray Observations
  ...]. This should not be a problem during the decay phase of a flare when any plasma is likely to be in thermal equilibrium but may be an issue during the impul ... Broadly speaking, the intensity of a line from a particular element for a plasma with a given emission measure and temperature is directly proportional to t
  10 KB (1,613 words) - 16:22, 22 August 2018
• RHESSI Science Nuggets
  |title = Sun-as-a-star Analysis of the M8.7 Flare on 2022 October 2 Using H-alpha and EUV Spectra Taken by SMART/SDDI and SDO |description = Whole-Sun spectroscopic observations can readily detect ejecta
  48 KB (6,239 words) - 12:34, 26 April 2024
• The Post-Burst Increase
  |next_nugget = [[The Flare that Time Forgot]] new observations make highly relevant.
  6 KB (955 words) - 17:35, 22 August 2018
• Abundances in Solar Flares
  |title = Abundances in Solar Flares |previous_nugget = [[Homing in on Flare Energy]]
  6 KB (1,011 words) - 07:38, 18 April 2014
• Microwave Images of a Single-Loop Flare: Observations and Simulations
  |title = Microwave Images of a Single-Loop Flare: Observations and Simulations |previous_nugget = [[Abundances in Solar Flares]]
  9 KB (1,294 words) - 02:51, 4 June 2014
• Fine Structure in Flare Soft X-ray Light Curves
  |title = Fine Structure in Flare Soft X-ray Light Curves ...t curves in six energy bands between 6 keV and 1 MeV (bottom) for the X4.8 flare on 23 July 2002. The step down in the 6 - 12 and 12 - 25 keV fluxes at 00:2
  12 KB (1,963 words) - 19:09, 21 September 2015
• RHESSI Science Nuggets 200 to 299
  |title = High Resolution Temporal and Spatial Structure of a White Light Flare |title = Multi-Instrument Solar Flare Observations II: A SC24 retrospective
  28 KB (3,638 words) - 14:45, 25 January 2018
• Fast electron recombination: a neglected HXR source
  ...rrors in estimating the number of energetic electrons accelerated during a flare that, under certain circumstances, can be very significant. ...y of detailed reconstruction of source electron spectra offering important new constraints on the electron energy budget and acceleration processes.
  7 KB (1,115 words) - 11:48, 27 August 2018
• MinXSS and RHESSI measure flare spectra over 1-15 keV
  |title = MinXSS and RHESSI measure flare spectra over 1-15 keV RHESSI (Ref. 1) has been performing high-quality X-ray and gamma-ray solar measurements
  4 KB (613 words) - 15:41, 6 February 2018
• Joint MinXSS and RHESSI Flare X-ray Spectra between 1 and 15 keV
  |title = MinXSS and RHESSI measure flare spectra over 1-15 keV RHESSI (Ref. 1) has been performing high-quality X-ray and gamma-ray solar measurements
  4 KB (616 words) - 09:47, 7 February 2018