File:Massoneetal1 2004.jpg: Difference between revisions
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imported>Bdennis (X-ray photon flux spectra for the time interval (01:39:04–01:39:48 UT) during the 2002 August 21 flare. This spectrum was obtained by processing the RHESSI count spectrum through the SPEX software on the Solar Software tree and is robust in the count/ph) |
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Latest revision as of 14:33, 1 November 2024
X-ray photon flux spectra for the time interval (01:39:04–01:39:48 UT) during the 2002 August 21 flare. This spectrum was obtained by processing the RHESSI count spectrum through the SPEX software on the Solar Software tree and is robust in the count/photon energy range considered (Massone et al. 2004, "Anisotropic Bremsstrahlung Emission and the Form of Regularized Electron Flux Spectra in Solar Flares," ApJ, 613, 1233).
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