File:Massoneetal1 2004.jpg

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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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current15:11, 6 February 2012Thumbnail for version as of 15:11, 6 February 2012770×575 (59 KB)Bdennis (Talk | contribs) (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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