File:Caspi&Lin2010.jpg: Difference between revisions

X-ray spectrum and image of the 2002 July 23 X4.8 flare. Photon flux spectra (black), model fit (Fe and Fe-Ni lines: olive; super-hot: brown; hot: magenta; non-thermal: green; total model: blue), and normalized residuals during the RHESSI SXR peak (~00:31:30 UT), when the super-hot component is strongest. Inset: 50% and 90% contours of 6.3-7.3 (olive solid), 9-12 (blue dotted), 17-18 (brown dashed), and 60-100 keV (green dot-dashed) images at the same time; the crosses denote the derived centroid locations (and uncertainties) of the super-hot (brown; left) and hot (magenta; right) components.