The Use of Electron Maps to Constrain Some Physical Properties of Solar Flares

Physics

Scientific paper

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Sun: Flares, Sun: X-Rays, Methods: Regularization, Methods: Positivity Constraint

Scientific paper

The most direct representation of the measurements provided by the Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) is a set of Fourier components of the X-ray radiation sampled at discrete points of the spatial-frequency plane, the so called visibilities. Here we review methods for the reconstruction of X-ray and electron maps using RHESSI visibilities and show how the electron maps can be utilized to infer information about the physical properties of the acceleration region during flaring events.

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