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X-Ray Polarimetry Workshop
SLAC, Stanford, California
9-11 February 2004


absID

 

Hard X-Ray Polarization and Particle Acceleration in Solar Flares

Gordon

Emslie

UAH

emslieg@uah.edu

A. Gordon Emslie, UAH

The cross-section for bremsstrahlung production at hard X-ray energies is a strong function of the direction of the emitted photon relative to the incident electron (directivity) and of the polarization state of the emitted photon. Thus, measurements of hard X-ray polarization provide information on the anisotropy (beaming) of the accelerated electrons. I will review the (extensive) theoretical work in this area in anticipation of the recent observations by RHESSI, and the prospects of these observations as a diagnostic of particle acceleration processes in solar flares.

 

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