  We have performed the first polarimetry of solar flare emission at gamma-ray
energies (0.2-1 MeV). These observations were performed with the Reuven Ramaty
High Energy Solar Spectroscopic Imager (RHESSI) for two large flares: the GOES
X4.8-class solar flare of 2002 July 23, and the X17-class flare of 2003 October
28. We have marginal polarization detections in both flares, at levels of 21%
+/- 9% and -11% +/- 5% respectively. These measurements significantly constrain
the levels and directions of solar flare gamma-ray polarization, and begin to
probe the underlying electron distributions.
