Solar Gamma-Ray Lines at High Resolution with RHESSI

Details Solar Gamma-Ray Lines at High Resolution with RHESSI Solar Gamma-Ray Lines at High Resolution with RHESSI

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....6.3187m&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

Scientific paper

For the first time, gamma-ray lines from nuclear de-excitation in a solar flare have been resolved by an instrument with high energy resolution. The lines were observed by the Reuven Ramaty High Energy Solar spectroscopic Imager (RHESSI) during an X4.8 solar flare on 23 June 2002. The lines show a surprisingly high degree of redshift considering the flare's position near the solar limb.

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