First Non-Solar Results From HESSI

Details First Non-Solar Results From HESSI First Non-Solar Results From HESSI

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aps..apru11012s&link_type=abstract

American Physical Society, April Meeting, Jointly Sponsored with the High Energy Astrophysics Division (HEAD) of the American As

Astronomy and Astrophysics

Astrophysics

Scientific paper

The High Energy Solar Spectroscopic Imager (HESSI), to be launched January 24, functions as an all-sky monitor in the x-ray and gamma-ray range in addition to its primary mission of studying solar flares. With nine large germanium detectors, it is the largest high-resolution gamma-ray instrument ever flown in space. HESSI will study gamma-ray bursts, gamma-ray lines from radioactive isotopes in the Galaxy, accreting and isolated pulsars, and other bright sources. I will report for the HESSI team on the first results and planned projects for non-solar research with HESSI.

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