Solar gamma-ray physics comes of age

Details Solar gamma-ray physics comes of age Solar gamma-ray physics comes of age

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..587..603s&link_type=abstract

GAMMA 2001: Gamma-Ray Astrophysics 2001. AIP Conference Proceedings, Volume 587, pp. 603-612 (2001).

Astronomy and Astrophysics

Astrophysics

5

Spectroscopy And Spectrophotometry, Particle Emission, Solar Wind, Gamma-Ray

Scientific paper

The launch of NASA's HESSI satellite will provide solar scientists with >= 2arcsec imaging/>= 2 keV spectroscopy of solar flares from ~10 keV to 10 MeV for the first time. We summarize recent developments in our understanding of solar flares based primarily on gamma-ray line measurements made over the past twenty years with instruments having moderate spectral resolution. These measurements have provided information on solar ambient abundance, density and temperature; accelerated particle composition, spectra, and transport; and flare energetics. .

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