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Flare physics at high energiesHigh-energy processes, involving a rich variety of accelerated particle phenomena, lie at the core of the solar flare problem. The most direct manifestation of these processes are high-energy radiations, gamma rays, hard X-rays and neutrons, as well as the accelerated particles themselves, which can be detected in interplanetary space. In the study of astrophysics from the moon, the understanding of these processes should have great importance. The inner solar system environment is strongly influenced by activity on the sun; the physics of solar flares is of great intrinsic interest; and much high-energy astrophysics can be learned from investigations of flare physics at high energies.
Document ID
19910071961
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Ramaty, R.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1990
Subject Category
Solar Physics
Meeting Information
Meeting: Astrophysics from the Moon
Location: Annapolis, MD
Country: United States
Start Date: February 5, 1990
End Date: February 7, 1990
Sponsors: NASA
Accession Number
91A56584
Distribution Limits
Public
Copyright
Other

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