Astronomy and Astrophysics – Astronomy
Scientific paper
May 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aas...180.3304z&link_type=abstract
American Astronomical Society, 180th AAS Meeting, #33.04; Bulletin of the American Astronomical Society, Vol. 24, p.780
Astronomy and Astrophysics
Astronomy
Scientific paper
The HESP mission will explore the mechanisms of impulsive energy release, particle acceleration, and energy transport in solar flares. The quantitative understanding of these mechanisms (and the intricate relationships between them) forms the heart of the solar flare problem. The purpose of complementary observations is to furnish information on the thermal, dynamic, and magnetic context in which high-energy flare emissions are produced. In particular, complementary high resolution spatial and spectral observations that can be used to determine the density, temperature, and velocity distributions, as well as the magnetic morphology of the flaring active region will be invaluable in the interpretation of data obtained with the main HESP instrument. Examples of space-based observations that can support the objectives of the HESP mission will be described. Replace this sentence with your abstract.
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