Corona: Coordinated research on non-thermal processes in astrophysics

Details Corona: Coordinated research on non-thermal processes in astrophysics Corona: Coordinated research on non-thermal processes in astrophysics

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991udnw.rept.....m&link_type=abstract

Final Report, 1 May 1988 - 30 Apr. 1991 Delaware Univ., Newark.

Astronomy and Astrophysics

Astrophysics

Astrophysics, Atmospheric Turbulence, Particle Energy, Plasma Heating, Stellar Coronas, Stellar Winds, Convective Heat Transfer, Magnetic Field Reconnection, Magnetohydrodynamic Turbulence, Nonthermal Radiation, Temperature Effects

Scientific paper

Several problems in astrophysics are examined where departures from purely thermal behavior are expected to produce effects which are detectable by a variety of NASA satellites. The problems identified as worthy of study include coronal heating in stars, deposition of non-thermal particle energy in stars from external sources, and turbulence in atmospheres and winds of stars. The progress in solving these problems is summarized.

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