Solar coronal non-thermal processes (Solar Maximum Mission)

Details Solar coronal non-thermal processes (Solar Maximum Mission) Solar coronal non-thermal processes (Solar Maximum Mission)

Feb 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ucsd.reptq....h&link_type=abstract

Final Report California Univ., San Diego, La Jolla. Center for Astrophysics and Space Sciences.

Astronomy and Astrophysics

Astrophysics

Photosphere, Solar Corona, X Ray Sources, Electron Transfer, Monte Carlo Method, Solar Maximum Mission, X Ray Telescopes

Scientific paper

The Solar Maximum Mission was used to study solar coronal phenomena in
hard X-radiation, since its instrument complement included the first
solar hard X-ray telescope. Phenomena related to those discovered from
OSO-5 and OSO-7 observations were emphasized.

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