Coronal structure at the July 1981 eclipse

Details Coronal structure at the July 1981 eclipse Coronal structure at the July 1981 eclipse

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983pazh....9..572n&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 9, Sept. 1983, p. 572-574) Soviet Astronomy Letters (ISSN 0360-0327), vol. 9, Sept.-Oct

Astronomy and Astrophysics

Astronomy

1

Solar Corona, Solar Eclipses, Solar Prominences, Astronomical Photography, U.S.S.R.

Scientific paper

Observations of the total solar eclipse of July 31, 1981, in Kazakhstan,
furnish a drawing of the principal coronal features out to 4 solar
radii. The association of these structures with prominences and active
regions is studied. On the west, the corona displayed a classical
maximum shape; on the east, it resembled a typical solar-minimum corona.

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