Shape and structure of the corona during the November 3, 1994 eclipse

Details Shape and structure of the corona during the November 3, 1994 eclipse Shape and structure of the corona during the November 3, 1994 eclipse

Jan 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995coska..25..117k&link_type=abstract

Contributions of the Astronomical Observatory Skalnate Pleso, Volume 25, p. 117-119

Astronomy and Astrophysics

Astronomy

1

Solar Corona, Solar Eclipses, Coronal Holes, Stellar Mass, Solar Cycles, Solar Magnetic Field, Solar Wind, Plumes, Stellar Mass Ejection, Astronomical Photometry, Plasma Diagnostics

Scientific paper

A brief description of the scientific goals and preliminary results
related to the 3 Nov. 1994 eclipse at Putre, is given. The white-light
corona was of minimum type with two large helmet streamers seen up to 7
- 8 R(solar radius), and located around the solar equator in the E- and
W-limbs. Coronal holes and plumes are located around the solar poles.

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