Structure and shape of the white-light corona during March 9, 1997 and February 26, 1998 eclipses

Details Structure and shape of the white-light corona during March 9, 1997 and February 26, 1998 eclipses Structure and shape of the white-light corona during March 9, 1997 and February 26, 1998 eclipses

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999coska..28..210m&link_type=abstract

Contributions of the Astronomical Observatory Skalnate Pleso, vol. 28, no. 3, p. 210-215.

Astronomy and Astrophysics

Astronomy

2

The Sun, Corona, Structure

Scientific paper

Structures of the white-light corona (WLC) as were observed during last total solar eclipses on March 9, 1997 and February 26, 1998 are discussed. Both eclipses occurred in the minimum of cycle activity at the beginning of cycle 23. The WLC was a minimum type with many polar rays and extended helmet streamers, located in middle heliographic latitudes or very close to the equator, and coronal holes around the poles. Flattening index is derived, and turn out to be, a+b = 0.27 for 1997, and a+b = 0.22 for 1998, respectively.

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