The total brightness of the corona during the solar eclipse of February 16, 1980

Details The total brightness of the corona during the solar eclipse of February 16, 1980 The total brightness of the corona during the solar eclipse of February 16, 1980

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985baicz..36...73r&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 36, no. 2, 1985, p. 73-77.

Astronomy and Astrophysics

Astronomy

1

Brightness Distribution, Solar Corona, Solar Eclipses, Logarithms, Solar Radiation

Scientific paper

The total brightness of the white-light corona was determined for the total solar eclipse of February 16, 1980. Its value for the standard region 1.03 ≤ ρ ≤ 6.00 is Jk = 1.29×10-6 of the mean brightness of the solar disk at λeff = 570 nm. The values for solar eclipses of 1962, 1965, 1966, 1968 and 1970 were determined in a similar way. It was found that, in spite of the nearly spherically symmetrical appearance of the white-light corona in the solar activity maximum, the radiation maximum during this period is produced in the equatorial regions (±45°).

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