Variations of the total brightness of the white-light corona with the phase of the solar cycle

Details Variations of the total brightness of the white-light corona with the phase of the solar cycle Variations of the total brightness of the white-light corona with the phase of the solar cycle

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985baicz..36...77r&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 36, no. 2, 1985, p. 77-81.

Astronomy and Astrophysics

Astronomy

12

Brightness Distribution, Solar Corona, Solar Cycles, Data Reduction, Ellipticity, Periodic Variations

Scientific paper

The good agreement is demonstrated between the total brightness of the white-light corona in the standard region (1.03 - 6.00 R_sun;) in dependence on the phase of the solar cycle. Its observed values are within the interval of 0.48 (minimum) and 1.42 (maximum) × 10-6 of the mean brightness of the solar disk. Within the range of observational errors, no difference in the values of the total brightness of the white-light corona was observed between the individual cycles during this century. The dependence between ellipticity and the total brightness was determined in relation to the solar cycle phase.

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