The green corona brightness and turning points in cycle 21

Details The green corona brightness and turning points in cycle 21 The green corona brightness and turning points in cycle 21

Aug 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993azh....70..856b&link_type=abstract

Astronomicheskij Zhurnal, vol. 70, p. 856

Astronomy and Astrophysics

Astronomy

4

Solar Corona, Brightness Distribution, Solar Cycles, Stellar Spectra, Distribution Functions, Spectral Energy Distribution

Scientific paper

An analysis is presented of the brightness distribution of the green corona performed on the basis of standard observations of the corona during 1977-1986 grouped according to half-years and latitude zones (equatorial, middle, and polar latitudes). A statistical investigation using the principal component method indicates that cycle phase and latitude variations can be described with an evolving distribution mode. A 'latitude-time' diagram for the regimes under consideration is constructed, and the phenomenology of the observed variations of the distributions, which apparently reflects the temporal-spatial dynamics of the magnetic structure in the corona, is discussed.

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