White-light coronal structures during the 1988 -- 1998 eclipses

Details White-light coronal structures during the 1988 -- 1998 eclipses White-light coronal structures during the 1988 -- 1998 eclipses

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999coska..28..230b&link_type=abstract

Contributions of the Astronomical Observatory Skalnate Pleso, vol. 28, no. 3, p. 230-236.

Astronomy and Astrophysics

Astronomy

4

The Sun, Corona, Magnetic Fields

Scientific paper

Large-scale coronal structures (helmet streamers), observed in the white-light solar corona during total eclipses, are mostly seen above prominences. These streamers are supported by the global magnetic field of the Sun. However, the distribution of prominences over a solar cycle shows both the poleward and equatorward migrations. The location of observed white-light coronal streamers during total eclipses in the period 1988 --1998 will be compared and discussed with that of prominences. It seems that the distribution of the above mentioned streamers matches the distribution of prominences and shifts together with prominence belts to the poles. A possible scenario for a such development is described and discussed.

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