On the physical significance of white light polar plumes in the solar corona

Details On the physical significance of white light polar plumes in the solar corona On the physical significance of white light polar plumes in the solar corona

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....90..344s&link_type=abstract

Astronomy and Astrophysics, vol. 90, no. 3, Oct. 1980, p. 344-349. Research supported by the Centre National de la Recherche Sc

Astronomy and Astrophysics

Astrophysics

4

Coronal Holes, Solar Corona, Solar Eclipses, Solar Flares, Astronomical Photography, Polar Caps, Temperature Distribution, Visual Observation

Scientific paper

Using white light photographs of the 30 June 1973 solar eclipse, it is shown that the plumes observed on the south pole are the upper parts of jets originating at the edge of the polar coronal hole (filament channel). A density and temperature model is derived which confirms this interpretation. It is deduced that the XUV plumes associated with bright points do not generally correspond to the white light polar plumes.

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