Structure of coronal rays

Details Structure of coronal rays Structure of coronal rays

Oct 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993azh....70.1092v&link_type=abstract

Astronomicheskij Zhurnal, vol. 70, p. 1092

Astronomy and Astrophysics

Astronomy

2

Solar Corona, Electron Density (Concentration), Solar Magnetic Field, Lines Of Force, Sunlight, Solar Electrons, Continuity Equation, Plasma Density

Scientific paper

The ray structures of the corona are treated as folds and plies of magnetic surfaces with a large gradient of electron density when projected to the picture plane. The number of the intersections of the rays with an arbitrary closed contour in the projection plane is shown to be even. This allows the classification of the singular points of the observed structures. Such a classification is performed, and results of an analysis of singular points of the corona are presented for the period 1936-1984.

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