Solar cycle variation of large-scale coronal structures

Details Solar cycle variation of large-scale coronal structures Solar cycle variation of large-scale coronal structures

Oct 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974soph...38..439a&link_type=abstract

Solar Physics, vol. 38, Oct. 1974, p. 439-447.

Physics

3

Interplanetary Magnetic Fields, Line Spectra, Photosphere, Solar Corona, Solar Cycles, Solar Magnetic Field, Luminous Intensity, Magnetic Field Configurations, Periodic Variations, Polarity

Scientific paper

A green line intensity variation is associated with the interplanetary and photospheric magnetic sector structure. This effect depends on the solar cycle and occurs with the same amplitude in the latitude range 60 N-60 S. Extended longitudinal coronal structures are suggested, which indicate the existence of closed magnetic field lines over the neutral line, separating adjacent regions of opposite polarities on the photospheric surface.

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