Differential rotation and reconnection as basic causes of some coronal reorientations

Details Differential rotation and reconnection as basic causes of some coronal reorientations Differential rotation and reconnection as basic causes of some coronal reorientations

Oct 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975soph...44..503h&link_type=abstract

Solar Physics, vol. 44, Oct. 1975, p. 503-508.

Physics

8

Magnetic Field Configurations, Solar Corona, Solar Cycles, Solar Magnetic Field, Solar Rotation, Lines Of Force, Magnetic Flux, Photosphere, Polar Regions, Sunspots

Scientific paper

A process is suggested by which a coronal structure (with underlying filament) may form between a polar crown structure and a low-latitude bipolar region. During the ascending phase of the solar cycle the identifying underlying filament should lie poleward and westward of the active region, but during the descending phase it should appear as an eastward extension of the filament separating leader and follower photospheric fields within the active region.

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