Association of coronal holes with large scale solar magnetic fields

Details Association of coronal holes with large scale solar magnetic fields Association of coronal holes with large scale solar magnetic fields

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984basi...12..357s&link_type=abstract

Astronomical Society of India, Bulletin, vol. 12, Dec. 1984, p. 357-363.

Astronomy and Astrophysics

Astronomy

Coronal Holes, Solar Corona, Solar Magnetic Field, Field Strength, Polarity, Solar Rotation

Scientific paper

The association of coronal holes with large-scale solar magnetic fields has been investigated. It is concluded that coronal holes always form in the large unipolar magnetic field patterns, and no specific polarity rule holds true for low-latitude coronal holes. The coronal holes show a strong tendency to bypass the opposite polarity regions in their location. Coronal holes get fragmented into pieces, if opposite polarity flux encroaches and/or erupts into their boundaries. The migration of coronal holes or their fragments and the growth of coronal holes out of hole fragments are also discussed.

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