Coronal holes and long-lived unipolar magnetic regions

Details Coronal holes and long-lived unipolar magnetic regions Coronal holes and long-lived unipolar magnetic regions

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984basi...12..404s&link_type=abstract

Astronomical Society of India, Bulletin, vol. 12, Dec. 1984, p. 404-410.

Astronomy and Astrophysics

Astronomy

Coronal Holes, Solar Corona, Solar Magnetic Field, Polar Caps, Synoptic Measurement, Temporal Distribution

Scientific paper

Association of coronal holes with long-lived unipolar magnetic regions (LLUMRs) which survived for four solar rotations is examined. It is noticed that every coronal hole fits in well within the LLUMR. The coronal holes are also seen to dissolve as a consequence of the LLUMR boundary zone evolution and emergence of opposite polarity regions within the coronal hole boundary.

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