Long-term evolution of a high-latitude active region

Details Long-term evolution of a high-latitude active region Long-term evolution of a high-latitude active region

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988soph..117..227m&link_type=abstract

(Solar Cycle Workshop, Meeting, 2nd, Lake Tahoe, CA, May 1987) Solar Physics (ISSN 0038-0938), vol. 117, no. 2, 1988, p. 227-241

Physics

14

Magnetic Signatures, Polarized Radiation, Solar Activity, Solar Cycles, Solar Magnetic Field, H Alpha Line, Solar Observatories, Solar Rotation

Scientific paper

The decay phase of one of the largest active regions of solar cycle 22 that developed by the end of June 1987 is studied. Migration of the magnetic fields northward, poleward, and equatorward is shown to lead to the apparent rotation of the magnetic axis of the region. The sunspot motions and pattern of evolution of the magnetic fields noted provide evidence for the existence of a large-scale velocity field within the active region.

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