Processes observable in the photosphere during the formation of an active region. III - Development of an active region at the edge of an older bipolar magnetic field

Details Processes observable in the photosphere during the formation of an active region. III - Development of an active region at the edge of an older bipolar magnetic field Processes observable in the photosphere during the formation of an active region. III - Development of an active region at the edge of an older bipolar magnetic field

Aug 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984baicz..35..224b&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 35, Aug. 1984, p. 224-232.

Astronomy and Astrophysics

Astronomy

5

Photosphere, Solar Activity, Solar Magnetic Field, Magnetic Field Configurations, Sunspots

Scientific paper

Processes visible during several impulses of new sunspot formations at the periphery of an older large background magnetic field body, in which one rotation earlier the large June-July 1974 proton-flare region developed, are discussed. The coalescence of separate nuclei into the future umbra and the counter-clockwise rotation of the whole leading region, the change of the rotational sense during its further development, as well as the non-simultaneous development of individual parts of the active region are underlined.

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