Do prominences migrate equatorwards?

Details Do prominences migrate equatorwards? Do prominences migrate equatorwards?

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984soph...93..393m&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 93, July 1984, p. 393-396.

Physics

21

Equatorial Atmosphere, Solar Magnetic Field, Solar Prominences, H Alpha Line, Latitude, Solar Cycles

Scientific paper

The mean latitude of prominence samples referring to one boundary of the polarity division line of the large-scale magnetic field is calculated on the basis of Hα charts in the period 1955 - 1982. It is shown that the magnetic field in that period had a latitude zonal structure. The boundaries of the latitude zones of the magnetic field had no regular equatorwards migration. They either oscillated near the mean boundaries at 0°, ±20°, ±40°, or migrated polewards.

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