Active longitudes of sunspots

Details Active longitudes of sunspots Active longitudes of sunspots

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ge%26ae..49..866o&link_type=abstract

Geomagnetism and Aeronomy, Volume 49, Issue 7, pp.866-870

Physics

1

Scientific paper

The inhomogeneity of the sunspot group longitude distribution has been determined depending on the rotation period used to determine a longitude. The statistical significance of the found active longitudes has been estimated. It has been indicated that a rather high reliability is reached only when the synodic rotation period is close to 27 and 28 days. In this case active longitudes show the long-term variation related to the north-south asymmetry of the sunspot formation. It is assumed that active longitudes are related to the relic magnetic field frozen in a uniformly rotating solar radiative zone.

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