The meridional motions of stable recurrent sunspots

Details The meridional motions of stable recurrent sunspots The meridional motions of stable recurrent sunspots

Sep 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...249..528l&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 249, no. 2, Sept. 1991, p. 528-532.

Astronomy and Astrophysics

Astrophysics

13

Solar Cycles, Solar Rotation, Spectroheliographs, Sunspots, Data Bases, Photosphere, Solar Wind

Scientific paper

The data bases of the Greenwich photoheliographic results and the similar data from the Kanzelhohe are used to determine meridional motions of a special sample of identical stable recurrent sunspots within the period from 1948 until 1976. The motions are determined by two different methods: from linear fits of the latitudes during the sunspot disk passage and from mean latitudes at about central meridian passages of recurrencies. The latter method is more reliable and allows also to determine an indication for a braking of the meridional motions with aging of the spots.

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