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Variations of the sun's diameter

Publisher
Elsevier Science
Year
1885
Tongue
English
Weight
65 KB
Volume
120
Category
Article
ISSN
0016-0032

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๐Ÿ“œ SIMILAR VOLUMES

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It is presumed that a north-southern asymmetry of a solid-body rotation of large spots, depending on even and odd solar activity cycles (Gigolashvili and Khutsishvilil 1989, 1990) may possibly be explained by the asymmetry of the appearance of large structures with strong magnetic fields in the corr

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For the purpose of identifying five-min oscillations we analyze long-term continuous observations of the solar magnetic field (with a duration from 3 to 11 hours) with 0.5 D e spatial resolution obtained with the STOP telescope (Solar Telescope for Operative Predictions) at the Sayan observatory in