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Concerning time variation observations of the global magnetic field of the Sun

โœ Scribed by M. L. Demidov

Publisher
Springer
Year
1995
Tongue
English
Weight
297 KB
Volume
159
Category
Article
ISSN
0038-0938

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๐Ÿ“œ SIMILAR VOLUMES

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โœ V. M. Grigoryev; M. L. Demidov ๐Ÿ“‚ Article ๐Ÿ“… 1991 ๐Ÿ› Springer ๐ŸŒ English โš– 415 KB

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

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The energetical aspect of solar phenomena of different spatial and time scales has been studied with special attention to global magnetic fields, Cyclic regularities in the heliosphere are determined by energetics of global magnetic fields. The energy variation of global fields consists of a number

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Based on an analysis of the latitude and longitude regularities in the distribution of the sign of the background magnetic field (BMF) on the solar surface for 14 years (1969)(1970)(1971)(1972)(1973)(1974)(1975)(1976)(1977)(1978)(1979)(1980)(1981)(1982), a classification of BMF distributions in the