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dc.contributor.author |
Leiko, U.M. |
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dc.date.accessioned |
2015-04-03T16:54:03Z |
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dc.date.available |
2015-04-03T16:54:03Z |
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dc.date.issued |
2005 |
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dc.identifier.citation |
Large-scale magnetic fields of Sun-heliosphere magnetic system / U.M. Leiko // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 187-188. — Бібліогр.: 3 назв. — англ. |
uk_UA |
dc.identifier.issn |
0233-7665 |
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dc.identifier.uri |
http://dspace.nbuv.gov.ua/handle/123456789/79640 |
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dc.description.abstract |
Some results of investigations of solar and interplanetary magnetic fields are presented. The time series of the solar background magnetic field (SBMF) of ±20 degree for 1904–2000, solar mean magnetic field (SMMF) for 1975–2003, and interplanetary magnetic field (IMF) for 1947–2001 were used. A change of the Sun’s rotation regime in the middle of the 20th century is confirmed. The rotation of the sector structures of SBMF, SMMF, and IMF had not identical character during common interval of the observations. |
uk_UA |
dc.description.sponsorship |
I would like to thank all the observers for the possibility to work with LSMF data, and the Organizing Committee for giving me a chance to represent this paper at the Conference. |
uk_UA |
dc.language.iso |
en |
uk_UA |
dc.publisher |
Головна астрономічна обсерваторія НАН України |
uk_UA |
dc.relation.ispartof |
Кинематика и физика небесных тел |
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dc.subject |
MS2: Physics of Solar Atmosphere |
uk_UA |
dc.title |
Large-scale magnetic fields of Sun-heliosphere magnetic system |
uk_UA |
dc.type |
Article |
uk_UA |
dc.status |
published earlier |
uk_UA |
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