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dc.contributor.author |
Kasinskii, V. |
|
dc.contributor.author |
Kasinskaia, L.I. |
|
dc.date.accessioned |
2015-04-03T16:55:22Z |
|
dc.date.available |
2015-04-03T16:55:22Z |
|
dc.date.issued |
2005 |
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dc.identifier.citation |
Differential rotation of chromosphere and photosphere in the rising phase of N22 cycle of the Sun: torsional oscillations / V. Kasinskii, L.I. Kasinskaia // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 189-191. — Бібліогр.: 3 назв. — англ. |
uk_UA |
dc.identifier.issn |
0233-7665 |
|
dc.identifier.uri |
http://dspace.nbuv.gov.ua/handle/123456789/79641 |
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dc.description.abstract |
The angular velocities of chromosphere and photosphere are calculated for 1987–1990 on the basis of heliographic coordinates of the chromospheric flares and sunspots (Solar Geophysical Data). The time resolution accepted is 0.25 year. The mean equatorial rotations of chromosphere and photosphere practically coincide. However, the differential coefficients in the chromosphere and photosphere, b, have strongly different behaviour. The value bch – bph change regularly from “+” sign to “−” sign over two-year interval. Thus, the idea of a torsion like oscillations of “chromosphere–photosphere” is supported. |
uk_UA |
dc.description.sponsorship |
One of the authors should be grateful to Prof. Ya. Yatskiv for official invitation to the MAO-2004 Conference, Kyiv, Ukraine, July 15–17, 2004. |
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 |
|
dc.subject |
MS2: Physics of Solar Atmosphere |
uk_UA |
dc.title |
Differential rotation of chromosphere and photosphere in the rising phase of N22 cycle of the Sun: torsional oscillations |
uk_UA |
dc.type |
Article |
uk_UA |
dc.status |
published earlier |
uk_UA |
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