Differential rotation of chromosphere and photosphere in the rising phase of N22 cycle of the Sun: torsional oscillations

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 pra...

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Veröffentlicht in:Кинематика и физика небесных тел
Datum:2005
Hauptverfasser: Kasinskii, V., Kasinskaia, L.I.
Format: Artikel
Sprache:English
Veröffentlicht: Головна астрономічна обсерваторія НАН України 2005
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Online Zugang:https://nasplib.isofts.kiev.ua/handle/123456789/79641
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Zitieren: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.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
id nasplib_isofts_kiev_ua-123456789-79641
record_format dspace
spelling Kasinskii, V.
Kasinskaia, L.I.
2015-04-03T16:55:22Z
2015-04-03T16:55:22Z
2005
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.
0233-7665
https://nasplib.isofts.kiev.ua/handle/123456789/79641
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.
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.
en
Головна астрономічна обсерваторія НАН України
Кинематика и физика небесных тел
MS2: Physics of Solar Atmosphere
Differential rotation of chromosphere and photosphere in the rising phase of N22 cycle of the Sun: torsional oscillations
Article
published earlier
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
title Differential rotation of chromosphere and photosphere in the rising phase of N22 cycle of the Sun: torsional oscillations
spellingShingle Differential rotation of chromosphere and photosphere in the rising phase of N22 cycle of the Sun: torsional oscillations
Kasinskii, V.
Kasinskaia, L.I.
MS2: Physics of Solar Atmosphere
title_short Differential rotation of chromosphere and photosphere in the rising phase of N22 cycle of the Sun: torsional oscillations
title_full Differential rotation of chromosphere and photosphere in the rising phase of N22 cycle of the Sun: torsional oscillations
title_fullStr Differential rotation of chromosphere and photosphere in the rising phase of N22 cycle of the Sun: torsional oscillations
title_full_unstemmed Differential rotation of chromosphere and photosphere in the rising phase of N22 cycle of the Sun: torsional oscillations
title_sort differential rotation of chromosphere and photosphere in the rising phase of n22 cycle of the sun: torsional oscillations
author Kasinskii, V.
Kasinskaia, L.I.
author_facet Kasinskii, V.
Kasinskaia, L.I.
topic MS2: Physics of Solar Atmosphere
topic_facet MS2: Physics of Solar Atmosphere
publishDate 2005
language English
container_title Кинематика и физика небесных тел
publisher Головна астрономічна обсерваторія НАН України
format Article
description 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.
issn 0233-7665
url https://nasplib.isofts.kiev.ua/handle/123456789/79641
citation_txt 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.
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