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: | , |
| Format: | Artikel |
| Sprache: | English |
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Головна астрономічна обсерваторія НАН України
2005
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| Online Zugang: | https://nasplib.isofts.kiev.ua/handle/123456789/79641 |
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| Назва журналу: | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| 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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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. |
| work_keys_str_mv |
AT kasinskiiv differentialrotationofchromosphereandphotosphereintherisingphaseofn22cycleofthesuntorsionaloscillations AT kasinskaiali differentialrotationofchromosphereandphotosphereintherisingphaseofn22cycleofthesuntorsionaloscillations |
| first_indexed |
2025-12-07T18:28:49Z |
| last_indexed |
2025-12-07T18:28:49Z |
| _version_ |
1850875187599245312 |