Time-Latitude Prominence and the Green Corona Distribution Over the Solar Activity Cycle
Abstract We present a distribution of prominences over the solar cycle activity. There are found both polar and equatorial branches of prominences that migrate in opposite directions. Prominences of the high-latitude crown migrate, starting in the minimum of the cycle, towards the poles, which they...
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Language: | English |
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Cambridge University Press (CUP)
1998
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Online Access: | http://dx.doi.org/10.1017/s0252921100048132 https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S0252921100048132 |
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crcambridgeupr:10.1017/s0252921100048132 2024-04-28T08:31:57+00:00 Time-Latitude Prominence and the Green Corona Distribution Over the Solar Activity Cycle Minarovjech, M. Rybanský, M. Rušin, V. 1998 http://dx.doi.org/10.1017/s0252921100048132 https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S0252921100048132 en eng Cambridge University Press (CUP) https://www.cambridge.org/core/terms International Astronomical Union Colloquium volume 167, page 484-487 ISSN 0252-9211 journal-article 1998 crcambridgeupr https://doi.org/10.1017/s0252921100048132 2024-04-02T06:54:09Z Abstract We present a distribution of prominences over the solar cycle activity. There are found both polar and equatorial branches of prominences that migrate in opposite directions. Prominences of the high-latitude crown migrate, starting in the minimum of the cycle, towards the poles, which they reach at the maximum of the cycle and then decay. The equatorward-migrating branch of prominences appears also in the minimum of the cycle at mid-latitudes and disappears at the end of the cycle. The distribution of the prominences is compared with a time-latitudinal distribution of the green corona. It is assumed that the polar branches in cycle 23 will reach the poles in 2002 (the north pole) and 2003 (the south one), respectively. Article in Journal/Newspaper North Pole Cambridge University Press International Astronomical Union Colloquium 167 484 487 |
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Open Polar |
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Cambridge University Press |
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crcambridgeupr |
language |
English |
description |
Abstract We present a distribution of prominences over the solar cycle activity. There are found both polar and equatorial branches of prominences that migrate in opposite directions. Prominences of the high-latitude crown migrate, starting in the minimum of the cycle, towards the poles, which they reach at the maximum of the cycle and then decay. The equatorward-migrating branch of prominences appears also in the minimum of the cycle at mid-latitudes and disappears at the end of the cycle. The distribution of the prominences is compared with a time-latitudinal distribution of the green corona. It is assumed that the polar branches in cycle 23 will reach the poles in 2002 (the north pole) and 2003 (the south one), respectively. |
format |
Article in Journal/Newspaper |
author |
Minarovjech, M. Rybanský, M. Rušin, V. |
spellingShingle |
Minarovjech, M. Rybanský, M. Rušin, V. Time-Latitude Prominence and the Green Corona Distribution Over the Solar Activity Cycle |
author_facet |
Minarovjech, M. Rybanský, M. Rušin, V. |
author_sort |
Minarovjech, M. |
title |
Time-Latitude Prominence and the Green Corona Distribution Over the Solar Activity Cycle |
title_short |
Time-Latitude Prominence and the Green Corona Distribution Over the Solar Activity Cycle |
title_full |
Time-Latitude Prominence and the Green Corona Distribution Over the Solar Activity Cycle |
title_fullStr |
Time-Latitude Prominence and the Green Corona Distribution Over the Solar Activity Cycle |
title_full_unstemmed |
Time-Latitude Prominence and the Green Corona Distribution Over the Solar Activity Cycle |
title_sort |
time-latitude prominence and the green corona distribution over the solar activity cycle |
publisher |
Cambridge University Press (CUP) |
publishDate |
1998 |
url |
http://dx.doi.org/10.1017/s0252921100048132 https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S0252921100048132 |
genre |
North Pole |
genre_facet |
North Pole |
op_source |
International Astronomical Union Colloquium volume 167, page 484-487 ISSN 0252-9211 |
op_rights |
https://www.cambridge.org/core/terms |
op_doi |
https://doi.org/10.1017/s0252921100048132 |
container_title |
International Astronomical Union Colloquium |
container_volume |
167 |
container_start_page |
484 |
op_container_end_page |
487 |
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1797589299189776384 |