The sunspot cycle no. 24 in relation to long term solar activity variation

The solar minimum between solar cycles 23 and 24 during the period 2007–2009 has been the longest and deepest one at least since for the last 100 years. We suggest that the Sun is going to his next supercenturial minimum. The main aim of this paper is to tell about arguments concerning this statemen...

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Autores principales: Komitov, Boris, Kaftan, Vladimir
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Elsevier 2013
Materias:
Original Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4295042/
https://www.ncbi.nlm.nih.gov/pubmed/25685429
http://dx.doi.org/10.1016/j.jare.2013.02.001
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author Komitov, Boris
Kaftan, Vladimir
author_facet Komitov, Boris
Kaftan, Vladimir
author_sort Komitov, Boris
collection PubMed
description The solar minimum between solar cycles 23 and 24 during the period 2007–2009 has been the longest and deepest one at least since for the last 100 years. We suggest that the Sun is going to his next supercenturial minimum. The main aim of this paper is to tell about arguments concerning this statement. They are based on series of studies, which have been provided during the period since 1997 up to 2010. The progress of solar cycle 24 since its minimum at the end of 2008 up to the end of October 2011 in the light of long term solar activity dynamics is analyzed.
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spelling pubmed-42950422015-02-14 The sunspot cycle no. 24 in relation to long term solar activity variation Komitov, Boris Kaftan, Vladimir J Adv Res Original Article The solar minimum between solar cycles 23 and 24 during the period 2007–2009 has been the longest and deepest one at least since for the last 100 years. We suggest that the Sun is going to his next supercenturial minimum. The main aim of this paper is to tell about arguments concerning this statement. They are based on series of studies, which have been provided during the period since 1997 up to 2010. The progress of solar cycle 24 since its minimum at the end of 2008 up to the end of October 2011 in the light of long term solar activity dynamics is analyzed. Elsevier 2013-05 2013-03-30 /pmc/articles/PMC4295042/ /pubmed/25685429 http://dx.doi.org/10.1016/j.jare.2013.02.001 Text en © 2013 Cairo University. Production and hosting by Elsevier B.V. All rights reserved. http://creativecommons.org/licenses/by-nc-nd/3.0/ This is an open access article under the CC BY-NC-ND license (http://creativecommons.org/licenses/by-nc-nd/3.0/).
spellingShingle Original Article
Komitov, Boris
Kaftan, Vladimir
The sunspot cycle no. 24 in relation to long term solar activity variation
title The sunspot cycle no. 24 in relation to long term solar activity variation
title_full The sunspot cycle no. 24 in relation to long term solar activity variation
title_fullStr The sunspot cycle no. 24 in relation to long term solar activity variation
title_full_unstemmed The sunspot cycle no. 24 in relation to long term solar activity variation
title_short The sunspot cycle no. 24 in relation to long term solar activity variation
title_sort sunspot cycle no. 24 in relation to long term solar activity variation
topic Original Article
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4295042/
https://www.ncbi.nlm.nih.gov/pubmed/25685429
http://dx.doi.org/10.1016/j.jare.2013.02.001
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