On the long-term variability of the green corona accordingly to four existing databases

We examine four long-term databases of monthly means of the whole disc green coronal brightness which cover the period of the last five and a half solar cycles to verify them, and compare their usefulness, as indices characterize the solar activity. We use the data from (1) the Norikura Observatory,...

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Published in:Кинематика и физика небесных тел
Date:2005
Main Authors: Kobylinski, Z., Baranska, A., Ajabshirizadeh, A.
Format: Article
Language:English
Published: Головна астрономічна обсерваторія НАН України 2005
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Online Access:https://nasplib.isofts.kiev.ua/handle/123456789/79618
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Journal Title:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Cite this:On the long-term variability of the green corona accordingly to four existing databases / Z. Kobylinski, A. Baranska, A. Ajabshirizadeh // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 129-133. — Бібліогр.: 20 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
id nasplib_isofts_kiev_ua-123456789-79618
record_format dspace
spelling Kobylinski, Z.
Baranska, A.
Ajabshirizadeh, A.
2015-04-03T15:39:06Z
2015-04-03T15:39:06Z
2005
On the long-term variability of the green corona accordingly to four existing databases / Z. Kobylinski, A. Baranska, A. Ajabshirizadeh // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 129-133. — Бібліогр.: 20 назв. — англ.
0233-7665
https://nasplib.isofts.kiev.ua/handle/123456789/79618
We examine four long-term databases of monthly means of the whole disc green coronal brightness which cover the period of the last five and a half solar cycles to verify them, and compare their usefulness, as indices characterize the solar activity. We use the data from (1) the Norikura Observatory, (2) the Kislovodsk Observatory, (3) intensities detected by several coronographs and converted to the common photometric scale of Pic du Midi, (4) coronal indices obtained from detections of several observatories and converted to the photometric scale of Lomnicky Stit. We compare them by means of correlative analysis with the time series of sunspot numbers. The data (2) demonstrate the best agreement with sunspot number as the reference (r = 0.88).
We acknowledge the Main Astronomical Observatory, Kyiv, Ukraine, for the financial support in participation in the MAO-2004 Conference and we thank Dr. V. Rusin and Dr. T. Sakurai for sending the GCL data sets.
en
Головна астрономічна обсерваторія НАН України
Кинематика и физика небесных тел
MS2: Physics of Solar Atmosphere
On the long-term variability of the green corona accordingly to four existing databases
Article
published earlier
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
title On the long-term variability of the green corona accordingly to four existing databases
spellingShingle On the long-term variability of the green corona accordingly to four existing databases
Kobylinski, Z.
Baranska, A.
Ajabshirizadeh, A.
MS2: Physics of Solar Atmosphere
title_short On the long-term variability of the green corona accordingly to four existing databases
title_full On the long-term variability of the green corona accordingly to four existing databases
title_fullStr On the long-term variability of the green corona accordingly to four existing databases
title_full_unstemmed On the long-term variability of the green corona accordingly to four existing databases
title_sort on the long-term variability of the green corona accordingly to four existing databases
author Kobylinski, Z.
Baranska, A.
Ajabshirizadeh, A.
author_facet Kobylinski, Z.
Baranska, A.
Ajabshirizadeh, A.
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 We examine four long-term databases of monthly means of the whole disc green coronal brightness which cover the period of the last five and a half solar cycles to verify them, and compare their usefulness, as indices characterize the solar activity. We use the data from (1) the Norikura Observatory, (2) the Kislovodsk Observatory, (3) intensities detected by several coronographs and converted to the common photometric scale of Pic du Midi, (4) coronal indices obtained from detections of several observatories and converted to the photometric scale of Lomnicky Stit. We compare them by means of correlative analysis with the time series of sunspot numbers. The data (2) demonstrate the best agreement with sunspot number as the reference (r = 0.88).
issn 0233-7665
url https://nasplib.isofts.kiev.ua/handle/123456789/79618
citation_txt On the long-term variability of the green corona accordingly to four existing databases / Z. Kobylinski, A. Baranska, A. Ajabshirizadeh // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 129-133. — Бібліогр.: 20 назв. — англ.
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first_indexed 2025-11-30T18:25:51Z
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