Solar active longitudes and their rotation

Abstract In this thesis solar active longitudes of X-ray flares and sunspots are studied. The fact that solar activity does not occur uniformly at all heliographic longitudes was noticed by Carrington as early as in 1843. The longitude ranges where solar activity occurs preferentially are called act...

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Main Author: Zhang, L. (Liyun)
Other Authors: Mursula, K. (Kalevi)
Format: Doctoral Thesis
Language:English
Published: University of Oulu 2013
Subjects:
Online Access:http://urn.fi/urn:isbn:9789526200262
http://nbn-resolving.de/urn:isbn:9789526200262
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spelling ndltd-oulo.fi-oai-oulu.fi-isbn978-952-62-0026-22017-10-14T04:16:33ZSolar active longitudes and their rotationZhang, L. (Liyun)info:eu-repo/semantics/openAccess© University of Oulu, 2013info:eu-repo/semantics/altIdentifier/pissn/1239-4327X-ray flaresactive longitudessolar activitysolar rotationsunspotsAbstract In this thesis solar active longitudes of X-ray flares and sunspots are studied. The fact that solar activity does not occur uniformly at all heliographic longitudes was noticed by Carrington as early as in 1843. The longitude ranges where solar activity occurs preferentially are called active longitudes. Active longitudes have been found in various manifestations of solar activity, such as sunspots, flares, radio emission bursts, surface and heliospheric magnetic fields, and coronal emissions. However, the active longitudes found when using different rigidly rotating reference frames differ significantly from each other. One reason is that the whole Sun does not rotate rigidly but differentially at different layers and different latitudes. The other reason is that the rotation of the Sun also varies with time. Earlier studies used a dynamic rotation frame for the differential rotation of the Sun and found two persistent active longitudes of sunspots in 1878-1996. However, the migration of active longitudes with respect to the Carrington rotation was treated there rather coarsely. We improved the accuracy of migration to less than one hour. Accordingly, not only the rotation parameters for each class of solar flares and sunspots are found to agree well with each other, but also the non-axisymmetry of flares and sunspots is systematically increased. We also studied the long-term variation of solar surface rotation. Using the improved analysis, the spatial distribution of sunspots in 1876-2008 is analyzed. The statistical evidence for different rotation in the northern and southern hemispheres is greatly improved by the revised treatment. Moreover, we have given consistent evidence for the periodicity of about one century in the north-south difference.University of OuluMursula, K. (Kalevi)Usoskin, I. (Ilya)2013-01-29info:eu-repo/semantics/doctoralThesisinfo:eu-repo/semantics/publishedVersionapplication/pdfhttp://urn.fi/urn:isbn:9789526200262urn:isbn:9789526200262eng
collection NDLTD
language English
format Doctoral Thesis
sources NDLTD
topic X-ray flares
active longitudes
solar activity
solar rotation
sunspots
spellingShingle X-ray flares
active longitudes
solar activity
solar rotation
sunspots
Zhang, L. (Liyun)
Solar active longitudes and their rotation
description Abstract In this thesis solar active longitudes of X-ray flares and sunspots are studied. The fact that solar activity does not occur uniformly at all heliographic longitudes was noticed by Carrington as early as in 1843. The longitude ranges where solar activity occurs preferentially are called active longitudes. Active longitudes have been found in various manifestations of solar activity, such as sunspots, flares, radio emission bursts, surface and heliospheric magnetic fields, and coronal emissions. However, the active longitudes found when using different rigidly rotating reference frames differ significantly from each other. One reason is that the whole Sun does not rotate rigidly but differentially at different layers and different latitudes. The other reason is that the rotation of the Sun also varies with time. Earlier studies used a dynamic rotation frame for the differential rotation of the Sun and found two persistent active longitudes of sunspots in 1878-1996. However, the migration of active longitudes with respect to the Carrington rotation was treated there rather coarsely. We improved the accuracy of migration to less than one hour. Accordingly, not only the rotation parameters for each class of solar flares and sunspots are found to agree well with each other, but also the non-axisymmetry of flares and sunspots is systematically increased. We also studied the long-term variation of solar surface rotation. Using the improved analysis, the spatial distribution of sunspots in 1876-2008 is analyzed. The statistical evidence for different rotation in the northern and southern hemispheres is greatly improved by the revised treatment. Moreover, we have given consistent evidence for the periodicity of about one century in the north-south difference.
author2 Mursula, K. (Kalevi)
author_facet Mursula, K. (Kalevi)
Zhang, L. (Liyun)
author Zhang, L. (Liyun)
author_sort Zhang, L. (Liyun)
title Solar active longitudes and their rotation
title_short Solar active longitudes and their rotation
title_full Solar active longitudes and their rotation
title_fullStr Solar active longitudes and their rotation
title_full_unstemmed Solar active longitudes and their rotation
title_sort solar active longitudes and their rotation
publisher University of Oulu
publishDate 2013
url http://urn.fi/urn:isbn:9789526200262
http://nbn-resolving.de/urn:isbn:9789526200262
work_keys_str_mv AT zhanglliyun solaractivelongitudesandtheirrotation
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