Solar active longitudes and their rotation
1University of Oulu, Faculty of Science, Department of Physics
|Online Access:||PDF Full Text (PDF, 2.7 MB)|
|Persistent link:|| http://urn.fi/urn:isbn:9789526200262
|Publish Date:|| 2013-01-29
|Thesis type:||Doctoral Dissertation
|Defence Note:||Academic dissertation to be presented, with the permission of the Faculty of
Science of the University of Oulu, for public discussion in the Auditorium L6,
Linnanmaa, on 30th November, 2012, at 12 o’clock noon.
Professor Kalevi Mursula
Professor Ilya Usoskin
Professor Roman Brajša
Associate Professor Dmitri Ivanovitch Ponyavin
Doctor Rainer Arlt
Professor Kalevi Mursula
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.
Report series in physical sciences
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