Computer Science
Scientific paper
Sep 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.535...59a&link_type=abstract
In: Solar variability as an input to the Earth's environment. International Solar Cycle Studies (ISCS) Symposium, 23 - 28 June 2
Computer Science
Solar Magnetic Field
Scientific paper
Total intensity of the magnetic field is derived from the radial values of large-scale magnetic field measured on WSO of Stanford University. Horizontal component of the magnetic field in and above the photosphere was derived by computing of the current free approximation, all for each Carrington rotation in the time interval from year 1976 to 2000. Spatial distribution of the enhanced regions of the total magnetic flux was studied during the activity cycle. Time-longitude evolution of the total flux patterns was tested in relationship with both positive and negative polarities evolution in solar photosphere. Close relationship between enhanced magnetic flux regions and the green corona bright regions is found. The study brings a new light on the problem of the "coronal rotation".
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