Other
Scientific paper
Jan 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001esasp.464..115m&link_type=abstract
In: Proceedings of the SOHO 10/GONG 2000 Workshop: Helio- and asteroseismology at the dawn of the millennium, 2-6 October 2000,
Other
1
Sun: Global Solar Cycle, Magnetic Fields, Poleward Migration Rate
Scientific paper
We show that the velocity of poleward migration of the magnetic fields is a linear function of the "strength of the solar cycle". We introduce a new index "the strength of the solar cycle" and represent this quantitatively by the two parameters: Σminrev Ssp - summation of all the annual means of sunspot areas Ssp of the cycle for the N and S hemispheres separately starting from the lowest value of the annual mean in Ssp in the minimum phase all the way to the year of the polarity reversal and Σminrev W - summation of the Wolf numbers as done for Σminrev Ssp but over the entire visible hemisphere. Each of these parameters according to us represents the "strength of the solar cycle" although they are not independent of each other. We also discuss some questions regarding the role of the meridional circulation in transporting the fields towards the poles.
Callebaut Dirk K.
Makarov Valentin I.
Sivaraman K. R.
Tlatov Andrej G.
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