Integral Properties of Solar Active Regions

Details Integral Properties of Solar Active Regions Integral Properties of Solar Active Regions

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003a%26at...22..335c&link_type=abstract

Astronomical and Astrophysical Transactions, vol. 22, Issue 3, p.335-355

Mathematics

Logic

2

Scientific paper

In the paper the results of investigations on ten solar active regions are presented. The main results are as follows: firstly, the total down-flow velocity exceeds the up-flow velocity by about two orders of magnitude in all the active regions; secondly, no correlation was found between the mean integral velocity flux and the mean integral magnetic flux for all the active regions; thirdly, it was found that, besides a direct correlation between the total sunspot area and the total magnetic flux in active regions, occasionally there is an inverse correlation between these parameters, and the inverse correlation times often corresponded to the structural and topological rebuilding of magnetic flux in the active regions; fourthly, a good correlation was found between some parameters of integral fluxes (magnetic and velocity) and X-ray flux variations.

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