Computer Science
Scientific paper
Aug 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd...3e..21b&link_type=abstract
Solar Active Regions and 3D Magnetic Structure, 26th meeting of the IAU, Joint Discussion 3, 16-17 August, 2006, Prague, Czech R
Computer Science
Scientific paper
Comparisons of the Fe XIV 530.3 nm coronal line brightness with the summary area of sunspots and with the magnetic field strength,extrapolated from the photospheric measurements for the 0.1 R[O ]height in the corona, are discussed. Different correlations of the green line brightness with the large-scale coronal magnetic fields and with the local fields of sunspots are found during different solar cycle phases. At the ascending phase of activity the large-scale coronal magnetic fields are best correlated, whereas, at the descending phase somewhat higher correlation of the green line brightness with the local magnetic fields of sunspots is observed. Results of this contribution may be useful when testifying various models of the solar corona heating.
Badalyan Olga G.
Bludova N. G.
Sykora Jan
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