On the correspondence between the coronal green-line brightness, magnetic field strength and some sunspot activity indices

Details On the correspondence between the coronal green-line brightness, magnetic field strength and some sunspot activity indices On the correspondence between the coronal green-line brightness, magnetic field strength and some sunspot activity indices

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005a%26at...24...39b&link_type=abstract

Astronomical and Astrophysical Transactions, vol. 24, Issue 1, p.39-44

Astronomy and Astrophysics

Astronomy

1

Sun, Corona, Coronal Green Line, Coronal Magnetic Field, Sunspots

Scientific paper

The coronal green-line brightness and strength of the large-scale magnetic field on synoptic maps have been compared with the areas and positions of sunspots. Good correspondence is shown to exist between these parameters in some periods close to the sunspot minimum. However, this is not a general rule, and the correspondence is violated in the epochs of high solar activity. One may suggest that this is the effect of the existence of solar magnetic fields of different spatial scales.

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