Relation of the green coronal line intensity to sunspot areas and magnetic fields of different scales

Author:

Badalyan O. G.,Bludova N. G.

Publisher

Pleiades Publishing Ltd

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference36 articles.

1. Altrock, R., Howe, R., and Ulrich, R., Solar torsional oscillations and their relationship to coronal activity, in Subsurface and Atmospheric Influences on Solar Activity, Howe, R., Komm, R.W., and Balasubramaniam, K.S., Eds., San Francisco, 2008, p. 335.

2. Altrock, R.C., Coronal Fe XIV emission during the whole heliosphere interval campaign, Solar Phys., 2011, vol. 274, pp. 251–257.

3. Altrock, R.C., Forecasting the maxima of solar cycle 24 with coronal Fe XIV emission, Solar Phys., 2013. doi: 10.1007/s11207-012-0216-1

4. Badalyan, O.G. and Obridko, V.N., Relationship between the coronal green line brightness and magneticfield strength, in Proc. 223rd IAU Symp. “Multi-Wavelength Investigations of Solar Activity,” Stepanov, A.V., Benevolenskaya, E.E., and Kosovichev, A.G., Eds., 2004a, pp. 371–372.

5. Badalyan, O.G. and Obridko, V.N., Solar magnetic fields and the intensity of the green coronal line, Astron. Rep., 2004b, vol. 48, no. 8, p. 678.

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