Pulsed nature of solar cycle 24

Author:

Benevolenskaya E. E.,Ponyavin Yu. D.

Publisher

Pleiades Publishing Ltd

Subject

Space and Planetary Science,Geophysics

Reference19 articles.

1. Antalova, A. and Gnevyshev, M.N., Latitudinal distribution of sunspot areas during the period 1874–1976, Astron. Inst. Czech. Bul., 1985, vol. 36, p. 61.

2. Benevolenskaya, E.E., A topological model of the solar magnetic field reversals, The Sun and Cool Stars, Tuominen, I., Moss, D., and Rudiger, G., Eds., Springer, 1991, vol. 380, pp. 234–236.

3. Benevolenskaya, E.E., Origin of the polar magnetic field reversals, Sol. Phys., 1996, vol. 167, pp. 47–55.

4. Benevolenskaya, E.E., A model of the double magnetic cycle of the Sun, Astrophys. J., 1998, vol. 509, pp. L49–L52.

5. Benevolenskaya, E.E., Kosovichev, A.G., and Scherrer, P.H., Detection of high-latitude waves of solar coronal activity in extreme-ultraviolet data from the solar and heliospheric observatory EUV imaging telescope, Astrophys. J., 2001, vol. 554, pp. L107–110.

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