MHD nature of the origination, dynamics, geoeffectiveness, and disappearance of the four-sector structure of the solar magnetic field during the cycle 23 decline phase-Reference-Cited by-同舟云学术

MHD nature of the origination, dynamics, geoeffectiveness, and disappearance of the four-sector structure of the solar magnetic field during the cycle 23 decline phase

Published:2009-06 Issue:3 Volume:49 Page:273-289
ISSN:0016-7932
Container-title:Geomagnetism and Aeronomy
language:en
Short-container-title:Geomagn. Aeron.

Author:

Ivanov K. G.,Kharshiladze A. F.

Publisher

Pleiades Publishing Ltd

Subject

Space and Planetary Science,Geophysics

Link

http://link.springer.com/content/pdf/10.1134/S0016793209030013.pdf

Reference20 articles.

1. E. Gibson, The Quiet Sun (NASA, Washington, D.C., 1973; Mir, Moscow, 1977).

2. K. G. Ivanov and A. F. Kharshiladze, “Intersector Disbalance of the Large-Scale Open Solar Magnetic Field Fluxes, Active and Passive Boundaries, and Solar-Terrestrial Extrastorms,” Geomagn. Aeron. 48(5), 605–622 (2008) [Geomagn. Aeron. 48, 578–594 (2008)].

3. K. G. Ivanov and A. F. Kharshiladze, “The Series of Solar-Terrestrial Superstorms of May–October, 2000. 1. Structure and Dynamics of the Open Solar Magnetic Field,” Geomagn. Aeron. 44(1), 1–8 (2004) [Geomagn. Aeron. 44, 1–6 (2004)].

4. K. G. Ivanov and A. F. Kharshiladze, “Solar-Terrestrial Extrastorm of August 22–24, 2005. 1. Solar Sources,” Geomagn. Aeron. 47(1), 27–32 (2007) [Geomagn. Aeron. 47, 23–28 (2007)].

5. K. G. Ivanov and A. F. Kharshiladze, “Solar-Terrestrial Storms of October 2003. 2. Five-Phase Dynamics of the Substorm of October 28–30,” Geomagn. Aeron. 47(6), 831–847 (2007a) [Geomagn. Aeron. 47, 787–802 (2007a)].

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