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Role of the large-scale solar magnetic field structure in the global organization of solar activity

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Abstract

The relation of the large-scale solar magnetic field structure to the most pronounced manifestations of solar activity (filaments, active regions, sunspots, coronal mass ejections, and coronal holes) has been studied.

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Authors and Affiliations

  1. Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radiowave Propagation, Russian Academy of Sciences, Troitsk, Moscow oblast, 142190, Russia

    E. V. Ivanov & V. N. Obridko

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  1. E. V. Ivanov
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  2. V. N. Obridko
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Correspondence to E. V. Ivanov.

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Ivanov, E.V., Obridko, V.N. Role of the large-scale solar magnetic field structure in the global organization of solar activity. Geomagn. Aeron. 54, 996–999 (2014). https://doi.org/10.1134/S0016793214080076

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  • DOI: https://doi.org/10.1134/S0016793214080076

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