Restructuring of the Solar Magnetic Fields and Flare Activity Centers in Cycle 24

Autor:	A. V. Mordvinov, E. M. Golubeva, A. V. Borovik, A. A. Zhdanov
Rok vydání:	2020
Předmět:	Physics 010308 nuclear & particles physics Restructuring media_common.quotation_subject Spatiotemporal Analysis Astronomy and Astrophysics Zonal and meridional Astrophysics Solar atmosphere 01 natural sciences Asymmetry Magnetic field law.invention Space and Planetary Science law Physics::Space Physics 0103 physical sciences Astrophysics::Solar and Stellar Astrophysics Astrophysics::Earth and Planetary Astrophysics 010303 astronomy & astrophysics Physics::Atmospheric and Oceanic Physics media_common Flare
Zdroj:	Astronomy Reports. 64:540-546
ISSN:	1562-6881 1063-7729
DOI:	10.1134/s106377292007001x
Popis:	The development of the solar magnetic activity in cycle 24 has been analyzed. It has been shown that the significant north–south asymmetry of magnetic activity was accompanied by the asynchronous reorganization of solar magnetic fields in the northern and southern hemispheres. The formation of unipolar magnetic regions after the decay of activity centers has been studied. The meridional transport of unipolar magnetic regions leading to changes in the zonal structure of the solar magnetic field has been shown. Long-lived centers of flare activity have been found to exist during the periods of magnetic field restructuring. The spatiotemporal analysis of the flare ensemble making it possible to diagnose non-stationary processes in the solar atmosphere has been shown.
Databáze:	OpenAIRE
Externí odkaz:	https://explore.openaire.eu/search/publication?articleId=doi_________::8730f562da8047fa9ce0b72898e511e5 https://doi.org/10.1134/s106377292007001x Zobrazit plný text záznamu Plný text ve formátu PDF Plný text ve formátu HTML
Nepřihlášeným uživatelům se plný text nezobrazuje	K zobrazení výsledku je třeba se přihlásit.