Large-scale flow and transport of magnetic flux in the solar convection zone

0124778 - ASU-R 20010031 RIV IN eng J - Článek v odborném periodiku
Ambrož, Pavel
Large-scale flow and transport of magnetic flux in the solar convection zone.
Journal of Astrophysics and Astronomy. Roč. 21, 3/4 (2000), s. 315-318. ISSN 0250-6335. E-ISSN 0973-7758.
[Colloquium of the International Astronomical Union /179./: Cyclical evolution of solar magnetic fields: Advances in theory and observations. Kodaikanal, 13.12.1999-16.12.1999]
Grant CEP: GA AV ČR IAA3003806; GA AV ČR KSK1003601
Výzkumný záměr: CEZ:AV0Z1003909
Klíčová slova: sun * large-scale flow * cyclic variations
Kód oboru RIV: BN - Astronomie a nebeská mechanika, astrofyzika
Impakt faktor: 0.625, rok: 2000

Flow systems of solar plasma create the large-scale cellular-like patterns with up-flow in the center and the down-flow on the boundaries. Distribution of the large-scale horizontal eddies was found in broad equatorial zone. Plot of RMS values of total horizontal velocity is shifted about 1.6 years before the similarly shaped variation of the magnetic flux.
Trvalý link: http://hdl.handle.net/11104/0023037