Magnetic helicity evolution during the solar activity cycle: Observations and dynamo theory

Astronomy and Astrophysics

Volumn 409, Issue 3, 2003, Pages 1097-1105

  Kleeorin, N ^a   Kuzanyan, K ^b   Moss, D ^c   Rogachevskii, I ^a   Sokoloff, D ^d   Zhang, H ^e  

^a BEN GURION UNIVERSITY OF THE NEGEV   (Israel)

^b PUSHKOV INSTITUTE OF TERRESTRIAL MAGNETISM   (Russian Federation)

^c UNIVERSITY OF MANCHESTER   (United Kingdom)

^d MOSCOW STATE UNIVERSITY   (Russian Federation)

^e CHINESE ACADEMY OF SCIENCES   (China)

Author keywords

Sun: magnetic fields

Indexed keywords

MAGNETIC FIELDS; MAGNETOHYDRODYNAMICS; MATHEMATICAL MODELS; SUN;

HELICITY EVOLUTION; MAGNETIC HELICITY; SOLAR ACTIVITY CYCLE;

ASTROPHYSICS;

EID: 0142135127     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20031126     Document Type: Article

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