A new dynamo mechanism in solar convection zone

Details A new dynamo mechanism in solar convection zone A new dynamo mechanism in solar convection zone

Jun 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001pbeio..37...55j&link_type=abstract

Astrophysics Reports. Publications of the Beijing Astronomical Observatory, No. 37, p. 55 - 61 (2001). In: Proceedings of the Ei

Astronomy and Astrophysics

Astrophysics

Sun: Dynamo, Sun: Magnetic Fields, Turbulent Plasma

Scientific paper

In this paper, based on a p-ω dynamo mechanism, we tried to explain the small-scale solar magnetic field in a quiet region. We derived that under certain condition, a new instability may occur, then the plasma turbulence becomes strong turbulence, and the strong thin flux tubes may be generated. These flux tubes emerge on the photosphere surface and form small-scale magnetic fields. We showed it using plane wave solution and obtained some interesting results.

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