Helicity of Solar Active Regions from a Dynamo Model

Details Helicity of Solar Active Regions from a Dynamo Model Helicity of Solar Active Regions from a Dynamo Model

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006japa...27...87c&link_type=abstract

Journal of Astrophysics and Astronomy, vol. 27, no.2 & 3, P. 87-91.

Astronomy and Astrophysics

Astrophysics

1

Mhd, Sun: Activity, Sun: Magnetic Fields, Sunspots

Scientific paper

We calculate helicities of solar active regions based on the idea that
poloidal flux lines get wrapped around a toroidal flux tube rising
through the convection zone, thereby giving rise to the helicity. We use
our solar dynamo model based on the Babcock-Leighton α-effect to
study how helicity varies with latitude and time.

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