Solar Interior: Convection Zone Flux Tubes

Details Solar Interior: Convection Zone Flux Tubes Solar Interior: Convection Zone Flux Tubes

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000eaa..booke2244f&link_type=abstract

"Encyclopedia of Astronomy and Astrophysics, Edited by Paul Murdin, article 2244. Bristol: Institute of Physics Publishing, 2001

Astronomy and Astrophysics

Astrophysics

Sun, Solar Interior

Scientific paper

The magnetic field at the solar surface reflects the presence of isolated flux tubes below the photosphere. The magnetic field is not diffusively distributed over the entire surface but is concentrated into regions of rather intense field, ranging from SUNSPOTS—with diameters of approximately 20 000 km and field strengths of 3000 G—down to smaller magnetic elements (100-200 km and 1000 G). The e...

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