Elaboration of the new magnetohydrostatic sunspot theory Double return flux model

Details Elaboration of the new magnetohydrostatic sunspot theory Double return flux model Elaboration of the new magnetohydrostatic sunspot theory Double return flux model

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983soph...88..117o&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 88, Oct. 1983, p. 117-135.

Physics

20

Astronomical Models, Magnetic Field Configurations, Magnetohydrostatics, Solar Magnetic Field, Sunspots, Data Acquisition, Magnetic Flux, Magnetometers, Photointerpretation, Pressure Distribution

Scientific paper

An extension of the recently formulated Return Flux Sunspot Model is presented. The basic equation for a Double Return Flux Sunspot Model is derived, and a pressure distribution and magnetic field are calculated. The possible topology of the magnetic structure and its thermodynamic consequences are discussed. The paper includes a magnetogram of a single round sunspot (9 August, 1981). The authors attempt to interpret the observational data for the vertical component of magnetic field of this sunspot on the basis of the Double Return Flux Model.

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