A note on the values of the vertical gradient of the magnetic field in the Return Flux sunspot model

Details A note on the values of the vertical gradient of the magnetic field in the Return Flux sunspot model A note on the values of the vertical gradient of the magnetic field in the Return Flux sunspot model

Jan 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984soph...90...31o&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 90, Jan. 1984, p. 31-35.

Physics

9

Solar Magnetic Field, Stellar Models, Sunspots, Gradients, Magnetic Flux, Magnetohydrostatics, Solar Atmosphere, Solar Flux

Scientific paper

The Return Flux (RF) sunspot model (Osherovich, 1982) imposes a restriction on the value of the vertical gradient of the magnetic field, dB/dz, analogous to a restriction implied by the self-similar sunspot model of Schlüter and Temesvary (ST). The maximum value of the gradient, (dB/dz)max, is shown to be 10% smaller in the RF model than in the ST model. The dependence of (dB/dz)max on the sunspot radius is predicted.

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