Small-scale magnetic fields and convection in the solar photosphere

Details Small-scale magnetic fields and convection in the solar photosphere Small-scale magnetic fields and convection in the solar photosphere

May 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978mnras.183p..63w&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 183, May 1978, p. 63P-65P.

Physics

6

Convective Flow, Photosphere, Solar Atmosphere, Solar Granulation, Solar Magnetic Field, Boussinesq Approximation, Magnetic Effects, Solar Physics

Scientific paper

The detection of solar magnetic structures with diameters less than 300 km, as reported by Ramsey et al. (1977), is related to theoretical studies of the nonlinear interaction between magnetic fields and convection. In particular, it is shown that the location of the small-scale magnetic fields at the centers of granules cannot be readily explained on the basis of theoretical investigations of vigorous Boussinesq convection in a magnetic field.

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