The internal magnetic field distribution and the diameters of solar magnetic elements

Details The internal magnetic field distribution and the diameters of solar magnetic elements The internal magnetic field distribution and the diameters of solar magnetic elements

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...211..463z&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 211, no. 2, March 1989, p. 463-475.

Astronomy and Astrophysics

Astrophysics

62

Field Strength, Solar Atmosphere, Solar Magnetic Field, Atmospheric Models, Infrared Spectra, Line Spectra, Magnetic Flux, Radiative Transfer

Scientific paper

A diagnostic is proposed for the horizontal distribution and vertical gradient of the magnetic field with spatially unresolved solar magnetic elements. Radiative transfer calculations are conducted to model the magnetic field structure, which is fitted to observational data from a Fourier transform spectrometer. It is found that a vertical gradient of the magnetic field strength must be present in solar magnetic fluxtubes and that, in the lower photosphere, the field strength inside the fluxtube must be horizontally nearly constant. The magnetic field strengths and gradients derived at the disk center satisfy observations near 0.6 microns, if the appropriate model fluxtube size is chosen.

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