Configuration of the chromospheric magnetic field in a unipolar sunspot region

Details Configuration of the chromospheric magnetic field in a unipolar sunspot region Configuration of the chromospheric magnetic field in a unipolar sunspot region

Oct 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994soph..154..207z&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 154, no. 2, p. 207-214

Physics

11

Chromosphere, Magnetic Field Configurations, Solar Magnetic Field, Solar Prominences, Stellar Atmospheres, Sunspots, Magnetic Signatures, Penumbras, Solar Limb

Scientific paper

A set of H-Beta chromospheric magnetograms at various wavelengths near the line center, chromospheric Dopplergrams, and photospheric vector magnetograms of a unipolar sunspot region near the solar limb were obtained with the vector video magnetograph at the Huairou Solar Observing Station. The supernumbral chromospheric magnetic field is almost parallel to the surface at the outside of the sunspot penumbra, where the magnetic lines of force are mainly concentrated in the superpenumbral filaments. In the gaps between the filaments the chromospheric horizontal field is weak.

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