Magnetic field in solar prominences measured with a new spectrally scanning magnetograph

Details Magnetic field in solar prominences measured with a new spectrally scanning magnetograph Magnetic field in solar prominences measured with a new spectrally scanning magnetograph

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...114..347k&link_type=abstract

Astronomy and Astrophysics, vol. 114, no. 2, Oct. 1982, p. 347-350.

Astronomy and Astrophysics

Astrophysics

7

Magnetic Signatures, Polarization (Charge Separation), Solar Magnetic Field, Solar Prominences, Doppler Effect, Fine Structure, Zeeman Effect

Scientific paper

Observations of the longitudinal field strength in quiescent prominences obtained with the new redesigned spectrally scanning magnetograph installed in the Coude focus of the 53 cm coronograph of the Kislovodsk station are presented. With the instrument one can obtain magnetographic data as well as central intensities, equivalent widths, line widths, and shifts of the analyzed prominence lines. A first discussion, correlating magnetographic and spectroscopic data, is given

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