An analysis of measurements of the longitudinal and transverse magnetic field components in solar polar regions

Details An analysis of measurements of the longitudinal and transverse magnetic field components in solar polar regions An analysis of measurements of the longitudinal and transverse magnetic field components in solar polar regions

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988kfnt....4...80g&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 4, Sept.-Oct. 1988, p. 80-83. In Russian.

Computer Science

2

Magnetic Signatures, Solar Magnetic Field, Cross Sections, Line Spectra, Magnetic Flux, Poles, Visible Spectrum

Scientific paper

It is shown that the mean intensity of the longitudinal magnetic-field component is equal to 0.00042 T while that of the transverse component is 0.0075 T in the solar polar regions. The measurements were carried out with a spatial resolution of 4 x 2 arcsec. The difference is explained by the fact that the longitudinal component signal is formed by averaging the intensity while the tranverse component is formed by averaging the square of the intensity of the magnetic field of the fine structure elements over the magnetograph aperture.

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