Solar oscillations and the problem of magnetograph signal formation in the case of different intensities of the splitting components

Details Solar oscillations and the problem of magnetograph signal formation in the case of different intensities of the splitting components Solar oscillations and the problem of magnetograph signal formation in the case of different intensities of the splitting components

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987kfnt....3...19d&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 3, Nov.-Dec. 1987, p. 19-27. In Russian.

Computer Science

Magnetic Signatures, Signal Reception, Solar Activity, Solar Oscillations, Abundance, Algorithms, Brightness Temperature, Line Spectra

Scientific paper

The problem of magnetograph signal formation is considered with allowance for possible differences in the splitting-component intensities. This problem is of particular importance in studies of small-amplitude phenomena such as the global oscillations of the sun. An algorithm for signal formation is described which makes it possible (together with differential velocity measurements) to record relative brightness variations in the same line; this is of importance in the study of oscillatory processes.

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