The Zeeman pattern of magnetic lines and their statistical properties in the Fe I solar spectrum

Details The Zeeman pattern of magnetic lines and their statistical properties in the Fe I solar spectrum The Zeeman pattern of magnetic lines and their statistical properties in the Fe I solar spectrum

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985soph...99....1l&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 99, Sept. 1985, p. 1-15.

Physics

15

Iron, Solar Magnetic Field, Solar Spectra, Zeeman Effect, Histograms, Spectrum Analysis, Statistical Analysis

Scientific paper

The Zeeman patterns of magnetic lines are characterized by their first, second, and third order moments and a 'minimal equivalent' representation is suggested for each line. The statistical properties of the Zeeman patterns of the Fe I lines in the solar optical spectrum are analyzed in detail, and the various patterns are classified in three different types according to the relative position of the delta-components having larger strength.

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