Magnetosensitive Fe I and FeH lines in the 525.0-525.9 NM solar spectral region

Details Magnetosensitive Fe I and FeH lines in the 525.0-525.9 NM solar spectral region Magnetosensitive Fe I and FeH lines in the 525.0-525.9 NM solar spectral region

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987kfnt....3...87p&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 3, Sept.-Oct. 1987, p. 87-90. In Russian.

Computer Science

Iron Compounds, Line Spectra, Metallicity, Solar Magnetic Field, Solar Spectra, Spectrum Analysis, Magnetic Properties, Photosphere, Sunspots

Scientific paper

The blending of magnetosensitive Fe I 525.022, 525.065, and 525.347 nm
lines by FeH lines is discussed. In the 525.00-525.95 nm region of the
Liege solar atlas (1973), a number of weak lines not indicated in the
Rowland tables (1966) are revealed. Their wavelengths are approximately
evaluated; 18 'new' lines with FeH are identified.

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