The solar arsenic abundance

Details The solar arsenic abundance The solar arsenic abundance

Feb 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001kfnt...17...37g&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, vol. 17, no. 1, p. 37-44

Computer Science

1

Scientific paper

Comparison of the solar spectrum with calculations of the synthetic spectrum of the solar atmosphere in a wide spectral region permitted us to identify two absorption arsenic lines: lambdalambda 299.0984 nm and 303.2846 nm. The solar arsenic abundance as determined by the spectrum synthesis method: lgN = 2.33 using the spectral atlas of the solar disk center and the solar atmosphere model by Holweger and Muller. Wavelengths and oscillator strengths of molecular lines in the wavelength regions lambdalambda 299.0871-299.1041 and 303.2762-303.2952 nm were checked. The solar arsenic abundance is in good agreement with meteoritic arsenic abundance (2.37).

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