On the possibility of faint molecular lines of PO, PH, MgH(+), and CN in the solar spectrum

Details On the possibility of faint molecular lines of PO, PH, MgH(+), and CN in the solar spectrum On the possibility of faint molecular lines of PO, PH, MgH(+), and CN in the solar spectrum

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988soph..115..221s&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 115, no. 2, 1988, p. 221-227.

Physics

4

Molecular Spectra, Phosphorus Compounds, Solar Atmosphere, Solar Spectra, Spectral Line Width, Absorption Spectra, Cyanogen, Electron Transitions, Magnesium Compounds, Oscillator Strengths

Scientific paper

Equivalent width calculations for some electronic and vibration-rotation transitions of the molecules PO, PH, MgH+, and CN have been carried out for a few umbral, photospheric, and facular model atmospheres. It appears that a few weak lines of these molecules might appear in the umbral spectrum. Le Blanc bands of CN are too weak for detection in the solar spectrum.

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