Mn/I/ transition probabilities and the manganese solar abundance

Details Mn/I/ transition probabilities and the manganese solar abundance Mn/I/ transition probabilities and the manganese solar abundance

Jan 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979jqsrt..21...55g&link_type=abstract

Journal of Quantitative Spectroscopy and Radiative Transfer, vol. 21, Jan. 1979, p. 55-63.

Physics

9

Abundance, Line Spectra, Manganese, Solar Spectra, Transition Probabilities, Photosphere, Spectral Line Width, Time Of Flight Spectrometers

Scientific paper

Absolute transition probabilities have been measured for 80 lines from 14 levels in Mn I by mean-foil time-of-flight lifetime measurements combined with emission branching ratios from a hollow-cathode source. Using the Preliminary Edition of the Kitt Peak Solar Atlas the photospheric equivalent width for six of these lines that lie on the linear segment of the curve-of-growth has been measured. These lines yield a mean solar Mn abundance log (NMn/NH) + 12 = 5.55 (+0.12 -0.19).

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