Direct corroboration of the role of H(-) in solar absorption

Details Direct corroboration of the role of H(-) in solar absorption Direct corroboration of the role of H(-) in solar absorption

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.240....1j&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 240, Sept. 1, 1989, p. 1-5.

Astronomy and Astrophysics

Astronomy

6

Absorption Spectra, Hydrogen Ions, Limb Darkening, Negative Ions, Solar Spectra, Continuous Spectra, Infrared Spectra, Interstellar Extinction, Late Stars, Quantum Mechanics

Scientific paper

It is shown that absorption coefficients of the negative hydrogen ion and coefficients determined from analysis of solar limb darkening observations fit to better than 5 percent for most of the spectral range (0.4-2.4 microns) with a standard deviation of 3.8 percent. These results show considerable improvement over earlier analyses, which produce errors of nearly 40 percent at long wavelengths and a standard deviation of 19 percent when more accurate H(-) absorption coefficients are used in comparisons.

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