Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984sva....28...70s&link_type=abstract
(Astronomicheskii Zhurnal, vol. 61, Jan.-Feb. 1984, p. 118-120) Soviet Astronomy (ISSN 0038-5301), vol. 28, Jan.-Feb. 1984, p. 7
Astronomy and Astrophysics
Astronomy
Molecular Ions, Photons, Scattering Coefficients, Solar Radiation, Water Vapor, Molecular Spectra, Transition Probabilities
Scientific paper
The results of theoretical calculations of the transition probabilities and photon scattering coefficients for H2O(+) molecules in solar radiation are presented. The calculations were made for the various electronic and vibrational bands of the deformational transition. A table is presented which lists the wavelengths of the H2O(+) transitions for conditions on the earth. The H2O(+) bands observed in comets are found to be the most intense, and therefore most suitable for measurement. For the conditions of comet Kohoutek, the photon scattering coefficient was 0.22 photons/sec per molecule at AU 0.51 and 0.032 photons/sec per molecule at 1.5 and 1.37 AU from the sun on January 10, 1974.
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