Possible maser emission in certain lines of the H2O rotational spectrum

Details Possible maser emission in certain lines of the H2O rotational spectrum Possible maser emission in certain lines of the H2O rotational spectrum

Oct 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974azh....51.1114s&link_type=abstract

Astronomicheskii Zhurnal, vol. 51, Sept.-Oct. 1974, p. 1114-1116. In Russian.

Other

Interstellar Gas, Line Spectra, Maser Outputs, Optical Pumping, Rotational Spectra, Water Vapor, Electron Transitions, Infrared Spectra, Molecular Spectra, Population Inversion, Transition Probabilities

Scientific paper

Study of the possibility of chemical or collisional cascade maser pumping in certain lines of the H2O rotational spectrum other than the 1.35-cm line. For this purpose, a method proposed by Strel'nitskii (1971) is employed, in which the unsaturated relative population inversion is determined for each investigated transition. Out of 27 rotational transitions investigated the possibility of population inversion in 18 transitions ranging in wavelength from 150 to 1650 microns is demonstrated.

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