The DH ratio in the atmosphere of Uranus: Detection of the R5(1) line of HD
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[1] W. Smith,et al. Determination of the H2 4-0 S/1/ quadrupole line strength and pressure shift , 1980 .
[2] U. Fink,et al. The infrared spectra of Uranus, Neptune, and Titan from 0.8 to 2.5 microns , 1979 .
[3] W. Macy,et al. Detection of HD on Saturn and Uranus, and the D/H ratio , 1978 .
[4] L. Trafton. On the deuterium-to-hydrogen ratio in the atmosphere of Uranus , 1978 .
[5] D. Gautier,et al. On the thermal structure of Uranus from infrared measurements , 1978 .
[6] W. Smith,et al. Photoacoustic Measurements of Line Strengths for HD, CH4, NH3 Red Transitions. , 1977 .
[7] R. E. Danielson,et al. A saturation model of the atmosphere of Uranus , 1977 .
[8] L. Trafton. The aerosol distribution in Uranus' atmosphere - Interpretation of the hydrogen spectrum , 1976 .
[9] A. Mckellar,et al. The rotation-vibration spectrum of HD: wavelength and intensity measurements of the 3-0, 4-0, 5-0, and 6-0 electric dipole bands. , 1976 .
[10] L. Trafton. Titan: Unidentified Strong Absorptions in the Photometric Infrared , 1974 .
[11] O. White,et al. The Analysis and Restoration of Astronomical Data via the Fast Fourier Transform , 1971 .