The spectrum of Saturn from 1990 to 2230 cm−1 ; Abundances of AsH3, CH3D, CO, GeH4, NH3, and PH3

[1]  T. Geballe,et al.  The abundance of AsH3 in Jupiter , 1990 .

[2]  Emmanuel Lellouch,et al.  Detection of arsine in Saturn , 1989 .

[3]  J. Pollack,et al.  The carbon budget in the outer solar nebula. , 1989, Icarus.

[4]  D. Gautier,et al.  THE COMPOSITION OF OUTER PLANET ATMOSPHERES , 1989, Origin and Evolution of Planetary and Satellite Atmospheres.

[5]  M. S. Matthews,et al.  Planetary Science. (Book Reviews: Origin and Evolution of Planetary and Satellite Atmospheres) , 1989 .

[6]  T. Geballe,et al.  Arsine in Saturn and Jupiter , 1989 .

[7]  P. Bodenheimer,et al.  THEORIES OF THE ORIGIN AND EVOLUTION OF THE GIANT PLANETS , 1989, Origin and Evolution of Planetary and Satellite Atmospheres.

[8]  N. Grevesse,et al.  Abundances of the elements: Meteoritic and solar , 1989 .

[9]  B. Fegley,et al.  Chemical Constraints on the Water and Total Oxygen Abundances in the Deep Atmosphere of Saturn , 2004, astro-ph/0501128.

[10]  K. Noll.  Carbon Monoxide and Disequilibrium Dynamics in Saturn and Jupiter , 1988 .

[11]  T. Geballe,et al.  Evidence for Germane in Saturn , 1988 .

[12]  E. Lellouch,et al.  Evidence for Arsine (AsH3) in Saturn's Atmosphere , 1988 .

[13]  R. Prinn,et al.  The Predicted Abundances of Deuterium-bearing Gases in the Atmospheres of Jupiter and Saturn , 1988 .

[14]  T. Geballe,et al.  The Origin and Vertical Distribution of Carbon Monoxide in Jupiter , 1988 .

[15]  P. Varanasi,et al.  Measurements on 4.7 μm CH3D lines broadened by H2 and N2 at temperatures relevant to planetary atmospheres , 1987 .

[16]  P. Varanasi,et al.  Intensities and H2-broadened half-widths of Germane lines around 4.7 μm at temperatures relevant to Jupiter's atmosphere☆ , 1987 .

[17]  T. Encrenaz,et al.  Ammonia: Experimental absolute linestrengths and self-broadening parameters in the 1800- to 2100-cm−1 range , 1987 .

[18]  P. Drossart,et al.  High-Resolution Spectroscopy of Saturn at 5 micrometers II. Cloud Structure and Gaseous Composition , 1987 .

[19]  D. Muhleman,et al.  High Resolution VLA Observations of Saturn at 6 cm , 1987 .

[20]  D. Hunten,et al.  Moist convection and the abundance of water in the troposphere of Jupiter , 1987 .

[21]  Gordon L. Bjoraker,et al.  The abundance and distribution of water vapor in Jupiter's atmosphere , 1986 .

[22]  T. Geballe,et al.  Detection of carbon monoxide in Saturn , 1986 .

[23]  P. Bodenheimer,et al.  Planetesimal dissolution in the envelopes of the forming, giant planets , 1986 .

[24]  G. Bjoraker,et al.  The gas composition of jupiter derived from 5-μm airborne spectroscopic observations , 1986 .

[25]  T. Owen,et al.  Deuterium in the outer Solar System: evidence for two distinct reservoirs , 1986, Nature.

[26]  R. Prinn,et al.  Equilibrium and nonequilibrium chemistry of Saturn's atmosphere - Implications for the observability of PH3, N2, CO, and GeH4 , 1985 .

[27]  Steven T. Massie,et al.  Models of the millimeter-centimeter spectra of the giant planets , 1985 .

[28]  B. Bézard,et al.  The composition of Saturn's atmosphere at northern temperate latitudes from Voyager IRIS spectra - NH3, PH3, C2H2, C2H6, CH3D, CH4, and the Saturnian D/H isotopic ratio , 1984 .

[29]  D. Gautier,et al.  The helium abundance of Saturn from Voyager measurements , 1984 .

[30]  R. West,et al.  Clouds and aerosols in Saturn's atmosphere , 1984 .

[31]  R. Prinn,et al.  Composition and chemistry of Saturn's atmosphere , 1984 .

[32]  U. Fink,et al.  The NH3 spectrum in Saturn's 5 micron window , 1983 .

[33]  G. Guelachvili,et al.  Direct retrieval of lineshape parameters: Absolute line intensities for the ν2 band of CH3D , 1983 .

[34]  A Goldman,et al.  AFGL atmospheric absorption line parameters compilation: 1982 edition. , 1981, Applied optics.

[35]  L. Horn,et al.  Infrared observations of the saturnian system from voyager 1. , 1981, Science.

[36]  U. Fink,et al.  The middle-infrared spectrum of Saturn - Evidence for phosphine and upper limits to other trace atmospheric constituents , 1980 .

[37]  J. S. Lewis,et al.  Kinetic inhibition of CO and N2 reduction in the solar nebula , 1980 .

[38]  D. Lester,et al.  The phosphine abundance on Saturn derived from new 10-micrometer spectra , 1980 .

[39]  D. Gautier,et al.  Ammonia vertical density profiles in Jupiter and Saturn from their radioelectric and infrared emissivities , 1980 .

[40]  J. Logan,et al.  Carbon monoxide in jupiter's upper atmosphere: An extraplanetary source , 1978 .

[41]  U. Fink,et al.  Deuterated Methane Observed on Saturn , 1978, Science.

[42]  U. Fink,et al.  Upper limits to trace constituents in Jupiter's atmosphere from an analysis of its 5-μm spectrum , 1978 .

[43]  U. Fink,et al.  Germane in the atmosphere of Jupiter , 1978 .

[44]  R. Prinn,et al.  Carbon monoxide on jupiter and implications for atmospheric convection. , 1977, Science.

[45]  U. Fink,et al.  Phosphine in Jupiter's atmosphere - The evidence from high-altitude observations at 5 micrometers , 1977 .

[46]  U. Fink,et al.  Infrared Fourier spectrometer for laboratory use and for astronomical studies from aircraft and ground-based telescopes. , 1975, Applied optics.

[47]  Dudley A. Williams,et al.  Collisional broadening of CO absorption lines by foreign gases. , 1968 .