SWAS observations of water vapor in the Venus mesosphere

[1]  M. Gurwell,et al.  Mars surface and atmospheric temperature during the 2001 global dust storm , 2005 .

[2]  R. Clancy,et al.  Water vapor variations in the Venus mesosphere from microwave spectra , 2004 .

[3]  E. Bergin,et al.  Submillimeter Wave Astronomy Satellite Monitoring of the Postperihelion Water Production Rate of Comet C/1999 T1 (MCNaught-Hartley) , 2004 .

[4]  M. Gurwell.  Submillimeter Observations of Titan: Global Measures of Stratospheric Temperature, CO, HCN, HC3N, and the Isotopic Ratios 12C/13C and 14N/15N , 2004, astro-ph/0407169.

[5]  M. Gurwell,et al.  Submillimeter Wave Astronomy Satellite Performance on the ground and in orbit , 2004 .

[6]  R. Clancy,et al.  Observational definition of the Venus mesopause: vertical structure, diurnal variation, and temporal instability , 2003 .

[7]  M. Harwit,et al.  Submillimeter Wave Astronomy Satellite Observations of Water Vapor toward Comet C/1999 H1 (Lee) , 2000 .

[8]  M. Gurwell,et al.  Submillimeter Wave Astronomy Satellite Observations of Jupiter and Saturn:Detection of 557 GHz Water Emission from the Upper Atmosphere , 2000 .

[9]  M. Gurwell,et al.  Submillimeter Wave Astronomy Satellite Observations of the Martian Atmosphere: Temperature and Vertical Distribution of Water Vapor , 2000 .

[10]  Thermal infrared spectroscopy of Europa and Callisto , 2000 .

[11]  F. Mills.  Water vapor in the venus middle atmosphere , 1999 .

[12]  James M. Moran,et al.  The Submillimeter Array , 2004, Astronomical Telescopes and Instrumentation.

[13]  Gary J. Melnick,et al.  The Submillimeter Wave Astronomy Satellite: Science Objectives and Instrument Description , 1998, Astronomical Telescopes and Instrumentation.

[14]  F. Mills.  I. Observations and Photochemical Modeling of the Venus Middle Atmosphere. II. Thermal Infrared Spectroscopy of Europa and Callisto , 1998 .

[15]  P. Hamill,et al.  A new parameterization of H2SO4/H2O aerosol composition: Atmospheric implications , 1997 .

[16]  Donald M. Hunten,et al.  Venus II--geology, geophysics, atmosphere, and solar wind environment , 1997 .

[17]  P. Irwin.  Temporal and spatial variations in the Venus mesosphere retrieved from Pioneer Venus OIR , 1997 .

[18]  David Crisp,et al.  Ground‐based near‐infrared observations of the Venus nightside: 1.27‐μm O2(a 1Δ g ) airglow from the upper atmosphere , 1996 .

[19]  Athena Coustenis,et al.  Detectability of molecular species in planetary and satellite atmospheres from their rotational transitions , 1995 .

[20]  T. Encrenaz,et al.  The Thermal Profile and Water Abundance in the Venus Mesosphere from H2O and HDO Millimeter Observations , 1995 .

[21]  D. Muhleman,et al.  Observations of the CO bulge on Venus and implications for mesospheric winds , 1995 .

[22]  W. Borucki,et al.  Venus O2 visible and IR nightglow : implications for lower thermosphere dynamics and chemistry , 1994 .

[23]  M. Janssen.  Atmospheric Remote Sensing by Microwave Radiometry , 1993 .

[24]  P. Rosenkranz,et al.  Absorption of Microwaves by Atmospheric Gases , 1993 .

[25]  T. Encrenaz,et al.  First detection of HDO in the atmosphere of Venus at radio wavelengths : an estimate of the H2O vertical distribution , 1991 .

[26]  T. Owen,et al.  Deuterium on Venus: Observations From Earth , 1991, Science.

[27]  Duane O. Muhleman,et al.  Long-term (1979–1990) changes in the thermal, dynamical, and compositional structure of the Venus Mesosphere as inferred from microwave spectral line observations of 12CO, 13CO, and C18O , 1991 .

[28]  J. Gérard,et al.  The Venus nitric oxide night airglow: Model calculations based on the Venus thermospheric general circulation model , 1990 .

[29]  V. M. Linkin,et al.  Water vapor and sulfur dioxide abundances at the Venus cloud tops from the Venera-15 infrared spectrometry data , 1990 .

[30]  Jean-Michel Hartmann,et al.  Temperature and perturber dependences of water vapor line-broadening. Experiments at 183 GHz; calculations below 1000 GHz , 1989 .

[31]  B. Bézard,et al.  The 12C/13C and 16O/18O ratios in the atmosphere of Venus from high-resolution 10-μm spectroscopy , 1987 .

[32]  D. Muhleman,et al.  Diurnal CO variations in the Venus mesophere from CO microwave spectra , 1985 .

[33]  D. Muhleman,et al.  Chemical-dynamical models of the Venus mesosphere based upon diurnal microwave CO variations☆ , 1985 .

[34]  H. Müller,et al.  Submillimeter, millimeter, and microwave spectral line catalog. , 1985, Applied optics.

[35]  Henry E. Revercomb,et al.  Models of the structure of the atmosphere of Venus from the surface to 100 kilometers altitude , 1985 .

[36]  Fredric W. Taylor,et al.  The global distribution of water vapor in the middle atmosphere of Venus , 1982 .

[37]  Y. Yung,et al.  Photochemistry of the stratosphere of Venus: Implications for atmospheric evolution☆☆☆ , 1982 .

[38]  David W. Rusch,et al.  Morphology of the Venus ultraviolet night airglow , 1980 .

[39]  A. Stewart,et al.  Ultraviolet Night Airglow of Venus , 1979, Science.

[40]  A. K. Hui,et al.  Rapid computation of the Voigt and complex error functions , 1978 .

[41]  G. Reesor,et al.  Collision Induced Absorption in N2, CO2, and H2 at 2.3 cm−1 , 1975 .

[42]  E. Barker.  Observations of Venus water vapor over the disk of Venus: The 1972–1974 data using the H2O lines at 8197 Å and 8176 Å , 1975 .

[43]  Prasad Varanasi,et al.  Measurement of line widths of CO of planetary interest at low temperatures , 1975 .

[44]  W. Ho.  Microwave Absorption in Models of the Atmosphere of Venus. , 1966 .