Modelling the atmospheric CO2 10-μm non-thermal emission in Mars and Venus at high spectral resolution

[1]  E. Millour,et al.  A ground‐to‐exosphere Martian general circulation model: 1. Seasonal, diurnal, and solar cycle variation of thermospheric temperatures , 2009 .

[2]  F. Hourdin,et al.  Using Terrestrial GCMs to Understand Climate on Venus, Mars and Titan , 2008 .

[3]  R. Schieder,et al.  Venus upper atmosphere winds from ground-based heterodyne spectroscopy of CO2 at 10μm wavelength , 2008 .

[4]  R. Schieder,et al.  Temperatures in Venus upper atmosphere from mid-infrared heterodyne spectroscopy of CO2 around 10μm wavelength , 2008 .

[5]  E. Lellouch,et al.  A coordinated campaign of Venus ground-based observations and Venus Express measurements , 2008 .

[6]  Rudolf T. Schieder,et al.  Ultra high spectral resolution observations of planetary atmospheres using the Cologne tuneable heterodyne infrared spectrometer , 2008 .

[7]  S. Erard,et al.  A dynamic upper atmosphere of Venus as revealed by VIRTIS on Venus Express , 2007, Nature.

[8]  P. Drossart,et al.  Non-LTE infrared observations at Venus: From NIMS/Galileo to VIRTIS/Venus Express , 2007 .

[9]  R. Schieder,et al.  High spatial resolution mapping of Mars mesospheric zonal winds by infrared heterodyne spectroscopy of CO2 , 2006 .

[10]  Gang Li,et al.  The HITRAN 2008 molecular spectroscopic database , 2005 .

[11]  P. Drossart,et al.  Analysis of CO2 non-LTE emissions at 4.3μm in the Martian atmosphere as observed by PFS/Mars Express and SWS/ISO , 2005 .

[12]  Michael D. Smith,et al.  Observations of high‐altitude CO2 hot bands in Mars by the orbiting Thermal Emission Spectrometer , 2002 .

[13]  D. Deming,et al.  Measurements of Non-Thermal Infrared Emission Lines of Carbon Dioxide in the Mars Upper Atmosphere , 2001 .

[14]  D. Edwards,et al.  Non-LTE Infrared Emissions of CO2 in the Atmosphere of Venus , 2000 .

[15]  M. López‐Puertas,et al.  A non‐local thermodynamic equilibrium radiative transfer model for infrared emissions in the atmosphere of Mars: 2. Daytime populations of vibrational levels , 1994 .

[16]  M. López‐Puertas,et al.  A non-local thermodynamic equilibrium radiative transfer model for infrared emissions in the atmosphere of Mars: 1. Theoretical basis and nighttime populations of vibrational levels , 1994 .

[17]  D. Deming,et al.  Absolute wind velocities in the lower thermosphere of Venus using infrared heterodyne spectroscopy , 1991 .

[18]  G. Rybicki,et al.  The solution of radiative transfer problems in molecular bands without the LTE assumption by accelerated lambda iteration methods. , 1991 .

[19]  R. Dickinson,et al.  Venus mesosphere and thermosphere. III - Three-dimensional general circulation with coupled dynamics and composition , 1988 .

[20]  S. Drapatz,et al.  Investigation of the Martian atmosphere by 10 micron heterodyne spectroscopy , 1984 .

[21]  B. Gordiets,et al.  Non-equilibrium infrared radiation and natural laser effect in the atmospheres of Venus and Mars. , 1983 .

[22]  D. Deming,et al.  Observations of the 10-μm natural laser emission from the mesospheres of Mars and Venus , 1983 .

[23]  D. Buhl,et al.  Discovery of natural gain amplification in the 10-micrometer carbon dioxide laser bands on Mars: a natural laser. , 1981, Science.

[24]  E. C. Sutton,et al.  Heterodyne detection of CO2 emission lines and wind velocities in the atmosphere of Venus , 1976 .

[25]  T. Hewagama,et al.  Probing the Temperature of Mars' Mesosphere , 2008 .

[26]  D. Buhl,et al.  A new infrared heterodyne instrument for measurements of planetary wind and composition. , 1999 .

[27]  P. Edwards,et al.  GENLN2: A general line-by-line atmospheric transmittance and radiance model. Version 3.0: Description and users guide , 1992 .