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The transmission of light through a planetary atmosphere can be studied as a function of altitude and wavelength using stellar or solar occultations, giving often unique constraints on the atmospheric composition. For exoplanets, a transit yields a limb-integrated, wavelength-dependent transmission spectrum of an atmosphere. When scattering haze and/or cloud particles are present in the planetary...
The daytime convective boundary layer (CBL) of Mars and the transition to it after the cold night is studied on a warm dusty sol at the rover Spirit using temperature profiles from the miniature thermal emission spectrometer (mini-TES) and a 1-D model. The model’s net solar fluxes are linear in z in the CBL while the thermal fluxes decay logarithmically from about 8m upward, due mainly to the emissivity...
We analyze far-infrared (10–650cm −1 ) emissivity spectra of Saturn’s main rings obtained by the Cassini Composite Infrared Spectrometer (CIRS). In modeling of the spectra, the single scattering albedos of regolith grains are calculated using the Mie theory, diffraction is removed with the delta-Eddington approximation, and the hemispherical emissivities of macroscopic free-floating ring particles...
This paper describes a methodology for performing temperature retrievals in the martian atmosphere in the 60–90km altitude range using spectrally integrated 15μm CO 2 limb emissions measured by the Thermal Emission Spectrometer (TES), the infrared spectrometer on-board the Mars Global Surveyor (MGS). We show that a limited number of limb-geometry sequences observed by this instrument are characterized...
This work deals with the optical constant characterization of Titan aerosol analogues or “tholins” produced with the PAMPRE experimental setup and deposited as thin films onto a silicon substrate. Tholins were produced in different N 2 –CH 4 gaseous mixtures to study the effect of the initial methane concentration on their optical constants. The real (n) and imaginary (k) parts of...
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