Elemental abundances and minimum mass of heavy elements in the envelope of HD 189733b (2009)
Mousis, Olivier, Lunine, Jonathan I., Tinetti, Giovanna, Griffith, Caitlin A., Showman, Adam P., Alibert, Yann, ...
Oxygen (O) and carbon (C) have been inferred recently to be subsolar in abundance from spectra of the atmosphere of the transiting hot Jupiter HD 189733b. Yet, the mass and radius of the planet...
Global circulation as the main source of cloud activity on Titan (2009)
Rodriguez, Sébastien, Mouélic, Stéphane Le, Rannou, Pascal, Tobie, Gabriel, Baines, Kevin H., Barnes, Jason W., ...
Clouds on Titan result from the condensation of methane and ethane and, as on other planets, are primarily structured by circulation of the atmosphere. At present, cloud activity mainly occurs in the...
Global circulation as the main source of cloud activity on Titan (2009)
Rodriguez, Sébastien, Le Mouélic, Stéphane, Rannou, Pascal, Tobie, Gabriel, Baines, Kevin H., Barnes, Jason W., ...
Clouds on Titan result from the condensation of methane and ethane and, as on other planets, are primarily structured by circulation of the atmosphere. At present, cloud activity mainly occurs in the...
Global circulation as the main source of cloud activity on Titan (2009)
Rodriguez, Sébastien, Le Mouélic, Stéphane, Rannou, Pascal, Tobie, Gabriel, Baines, Kevin H., Barnes, Jason W., ...
Clouds on Titan result from the condensation of methane and ethane and, as on other planets, are primarily structured by circulation of the atmosphere. At present, cloud activity mainly occurs in the...
Convective plumes and the scarcity of Titan’s clouds (2008)
Ralph D. Lorenz, Caitlin A. Griffith, Jonathan I. Lunine, Christopher P. Mckay, Nilton O. Rennò, Citation Lorenz, ...
[1] We show that simple thermodynamic models of convective plumes predict the area fraction of convective plumes (i.e., updrafts) in Titan’s atmosphere to be 12 smaller than on Earth. This result...
Fluvial erosion and post erosional processes on Titan (2008)
Jaumann, Ralf, Brown, Robert H., Stephan, Katrin, Barnes, Jason W., Soderblom, Larry A., Sotin, Christophe, ...
The surface of Titan has been revealed by Cassini observations in the infrared and radar wavelength ranges as well as locally by the Huygens lander instruments. Sand seas, recently discovered lakes,...
Le méthane dans l'atmosphère de Titan : de la spectroscopie fondamentale à la planétologie (2008)
Boudon, Vincent, Champion, Jean Paul, Gabard, Tony, Loete, Michel, Coustenis, Athena, De Bergh, Catherine, ...
Le méthane (CH4) joue sur Tian, le plus gros satellite de Saturne, un rôle similaire à celui de l'eau sur Terre. Il y est de plus à l'origine d'une chimie organique complexe. La spectroscopie...
Le méthane dans l'atmosphère de Titan : de la spectroscopie fondamentale à la planétologie (2008)
Boudon, Vincent, Champion, Jean Paul, Gabard, Tony, Loete, Michel, Coustenis, Athena, De Bergh, Catherine, ...
Le méthane (CH4) joue sur Tian, le plus gros satellite de Saturne, un rôle similaire à celui de l'eau sur Terre. Il y est de plus à l'origine d'une chimie organique complexe. La spectroscopie...
Structure Of The Jovian Stratosphere At The Galileo Probe Entry Site (2007)
Roger Yelle Caitlin, Roger V. Yelle, Caitlin A. Griffith, Leslie A. Young
The structure of the Jovian stratosphere at the Galileo probe entry site is investigated through calculations of radiative heating rates based on measurements of the temperature profile, composition,...
Structure of the jovian stratosphere at the Galileo probe entry site (2001)
Roger V. Yelle, Caitlin A. Griffith
The structure of the Jovian stratosphere at the Galileo probe entry site is investigated through calculations of radiative heating rates based on measurements of the temperature profile, composition,...