D. Toublanc
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View article: Near-infrared absorption and radiative cooling of naphthalene dimers (C<sub>10</sub>H<sub>8</sub>)<sub>2</sub>
Near-infrared absorption and radiative cooling of naphthalene dimers (C<sub>10</sub>H<sub>8</sub>)<sub>2</sub> Open
Time-dependent blue shift of action spectra in storage rings are used to determine the radiative cooling rate of naphthalene dimer cations, (C 10 H 8 ) 2 + . DFTB-EXCI and Monte-Carlo models are successful in reproducing infrared cooling t…
View article: Inner southern magnetosphere observation of Mercury via SERENA ion sensors in BepiColombo mission
Inner southern magnetosphere observation of Mercury via SERENA ion sensors in BepiColombo mission Open
Mercury’s southern inner magnetosphere is an unexplored region as it was not observed by earlier space missions. In October 2021, BepiColombo mission has passed through this region during its first Mercury flyby. Here, we describe the obse…
View article: Dawn/Dusk Asymmetry of the Martian UltraViolet Terminator Observed Through Suprathermal Electron Depletions
Dawn/Dusk Asymmetry of the Martian UltraViolet Terminator Observed Through Suprathermal Electron Depletions Open
Suprathermal electron depletions are structures of the nightside ionosphere of Mars resulting from an equilibrium between electron loss and creation processes. Photoionization of oxygen and carbon dioxide by UV and EUV photons is the main …
View article: The heterogeneous coma of comet 67P/Churyumov-Gerasimenko as seen by ROSINA: H<sub>2</sub>O, CO<sub>2</sub>, and CO from September 2014 to February 2016
The heterogeneous coma of comet 67P/Churyumov-Gerasimenko as seen by ROSINA: H<sub>2</sub>O, CO<sub>2</sub>, and CO from September 2014 to February 2016 Open
Context. The ESA Rosetta mission has been investigating the environment of comet 67P/Churyumov-Gerasimenko (67P) since August 2014. Among the experiments on board the spacecraft, the ROSINA experiment (Rosetta Orbiter Spectrometer for Ion …
View article: Theory for planetary exospheres: III. Radiation pressure effect on the Circular Restricted Three Body Problem and its implication on planetary atmospheres
Theory for planetary exospheres: III. Radiation pressure effect on the Circular Restricted Three Body Problem and its implication on planetary atmospheres Open
The planetary exospheres are poorly known in their outer parts, since the\nneutral densities are low compared with the instruments detection capabilities.\nThe exospheric models are thus often the main source of information at such\nhigh a…
View article: K2-29 b/WASP-152 b: AN ALIGNED AND INFLATED HOT JUPITER IN A YOUNG VISUAL BINARY
K2-29 b/WASP-152 b: AN ALIGNED AND INFLATED HOT JUPITER IN A YOUNG VISUAL BINARY Open
In the present paper we report the discovery of a new hot Jupiter, K2-29 b, first detected by the Super-WASP observatory and then by the K2 space mission during its campaign 4. The planet has a period of 3.25 days, a mass of 0.73 ± 0.04 M …