Results 21 to 30 of about 141,901 (265)
Wind‐induced atmospheric escape: Titan [PDF]
Rapid thermospheric flows can significantly enhance the atmospheric loss rates and structures of atmospheric coronae of planetary bodies. Using descriptions of atmospheric escape based on molecular kinetic models, we show that such flows at the exobase of Titan could significantly increase the calculated constituent thermal and nonthermal escape rates.
R. E. Hartle +4 more
openaire +1 more source
Observing Atmospheric Escape in Sub-Jovian Worlds with JWST
Hydrodynamic atmospheric escape is considered an important process that shapes the evolution of sub-Jovian exoplanets, particularly those with short orbital periods.
Leonardo A. Dos Santos +3 more
doaj +1 more source
Developing a self‐consistent description of Titan's upper atmosphere without hydrodynamic escape [PDF]
In this study, we develop a best fit description of Titan's upper atmosphere between 500 km and 1500 km, using a one‐dimensional (1‐D) version of the three‐dimensional (3‐D) Titan Global Ionosphere‐Thermosphere Model.
Bell, Jared M. +6 more
core +1 more source
Photochemical enrichment of deuterium in Titan's atmosphere: new insights from Cassini-Huygens [PDF]
Cassini-Huygens data are used to re-examine the potential sources of the D/H enhancement over solar, measured in methane, in Titan's atmosphere. Assuming that the system is closed with respect to carbon, the use of constraints from the Huygens probe for ...
Audrey Moudens +7 more
core +4 more sources
Methane escape from Titan's atmosphere [PDF]
Measurements of the mole fractions of CH4 and 40Ar by the Ion Neutral Mass Spectrometer on the Cassini orbiter are analyzed to determine the rate of vertical mixing in Titan's atmosphere and the escape flux of CH4. Analysis of the 40Ar data indicates an eddy mixing rate of 2–5 × 107 cm2 s−1, an order of magnitude smaller than previously determined from
R. V. Yelle +2 more
openaire +1 more source
Remote sensing observations of far-ultraviolet (FUV) emissions have been used to estimate 3D neutral hydrogen (H) density models of the terrestrial exosphere under solar minimum (2008) and solar maximum (2013 and 2015) conditions.
Jochen H. Zoennchen +4 more
doaj +1 more source
The precipitation of energetic neutral atoms, produced through charge exchange collisions between solar wind ions and thermal atmospheric gases, is investigated for the Martian atmosphere.
Kharchenko, Vasili, Lewkow, Nicholas
core +1 more source
Ambipolar Electric Field, Photoelectrons, and their Role in Atmospheric Escape From Hot-jupiters [PDF]
Atmospheric mass-loss from Hot-jupiters can be large due to the close proximity of these planets to their host star and the strong radiation the planetary atmosphere receives.
Cohen, O., Glocer, A.
core +3 more sources
Narrow Loophole for H2-Dominated Atmospheres on Habitable Rocky Planets around M Dwarfs
Habitable rocky planets around M dwarfs that have H _2 -dominated atmospheres, if they exist, would permit characterizing habitable exoplanets with detailed spectroscopy using JWST, owing to their extended atmospheres and small stars.
Renyu Hu +2 more
doaj +1 more source
We present an atmospheric analysis of LTT 9779 b, a rare planet situated in the hot-Neptune desert, that has been observed with Hubble Space Telescope (HST)/WFC3 with G102 and G141.
Billy Edwards +29 more
doaj +1 more source

