Results 251 to 260 of about 1,115,032 (293)

The erosion of large primary atmospheres typically leaves behind substantial secondary atmospheres on temperate rocky planets. [PDF]

Nat Commun
Krissansen-Totton J, Wogan N, Thompson M, Fortney JJ.   +3 more
europepmc   +1 more source

Challenges in the standardization of in vitro cytotoxicity assays for comparative risk assessment of cold atmospheric pressure plasma devices. [PDF]

Sci Rep
Boeckmann L, Ficht PK, Bernhardt T, Borchardt T, Ossowska A, Milz W, Helmke A, Bekeschus S, Emmert S.   +8 more
europepmc   +1 more source

The rainout of formaldehyde favors a formose-based origin of life in shallow ponds

Scherf M, Constatinou T, Rimmer P, Woitke P, Ferus M, Lammer H, Cassone G, Weichbold F, Eminger P, Nemeckova K, Kacina J.   +10 more
europepmc   +1 more source

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Atmospheric escape from exoplanets: recent observations and theoretical models

Reviews of Modern Plasma Physics
The review aims to give an overview of atmospheric escape processes from exoplanets. I briefly discuss the physics of various escape processes responsible for atmospheric escape across different types of exoplanets.
Gopal Hazra
exaly   +2 more sources

Exospheres and Atmospheric Escape

Space Science Reviews, 2008
Aeronomy is a description of the physics and chemistry of the upper atmospheres and ionospheres of planetary bodies. In this chapter we consider those processes occurring in the upper atmosphere that determine the structure of the corona and lead to molecular escape.
, Valery Shematovich, Michael Combi
exaly   +4 more sources

Elevated atmospheric escape of atomic hydrogen from Mars induced by high-altitude water

Nature Geoscience, 2017
Nicholas Schneider, Michael Chaffin, Justin Deighan   +2 more
exaly   +2 more sources

Escaping atmospheres of extrasolar planets

Science, 2018
The study of helium absorption opens a new window on escaping exo ...
openaire   +2 more sources

Escape of Planetary Atmospheres. I. Escape Layer

The Physics of Fluids, 1961
The critical layer for thermal escape of a planetary atmosphere is treated on a model in which an isothermal exosphere at high temperature merges within a narrow zone (the endopause) of varying temperature into the remainder (the endosphere) of the atmosphere, isothermal above the level at which mixing stops.
openaire   +1 more source

Solar Wind Interaction and Atmospheric Escape

2017
International ...
Brain, David A., Barabash, Sergey, Bougher, Stephen W., Durut, Firat, Jakosky, Bruce M., Modolo, Ronan   +5 more
openaire   +2 more sources