Results 61 to 70 of about 20,660,199 (171)
The Astrophysical Journal LettersGiant planet atmospheres are thought to reflect the gas phase composition of the disk when and where they formed. However, these atmospheres may also be polluted via solid accretion or ice sublimation in the disk.
Eric R. Van Clepper +3 more
doaj +1 more source
Origin and early evolution of terrestrial planet atmospheres and oceans
Terrestrial, Atmospheric and Oceanic Sciences, 2019 Planet atmospheric compositions are determined by the availability of a gas species, its molecular weight and the mass (or gravity force) of a planet. Both Mercury and the Moon are not massive enough to hold any gas species to form an atmosphere.
Lin-gun Liu
doaj +1 more source
Inside the Fire Plume Chemical Interactions: A Review on Key Processes and Future Directions
Reviews of Geophysics, Volume 64, Issue 3, September 2026.Abstract Fire plumes are rising columns of heated air masses, consisting of gaseous and particulate matter generated by combustion, affecting air quality, climate and public health. The chemical species released undergo secondary reactions and participate in chemical and physical interactions, altering the properties of the fire plume.
E. Dovrou, A. Voulgarakis
wiley +1 more source
Life on Mars? The physiological perspective
Experimental Physiology, EarlyView.
Ronan M. G. Berg, Damian M. Bailey
wiley +1 more source
Significance of Size‐Dependent Hygroscopicity Parameterization for Aerosol‐Cloud Interactions
Journal of Geophysical Research: Atmospheres, Volume 131, Issue 16, 28 August 2026.Abstract Aerosol‐cloud interactions (aerosol indirect effects) are the most significant source of uncertainties in the effective radiative forcing (ERF) due to aerosols which can act as cloud condensation nuclei (CCN). Uncertainties in the indirect effect can result from systematic uncertainties in aerosol water uptake (hygroscopicity).
Kanishk Gohil +2 more
wiley +1 more source
Giant Planets from the Inside-Out
, 2022 40 pages, 16 figures. Review chapter submitted to Protostars and Planets VII, Editors: Shu-ichiro Inutsuka, Yuri Aikawa, Takayuki Muto, Kengo Tomida, and Motohide TamuraInternational audienceGiant planets acquire gas, ices and rocks during the early ...
Guillot, Tristan +5 more
core +1 more source
Geophysical Research Letters, Volume 53, Issue 15, 16 August 2026.Abstract Saturn's ring current, which modulates the global magnetic field configuration, varies dynamically with hot plasma injections. However, quantifying transient magnetic field disturbances remains challenging in the absence of in situ measurements on Saturn's surface.
Yimeng Li +7 more
wiley +1 more source
Temperatures of Jupiter’s Upper Atmosphere: The Role of the Planetary Magnetic Field
The Astrophysical Journal LettersThe primary source of heating in the upper atmospheres (thermospheres) of giant planets has been the subject of long debate. The conundrum (or “energy crisis”) consists in observed thermosphere temperatures at low and midlatitudes exceeding values ...
Ingo C. F. Müller-Wodarg +4 more
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Jupiter’s Interior with an Inverted Helium Gradient
The Planetary Science JournalJupiter’s gravity field observed by NASA’s Juno spacecraft indicates that the density in the 10–100 GPa region is lower than one would expect from a H/He adiabat with 0.5–5× solar water abundance, as has been observationally inferred in Jupiter’s ...
N. Nettelmann, J. J. Fortney
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The Astrophysical JournalWe present updated atmosphere models designed for calculating the postformation evolution and cooling of giant planets with masses between 0.3 and 10 M _J .
Yi-Xian Chen +3 more
doaj +1 more source