Results 111 to 120 of about 872,424 (257)

Planetary atmospheres Through Time: Effects of Mass Loss and Thermal Evolution [PDF]

arXiv
Atmospheric mass loss is a fundamental phenomenon shaping the structure and evolution of planetary atmospheres. It can engage processes ranging from global interactions with the host star and large-scale hydrodynamic outflows to essentially microphysical kinetic effects.
arxiv  

Planetary Atmospheres [PDF]

, 1950
D. L. Huestis, N. G. Adams, S. K. Atreya, K. H. Baines, R. F. Beebe, S. J. Bolton, S. W. Bougher, A. Coustenis, S. G. Edgington, A. J. Friedson, M. Galand, C. A. Griffith, S. L. Guberman, Heidi B. Hammel, Mark Hofstadter, A. P. Ingersoll, J. I. Lunine, M. Mendillo, J. Moses, Ingo Mueller‐Wodarg, Glenn S. Orton, K. A. Rages, T. G. Slanger, D. V. Titov, A. R. Vasavada, A.-S. Wong, R. V. Yelle   +26 more
openalex   +1 more source

ExoCubed: A Riemann-solver-based Cubed-sphere Dynamic Core for Planetary Atmospheres

The Astrophysical Journal
The computational fluid dynamics on a sphere is relevant to global simulations of geophysical fluid dynamics. Using the conventional spherical–polar (or lat–lon) grid results in a singularity at the poles, with orders-of-magnitude-smaller cell sizes at ...
Sihe Chen, Cheng Li
doaj   +1 more source

Spectroscopy of planetary atmospheres in our Galaxy

, 2013
About 20 years after the discovery of the first extrasolar planet, the number of planets known has grown by three orders of magnitude, and continues to increase at neck breaking pace.
G. Tinetti, T. Encrenaz, A. Coustenis
semanticscholar   +1 more source

Effects of planetary mass uncertainties on the interpretation of the reflectance spectra of Earth-like exoplanets [PDF]

arXiv
Atmospheric characterization of Earth-like exoplanets through reflected light spectroscopy is a key goal for upcoming direct imaging missions. A critical challenge in this endeavor is the accurate determination of planetary mass, which may influence the measurement of atmospheric compositions and the identification of potential biosignatures.
arxiv  

Kinetic and Photochemical Disequilibrium in the Potentially Carbon-rich Atmosphere of the Warm Jupiter WASP-69 b

The Astrophysical Journal
High-resolution transmission spectroscopy of the warm gas giant WASP-69 b has revealed the presence of H _2 O, CO, CH _4 , NH _3 , and C _2 H _2 in its atmosphere.
Nidhi Bangera, Christiane Helling, Gloria Guilluy, Patricio Cubillos, Luca Fossati, Paolo Giacobbe, Paul Rimmer, Daniel Kitzmann   +7 more
doaj   +1 more source

Exact and Approximate Solutions for Multiple Scattering by Cloudy and Hazy Planetary Atmospheres [PDF]

, 1969
James E. Hansen
openalex   +1 more source

On the radio occultation method for studying planetary atmospheres [PDF]

, 1968
Robert A. Phinney, Donald L. Anderson
openalex   +1 more source

EQUATION OF RADIATIVE TRANSFER IN A PLANETARY SPHERICAL ATMOSPHERE [PDF]

, 1961
J. Lenoble, Z. Sekera
openalex   +1 more source

Injection of meteoric phosphorus into planetary atmospheres

Planetary and Space Science, 2020
J. Carrillo-Sánchez, D. Bones, K. Douglas, G. Flynn, S. Wirick, B. Fegley, T. Araki, B. Kaulich, J. Plane   +8 more
semanticscholar   +1 more source