Results 81 to 90 of about 47,597 (232)

Ames facility for simulating planetary probe heating environments [PDF]

open access: yes, 1974
Progress is reported on the development of a giant-planet pilot facility which simulates the conditions expected at the peak heating point for a shallow entry into the atmosphere of Saturn, Jupiter, and ...
Stine, H. A.
core   +1 more source

Atmospheric Circulation of Hot Jupiters: A Shallow Three-Dimensional Model

open access: yes, 2009
Remote observing of exoplanetary atmospheres is now possible, offering us access to circulation regimes unlike any of the familiar Solar System cases. Atmospheric circulation models are being developed to study these new regimes but model validations and
Barman   +49 more
core   +1 more source

JWST-TST DREAMS: A Precise Water Abundance for Hot Jupiter WASP-17b from the NIRISS SOSS Transmission Spectrum

open access: yesThe Astronomical Journal
Water has proven to be ubiquitously detected in near-infrared (NIR) transmission spectroscopy observations of hot Jupiter atmospheres, including WASP-17b.
Dana R. Louie   +29 more
doaj   +1 more source

Jovian Vortices and Jets

open access: yesFluids, 2019
We explore the theory of isolated vortices in strongly sheared, deep zonal flows and the stability of these banded jets, as occur in Jupiter’s atmosphere This is done using the standard 2-layer quasigeostrophic model with the lower layer depth ...
Glenn R. Flierl   +2 more
doaj   +1 more source

Transit Thermal Control Design for Galileo Entry Probe for Planet Jupiter [PDF]

open access: yes, 1982
A totally passive design was completed for the thermal control of the Galileo entry probe during its transit to the planet Jupiter. The design utilizes radio isotope heater units, multilayer insulation blankets and a thermal radiator in conjunction with ...
Haverly, George C., Pitts, William
core   +1 more source

The Effect of Condensates on the Characterization of Transiting Planet Atmospheres with Transmission Spectroscopy

open access: yes, 2005
Through a simple physical argument we show that the slant optical depth through the atmosphere of a "hot Jupiter" planet is 35-90 times greater than the normal optical depth.
Ackerman   +40 more
core   +3 more sources

Hydrogen sulfide detection and strong methane depletion in the super-stellar metallicity atmosphere of hot Jupiter HD 189733b [PDF]

open access: green, 2023
Guangwei Fu   +16 more
openalex   +1 more source

Predicting CO Cameron‐Band Auroral Emission at Venus Using VEx Electron Observations

open access: yesGeophysical Research Letters
Various types of auroral emissions have been observed at (partially) magnetized planets (e.g., Earth, Jupiter, and Mars). Auroral emissions have also been observed at Venus, an unmagnetized planet, by the Pioneer Venus Orbiter (PVO) and ground‐based ...
Shaosui Xu   +7 more
doaj   +1 more source

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