- Implications of three|dimensional chemical transport in hot Jupiter ...🔍
- The Effect of 3D Transport|induced Disequilibrium ...🔍
- The Effect of 3D Transport|induced Disequilibrium Carbon ...🔍
- [2307.04931] Modelling the effect of 3D temperature and chemistry ...🔍
- a study of five chemical species on WASP|76b🔍
- [PDF] The Effect of 3D Transport|induced Disequilibrium Carbon ...🔍
- Modelling the effect of 3D temperature and chemistry on the cross ...🔍
- Chemical trends in Hot Jupiter atmospheres🔍
Implications of three|dimensional chemical transport in hot Jupiter ...
Implications of three-dimensional chemical transport in hot Jupiter ...
Our results show that consideration of 3D chemical transport is vital in understanding the chemical composition of hot Jupiter atmospheres.
Implications of three-dimensional chemical transport in hot Jupiter ...
Implications of three-dimensional chemical transport in hot Jupiter atmospheres: Results from a consistently coupled chemistry-radiation ...
Implications of three-dimensional chemical transport in hot Jupiter ...
We present results from a set of simulations using a fully coupled three-dimensional (3D) chemistry-radiation-hydrodynamics model and investigate the effect ...
Implications of three-dimensional chemical transport in hot Jupiter ...
We present results from a set of simulations using a fully coupled three-dimensional (3D) chemistry-radiation-hydrodynamics model and investigate the effect of ...
Implications of three-dimensional chemical transport in hot Jupiter ...
Implications of three-dimensional chemical transport in hot Jupiter atmospheres: Results from a consistently coupled chemistry-radiation-hydrodynamics model ...
Implications of three-dimensional chemical transport in hot Jupiter ...
Request PDF | Implications of three-dimensional chemical transport in hot Jupiter atmospheres: Results from a consistently coupled ...
The Effect of 3D Transport-induced Disequilibrium ... - NASA ADS
The Effect of 3D Transport-induced Disequilibrium Carbon Chemistry on the Atmospheric Structure, Phase Curves, and Emission Spectra of Hot Jupiter HD 189733b.
The Effect of 3D Transport-induced Disequilibrium Carbon ...
On hot Jupiter exoplanets, strong horizontal and vertical winds should homogenize the abundances of the important absorbers CH4 and CO much ...
The Effect of 3D Transport-induced Disequilibrium Carbon ...
On hot Jupiter exoplanets, strong horizontal and vertical winds should homogenize the abundances of the important absorbers CH4 and CO much faster than chemical ...
[2307.04931] Modelling the effect of 3D temperature and chemistry ...
Abstract:Ultra-hot Jupiters are perfect targets for transmission spectroscopy. However, their atmospheres feature strong spatial variations ...
a study of five chemical species on WASP-76b - Oxford Academic
Ultra-hot Jupiters are perfect targets for transmission spectroscopy. However, their atmospheres feature strong spatial variations in temperature, chemistry, ...
[PDF] The Effect of 3D Transport-induced Disequilibrium Carbon ...
The Effect of 3D Transport-induced Disequilibrium Carbon Chemistry on the Atmospheric Structure, Phase Curves, and Emission Spectra of Hot Jupiter HD 189733b.
Modelling the effect of 3D temperature and chemistry on the cross ...
At high resolution, the '3D-ness' of ultra-hot Jupiters causes the ... sectors during the transit, and (ii) atmospheric dynamics. In tandem ...
Chemical trends in Hot Jupiter atmospheres
Abundances in the Atmospheres of Three Hot Jupiters. ... The Effect of 3D Transport-induced Disequilibrium Carbon Chemistry on the Atmo-.
Implications of Disequilibrium Chemistry and Photochemical Hazes
The temperature changes by 50 to 100 K for the range of methane abundances expected from chemical kinetics calculations, with the dayside cooling and the ...
Hot Jupiters: Origins, Structure, Atmospheres - AGU Journals - Wiley
There are three main hypotheses for the origins of hot Jupiters: in situ formation, disk migration, and high eccentricity migration (Figure 1).
solar system - Effects of Hot Jupiters on habitable planets
The simulations by Fogg & Nelson indicate that volatiles from beyond the snow line would be mixed with the inner disk debris, leading to ...
Implications of three-dimensional chemical transport in hot Jupiter atmospheres: results from a consistently coupled chemistry-radiation-hydrodynamics model.
Nightside clouds and disequilibrium chemistry on the hot Jupiter ...
Comparisons with three-dimensional atmospheric models show that both the phase-curve shape and emission spectra strongly suggest the presence of ...
Understanding Atmospheric Escape of Hot Jupiters Using Radiation ...
have not followed the multi-dimensional effect (Christie et al. 2016 ... To understand the observed transit signature, the multi-dimensional hydrodynamics.