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• W4290973816 endingPage "256" @default.
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• W4290973816 abstract "ABSTRACT The atmospheres of ultra hot Jupiters (UHJs) are prime targets for the detection of molecules and atoms at both low and high spectral resolution. We study the atmospheres of the UHJs WASP-121b and WASP-189b by performing 3D general circulation models (GCMs) of these planets using high temperature correlated-k opacity schemes with ultra-violet (UV) absorbing species included. The GCM results are then post-processed at low and high spectral resolutions and compared to available data. The high resolution results are cross-correlated with molecular and atomic templates to produce mock molecular detections. Our GCM models produce similar temperature-pressure (T-p) structure trends to previous 1D radiative-convective equilibrium models of UHJs. Furthermore, the inclusion of UV opacities greatly shapes the thermal and dynamical properties of the high-altitude, low-pressure regions of the UHJ atmospheres, with sharp T-p inversions due to the absorption of UV light. This suggests that optical wavelength, high-resolution observations probe a dynamically distinct upper atmospheric region, rather than the deeper jet forming layers." @default.
• W4290973816 created "2022-08-13" @default.
• W4290973816 creator A5019327228 @default.
• W4290973816 creator A5026236815 @default.
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• W4290973816 creator A5073596124 @default.
• W4290973816 creator A5090284169 @default.
• W4290973816 creator A5090905168 @default.
• W4290973816 date "2022-08-11" @default.
• W4290973816 modified "2023-09-25" @default.
• W4290973816 title "The Mantis Network <tt>II</tt>: examining the 3D high-resolution observable properties of the UHJs WASP-121b and WASP-189b through GCM modelling" @default.
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