Results 111 to 120 of about 13,254 (205)
With the launch of the James Webb Space Telescope, we are firmly in the era of exoplanet atmosphere characterization. Understanding exoplanet spectra requires atmospheric simulations that span the diversity of planetary atmospheres.
Nicholas F. Wogan +9 more
doaj +1 more source
Lightning and charge processes in brown dwarf and exoplanet atmospheres. [PDF]
Helling C, Rimmer PB.
europepmc +1 more source
Limited Hysteresis in the Atmospheric Dynamics of Hot Jupiters
Over the past two decades, a coherent picture has emerged of the atmospheric dynamics of hot Jupiters from a combination of three-dimensional general circulation models and astronomical observations.
Thaddeus D. Komacek
doaj +1 more source
Exoplanet Atmospheres at High Spectral Resolution
High-resolution spectroscopy (HRS) has grown into one of the main techniques for characterizing the atmospheres of extrasolar planets. High spectral resolving power allows for the efficient removal of telluric and host-star contamination. Combined with the large collecting area of ground-based telescopes, it enables detailed studies of atmospheric ...
openaire +2 more sources
Towards Atmospheric Characterisation of Exoplanets
This thesis provides a multi-pronged approach towards paving the way for future space and ground based exoplanet characterisation e↵orts as well as providing new analysis of the atmosphere of the exoplanet HD 179949 b. This is done, firstly, by outlining engineering trade studies conducted for the attitude and orbit control system (AOCS) and sun shield
openaire +2 more sources
Minimizing Star-spot Contamination of Exoplanet Transit Spectroscopy Using Alternate Normalization
Recently, M. H. Currie et al. (2023) simulated the detection of molecules in the atmospheres of temperate rocky exoplanets transiting nearby M-dwarf stars.
Drake Deming +3 more
doaj +1 more source
Comparing Results from Two Uniform Phase-curve Surveys
We present a comparison of the two most recent and comprehensive Spitzer phase curve studies—L. Dang et al. and M. R. Swain et al.—which report analyses of the Spitzer 4.5 μ m phase curves.
Emeline Decocq +4 more
doaj +1 more source
Secondary eclipse observations are a powerful way to investigate whether or not a rocky exoplanet hosts an atmosphere, as an atmospheric presence would transport heat to the nightside and render the dayside colder than anticipated.
Christopher Monaghan +4 more
doaj +1 more source
Tropical Cyclones on Tidally Locked Rocky Planets: Dependence on Rotation Period
Tropical cyclones occur over the Earth’s tropical oceans, with characteristic genesis regions and tracks tied to the warm ocean surface that provide energy to sustain these storms.
Valeria Garcia +3 more
doaj +1 more source
Instrumentation prospects for rocky exoplanet atmospheres studies with high resolution spectroscopy. [PDF]
Rukdee S.
europepmc +1 more source

