The is for high-resolution optical spectroscopy. It studies exoplanet atmospheres to determine the vertical thermal structure, or T-P profile .
: The T-P profile shows how temperature changes with atmospheric pressure. In "ultra-hot Jupiters" like WASP-189 b, this profile often shows a thermal inversion . The atmosphere gets hotter at higher altitudes because of the absorption of stellar radiation by species like titanium oxide (TiO) or iron (Fe). Case Study: WASP-189 b Observations gost na asu tp
: Scientists compare observed spectra with theoretical models at different T-P points. This helps identify the temperature and pressure levels where certain elements exist. Structure for a Technical Write-up The is for high-resolution optical spectroscopy
: Define the exoplanet (e.g., WASP-189 b) and the use of high-resolution spectroscopy for atmospheric characterization. In "ultra-hot Jupiters" like WASP-189 b, this profile
: Discuss the detected species and whether the T-P profile indicates an atmospheric inversion or a "non-inverted" (decreasing temperature with height) structure. High-resolution Dayside Spectroscopy of WASP-189 b
