Temperature Structures Associated with Different Components of the Atmospheric Circulation on Tidally Locked Exoplanets

نویسندگان

چکیده

Observations of time-resolved thermal emission from tidally locked exoplanets can tell us about their atmospheric temperature structure. Telescopes such as JWST and ARIEL will improve the quality availability these measurements. This motivates an improved understanding processes that determine structure, particularly circulation. The circulation is important in determining temperatures, not only through its ability to transport heat, but also because any pattern needs be balanced by horizontal pressure contrasts, therefore implying a particular In this work, we show how global field on planet decomposed into contributions are different components These superrotating jet, stationary Rossby waves, divergent To achieve this, partition geopotential rotational circulation, with latter comprising jet waves. partitioned then implies corresponding partitioning via hydrostatic relation. We apply diagnostics idealised general model simulations, separate circulations together make up total three-dimensional each component contributes distinct signatures phase curve planet. conclude decomposition physically meaningful separation explains used fit observations emission.

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ژورنال

عنوان ژورنال: The Astrophysical Journal

سال: 2022

ISSN: ['2041-8213', '2041-8205']

DOI: https://doi.org/10.3847/1538-4357/ac8fed