Thermal tides on a hot Jupiter

Following the linear analysis laid out by Gu & Ogilvie 2009 (hereafter GO09), we investigate the dynamical response of a non-synchronized hot Jupiter to stellar irradiation. Besides the internal and Rossby waves considered by GO09, we study the Kelvin waves excited by the diurnal Fourier harmoni...

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Main Authors: Hsieh H.-F., Gu P.-G.
Format: Article
Language:English
Published: EDP Sciences 2011-07-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/20111604003
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spelling doaj-0d3c07dc8b6046ef83957ef5f45c1e682021-08-02T18:21:59ZengEDP SciencesEPJ Web of Conferences2100-014X2011-07-01160400310.1051/epjconf/20111604003Thermal tides on a hot JupiterHsieh H.-F.Gu P.-G.Following the linear analysis laid out by Gu & Ogilvie 2009 (hereafter GO09), we investigate the dynamical response of a non-synchronized hot Jupiter to stellar irradiation. Besides the internal and Rossby waves considered by GO09, we study the Kelvin waves excited by the diurnal Fourier harmonic of the prograde stellar irradiation. We also present a 2-dimensional plot of internal waves excited by the semi-diurnal component of the stellar irradiation and postulate that thermal bulges may arise in a hot Jupiter. Whether our postulation is valid and is consistent with the recent results from Arras & Socrates (2009b) requires further investigation. http://dx.doi.org/10.1051/epjconf/20111604003
collection DOAJ
language English
format Article
sources DOAJ
author Hsieh H.-F.
Gu P.-G.
spellingShingle Hsieh H.-F.
Gu P.-G.
Thermal tides on a hot Jupiter
EPJ Web of Conferences
author_facet Hsieh H.-F.
Gu P.-G.
author_sort Hsieh H.-F.
title Thermal tides on a hot Jupiter
title_short Thermal tides on a hot Jupiter
title_full Thermal tides on a hot Jupiter
title_fullStr Thermal tides on a hot Jupiter
title_full_unstemmed Thermal tides on a hot Jupiter
title_sort thermal tides on a hot jupiter
publisher EDP Sciences
series EPJ Web of Conferences
issn 2100-014X
publishDate 2011-07-01
description Following the linear analysis laid out by Gu & Ogilvie 2009 (hereafter GO09), we investigate the dynamical response of a non-synchronized hot Jupiter to stellar irradiation. Besides the internal and Rossby waves considered by GO09, we study the Kelvin waves excited by the diurnal Fourier harmonic of the prograde stellar irradiation. We also present a 2-dimensional plot of internal waves excited by the semi-diurnal component of the stellar irradiation and postulate that thermal bulges may arise in a hot Jupiter. Whether our postulation is valid and is consistent with the recent results from Arras & Socrates (2009b) requires further investigation.
url http://dx.doi.org/10.1051/epjconf/20111604003
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