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Atmospheric Responses to Radiative F...

Adams, Arthur Daniel.

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Atmospheric Responses to Radiative Forcing: Physics and Observability of Close-in and Highly Eccentric Planets.

Record Type:	Electronic resources : Monograph/item
Title/Author:	Atmospheric Responses to Radiative Forcing: Physics and Observability of Close-in and Highly Eccentric Planets./
Author:	Adams, Arthur Daniel.
Published:	Ann Arbor : ProQuest Dissertations & Theses, : 2019,
Description:	233 p.
Notes:	Source: Dissertations Abstracts International, Volume: 81-10, Section: B.
Contained By:	Dissertations Abstracts International81-10B.
Subject:	Astronomy. -
Online resource:	http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=22621604
ISBN:	9798607313487

Atmospheric Responses to Radiative Forcing: Physics and Observability of Close-in and Highly Eccentric Planets.
Adams, Arthur Daniel.

Atmospheric Responses to Radiative Forcing: Physics and Observability of Close-in and Highly Eccentric Planets. - Ann Arbor : ProQuest Dissertations & Theses, 2019 - 233 p.

Source: Dissertations Abstracts International, Volume: 81-10, Section: B.

Thesis (Ph.D.)--Yale University, 2019.

This item must not be sold to any third party vendors.

The thermal emission of exoplanets contains valuable information about the structures of their atmospheres. However, the current quality of observations allows for only a limited understanding of the physics at play. With this in mind we focus on infrared observables of close-in and eccentric planets, whose atmospheric responses may be characterized to leading order by the cycles of stellar forcing from their orbits and rotation. We approach modeling using a range of physical complexities. Firstly, we demonstrate in a re-assessment of Spitzer orbital phase curves that their shapes in many cases are well fit by a simple thermal model, in comparison with models of considerably more complexity. A few Hot Jupiters show phase offsets counter to the expectation of super-rotating winds on a tidally-locked planet; we detail the efficacy, feasibility, and observable consequences of high planet obliquity in reproducing these offsets. Finally, we explore the broad effects of high eccentricity and rotation rate on potentially observable phase variations from ocean-rich worlds, using the capabilities of a fully 3-dimensional climate model.

ISBN: 9798607313487Subjects--Topical Terms:

517668
Astronomy.
Subjects--Index Terms:

Atmospheres

Atmospheric Responses to Radiative Forcing: Physics and Observability of Close-in and Highly Eccentric Planets.
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245 1 0 $a Atmospheric Responses to Radiative Forcing: Physics and Observability of Close-in and Highly Eccentric Planets.
260 1 $a Ann Arbor : $b ProQuest Dissertations & Theses, $c 2019
300 $a 233 p.
500 $a Source: Dissertations Abstracts International, Volume: 81-10, Section: B.
500 $a Advisor: Laughlin, Gregory P.
502 $a Thesis (Ph.D.)--Yale University, 2019.
506 $a This item must not be sold to any third party vendors.
520 $a The thermal emission of exoplanets contains valuable information about the structures of their atmospheres. However, the current quality of observations allows for only a limited understanding of the physics at play. With this in mind we focus on infrared observables of close-in and eccentric planets, whose atmospheric responses may be characterized to leading order by the cycles of stellar forcing from their orbits and rotation. We approach modeling using a range of physical complexities. Firstly, we demonstrate in a re-assessment of Spitzer orbital phase curves that their shapes in many cases are well fit by a simple thermal model, in comparison with models of considerably more complexity. A few Hot Jupiters show phase offsets counter to the expectation of super-rotating winds on a tidally-locked planet; we detail the efficacy, feasibility, and observable consequences of high planet obliquity in reproducing these offsets. Finally, we explore the broad effects of high eccentricity and rotation rate on potentially observable phase variations from ocean-rich worlds, using the capabilities of a fully 3-dimensional climate model.
590 $a School code: 0265.
650 4 $a Astronomy. $3 517668
650 4 $a Astrophysics. $3 535904
650 4 $a Atmospheric sciences. $3 3168354
653 $a Atmospheres
653 $a Atmospheric characterization
653 $a Exoplanets
653 $a Phase curves
653 $a Photometry
690 $a 0606
690 $a 0596
690 $a 0725
710 2 $a Yale University. $b Astronomy. $3 3550212
773 0 $t Dissertations Abstracts International $g 81-10B.
790 $a 0265
791 $a Ph.D.
792 $a 2019
793 $a English
856 4 0 $u http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=22621604