Exact results in modeling planetary atmospheres - I. Gray atmospheres

被引：9

作者：

Chevallier, L.

Pelkowski, J.

Rutily, B.

机构：

[1] Observ Paris, Lab LUTH, F-92195 Meudon, France

[2] Univ Frankfurt, Inst Meteorol & Geophys, D-60325 Frankfurt, Germany

[3] Univ Lyon 1, F-69622 Villeurbanne, France

[4] Univ Lyon, F-69000 Lyon, France

[5] Observ Lyon, Ctr Rech Astron Lyon, F-69561 St Genis Laval, France

[6] Ecole Normale Super Lyon, CNRS, UMR 5574, F-69364 Lyon, France

来源：

JOURNAL OF QUANTITATIVE SPECTROSCOPY & RADIATIVE TRANSFER | 2007年 / 104卷 / 03期

关键词：

planetary atmospheres; radiative transfer; isotropic scattering; gray opacity; radiative equilibrium; temperature distribution;

D O I：

10.1016/j.jqsrt.2006.09.006

中图分类号：

O43 [光学];

学科分类号：

070207 ; 0803 ;

摘要：

An exact model is proposed for a gray, isotropically scattering planetary atmosphere in radiative equilibrium. The slab is illuminated on one side by a collimated beam and is bounded on the other side by an emitting and partially reflecting ground. We provide expressions for the incident and reflected fluxes on both boundary surfaces, as well as the temperature of the ground and the temperature distribution in the atmosphere, assuming the latter to be in local thermodynamic equilibrium. Tables and curves of the temperature distribution are included for various values of the optical thickness. Finally, semi-infinite atmospheres illuminated from the outside or by sources at infinity is dealt with. (c) 2006 Elsevier Ltd. All rights reserved.

引用

页码：357 / 376

页数：20

共 21 条

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[Anonymous], SITZUNGSBERICHT K MP

[3]

[Anonymous], GOTTINGER NACHR

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