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Non-Lte Radiative Transfer in the Atmosphere.

During the last three decades, it has become increasingly clear that atmospheric modelling and remote sounding of the atmosphere from space, to name just two important application areas, are affected by non-equilibrium processes which have not been incorporated into traditional radiative transfer ca...

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Detalles Bibliográficos
Clasificación:Libro Electrónico
Autor principal: Taylor, F. W.
Formato: Electrónico eBook
Idioma:Inglés
Publicado: Singapore : World Scientific Publishing Company, 2001.
Colección:Series on atmospheric, oceanic and planetary physics.
Temas:
Acceso en línea:Texto completo

MARC

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100 1 |a Taylor, F. W. 
245 1 0 |a Non-Lte Radiative Transfer in the Atmosphere. 
260 |a Singapore :  |b World Scientific Publishing Company,  |c 2001. 
300 |a 1 online resource (506 pages) 
336 |a text  |b txt  |2 rdacontent 
337 |a computer  |b c  |2 rdamedia 
338 |a online resource  |b cr  |2 rdacarrier 
490 1 |a Series on Atmospheric, Oceanic and Planetary Physics 
588 0 |a Print version record. 
520 |a During the last three decades, it has become increasingly clear that atmospheric modelling and remote sounding of the atmosphere from space, to name just two important application areas, are affected by non-equilibrium processes which have not been incorporated into traditional radiative transfer calculations. These processes, dubbed "non-LTE", are therefore the subject of growing interest among scholars and researchers dealing with the upper atmosphere. This important book provides the first comprehensive and "global" description of non-LTE infrared emissions in the atmosphere of the Earth an. 
505 0 |a Preface ; Chapter 1 Introduction and Overview ; 1.1 General Introduction ; 1.2 Basic Properties of the Earth's Atmosphere ; 1.2.1 Thermal structure ; 1.2.2 Composition ; 1.2.3 Energy balance ; 1.3 What is LTE? ; 1.4 Non-LTE Situations ; 1.5 The Importance of Non-LTE. 
505 8 |a 1.6 Some Historical Background 1.7 Non-LTE Models ; 1.8 Experimental Studies of Non-LTE ; 1.9 Non-LTE in Planetary Atmospheres ; 1.10 References and Further Reading ; Chapter 2 Molecular Spectra ; 2.1 Introduction ; 2.2 Energy Levels in Diatomic Molecules. 
505 8 |a 2.2.1 The Born-Oppenheimer approximation 2.2.2 Rotation of diatomic molecules ; 2.2.3 Vibrations of diatomic molecules ; 2.2.4 Breakdown of the Born-Oppenheimer approximation ; 2.3 Energy Levels in Polyatomic Molecules ; 2.3.1 General ; 2.3.2 Rotation of polyatomic molecules. 
505 8 |a 2.3.3 Vibration of polyatomic molecules 2.4 Transitions and Spectral Bands ; 2.4.1 The vibration-rotation band ; 2.4.2 Hot bands ; 2.4.3 Overtone bands ; 2.4.4 Isotope bands ; 2.4.5 Combination bands ; 2.5 Properties of Individual Vibration-Rotation Lines. 
505 8 |a 2.5.1 Spectral line strength 2.5.2 Widths and shapes of spectral lines ; 2.6 Interactions between Energy Levels ; 2.6.1 Fermi resonance ; 2.6.2 Coriolis interaction ; 2.6.3 Vibration-vibration transfer ; 2.7 References and Further Reading. 
590 |a ProQuest Ebook Central  |b Ebook Central Academic Complete 
650 0 |a Atmospheric thermodynamics. 
650 0 |a Planets  |x Atmospheres. 
650 0 |a Radiative transfer. 
650 6 |a Thermodynamique de l'atmosphère. 
650 6 |a Planètes  |x Atmosphères. 
650 6 |a Transfert radiatif. 
650 7 |a Atmospheric thermodynamics  |2 fast 
650 7 |a Planets  |x Atmospheres  |2 fast 
650 7 |a Radiative transfer  |2 fast 
776 0 8 |i Print version:  |z 9789810245665 
830 0 |a Series on atmospheric, oceanic and planetary physics. 
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