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Theory of Planetary Atmospheres : an Introduction to Their Physics and Chemistry.

Our subject is, of course, nothing more than applied physics and chemistry. But in addition to those basic sciences the student of planetary atmospheres needs an overview of atmospheric structure and physical processes as presently understood. This book is intended to help fill that need for both gr...

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Detalles Bibliográficos
Clasificación:Libro Electrónico
Autor principal: Chamberlain, Joseph W.
Otros Autores: Hunten, Donald M.
Formato: Electrónico eBook
Idioma:Inglés
Publicado: Burlington : Elsevier Science, 1989.
Temas:
Acceso en línea:Texto completo

MARC

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245 1 0 |a Theory of Planetary Atmospheres :  |b an Introduction to Their Physics and Chemistry. 
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505 0 |a Front Cover; Theory of Planetary Atmospheres: An Introduction to Their Physics and Chemistry; Copyright Page; CONTENTS; Preface to the Second Edition; Preface to the First Edition; Chapter 1. Vertical Structure of an Atmosphere; Chapter 2. Hydrodynamics of Atmospheres; Chapter 3. Chemistry and Dynamics of Earth's Stratosphere; Chapter 4. Planetary Astronomy; Chapter 5. Ionospheres; Chapter 6. Airglows, Auroras, and Aeronomy; Chapter 7. Stability of Planetary Atmospheres; Appendix I: A Table of Physical Constants; Appendix II: Planetary Characteristics. 
505 8 |a Appendix III: A Model of Earth's AtmosphereAppendix IV: Planetary Spacecraft Missions; Appendix V: Supplementary Reading; Appendix VI: The Planck Function; Appendix VII: Diffusion Coefficients; Appendix VIII: Ortho and Para Hydrogen; Appendix IX: Partition Functions for a Spherical Exosphere; Index. 
520 |a Our subject is, of course, nothing more than applied physics and chemistry. But in addition to those basic sciences the student of planetary atmospheres needs an overview of atmospheric structure and physical processes as presently understood. This book is intended to help fill that need for both graduate students and research scientists. Although the approach is mainly theoretical, very little basic physics is developed here. Material that is standard fare in third- and fourth-year physics courses is simply absorbed where needed. 
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