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Giant planets of our solar system: an introduction [Libro electrónico] / Patrick G. J. Irwin

Por: Irwin, Patrick G. J [autor/a].
Tipo de material: Libro en línea Libro en línea Series Editor: New York, New York, United States: Springer, c2003Descripción: xxiv, 320 páginas : ilustraciones ; 24 centímetros.ISBN: 3540313176; 9783540313175 (Print); 9783540377139 (Online).Tema(s): Planets -- AtmospheresDescriptor(es) geográficos: Jupiter (Planet) | Saturn (Planet) | Uranus (Planet) | Neptune (Planet)Nota de acceso: Disponible para usuarios de ECOSUR con su clave de acceso Nota de bibliografía: Incluye bibliografía e índice: páginas 313-320 Número de sistema: 55684Contenidos:Mostrar Resumen:
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This bookreviews the current state of knowledge of the atmospheres of the giant gaseous planets: Jupiter, Saturn, Uranus, and Neptune. The current theories of their formation are reviewed and their recently observed temperature, composition and cloud structures are contrasted and compared with simple thermodynamic, radiative transfer and dynamical models. The instruments and techniques that have been used to remotely measure their atmospheric properties are also reviewed, and the likely development of outer planet observations over the next two decades is outlined.

Recurso en línea: http://link.springer.com/openurl?genre=book&isbn=978-3-540-31317-5
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Recursos en línea (RE) 		Acervo General Recurso digital ECO40055684133

Incluye bibliografía e índice: páginas 313-320

1. Introduction.. 2. Formation of the giant planets.. 3. Evolution processes in outer planet atmospheres.. 4. Vertical structure of temperature, composition, and clouds.. 5. Dynamical processes.. 6. Radiative transfer processes in outer planetary atmospheres.. 7. Sources of remotely sensed data on the giant planets.. Index

Disponible para usuarios de ECOSUR con su clave de acceso

This bookreviews the current state of knowledge of the atmospheres of the giant gaseous planets: Jupiter, Saturn, Uranus, and Neptune. The current theories of their formation are reviewed and their recently observed temperature, composition and cloud structures are contrasted and compared with simple thermodynamic, radiative transfer and dynamical models. The instruments and techniques that have been used to remotely measure their atmospheric properties are also reviewed, and the likely development of outer planet observations over the next two decades is outlined. eng

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