Giant Planets of Our Solar System: An Introduction

Copertina anteriore
Springer Science & Business Media, 27 gen 2006 - 320 pagine
This book reviews 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.
 

Sommario

Formation of the giant planets 17
16
5
32
Evolution processes in outer planet atmospheres
53
3
59
Vertical structure of temperature composition and clouds
88
2
103
Dynamical processes
133
Radiative transfer processes in outer planetary atmospheres
197
ThermalIR spectra
236
4
247
Measurement of visible IR and microwave spectra
248
3
259
Groundbased visibleIR observatories
261
6
270
7
276
Index
311

4
212
Nonspherical particles
229

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