Titlebook: Giant Planets of Our Solar System; Atmospheres, Composi Patrick G. J. Irwin Book 2009Latest edition Springer-Verlag Berlin Heidelberg 2009

Colossal

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全国性

亚当心理阴影

carbohydrate

Dynamical processes,erial are transported, not just vertically, but horizontally as well. In this chapter we will consider the basic equations of fluid motion in rotating planetary atmospheres and see how these theoretical considerations relate to the observed winds, clouds, and storm systems observed in the atmospheres of the giant planets.

错

Book 2009Latest editionen extensively updated following the Cassini mission results for Jupiter/Saturn and the newest ground-based measurements for Uranus/Neptune as well as on the latest development in the theories on planet formation..

d-limonene

d-limonene

reperfusion

Introduction,in Jean Joseph Le Verrier (1811–1877) to independently predict the presence of a further planet, and Neptune was subsequently discovered close to its predicted position by Johann Gottfried Galle (1812–1910) in 1846. The mean observable properties of the outer planets are listed in Table 1.1.

AWE

Future of giant planet observations,ew measurements are expected in the next few years which will further improve our understanding of these giant worlds, and how they formed from circumplanetary disks. Some of the key questions concerning the atmospheres of the giant planets that still remain are

certain

Book 2009Latest editionheories 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 p