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Titlebook: Giant Planets of Our Solar System; An Introduction Patrick G. J. Irwin Book 20031st edition Springer-Verlag Berlin Heidelberg 2003 giant pl

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發(fā)表于 2025-3-21 19:10:25 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書目名稱Giant Planets of Our Solar System
副標(biāo)題An Introduction
編輯Patrick G. J. Irwin
視頻videohttp://file.papertrans.cn/386/385703/385703.mp4
概述Contains in one handy volume, for the first time, all the latest data and background information on gas giant planets.- Clearly explains all specialist terms used when they are first introduced, espec
叢書名稱Springer Praxis Books
圖書封面Titlebook: Giant Planets of Our Solar System; An Introduction Patrick G. J. Irwin Book 20031st edition Springer-Verlag Berlin Heidelberg 2003 giant pl
描述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.
出版日期Book 20031st edition
關(guān)鍵詞giant planets; planetary atmospheres; solar system; atmosphere; Cloud; development; formation; temperature
版次1
doihttps://doi.org/10.1007/3-540-37713-1
isbn_ebook978-3-540-37713-9
copyrightSpringer-Verlag Berlin Heidelberg 2003
The information of publication is updating

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https://doi.org/10.1007/3-540-37713-1giant planets; planetary atmospheres; solar system; atmosphere; Cloud; development; formation; temperature
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Patrick G. J. IrwinContains in one handy volume, for the first time, all the latest data and background information on gas giant planets.- Clearly explains all specialist terms used when they are first introduced, espec
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發(fā)表于 2025-3-22 06:53:55 | 只看該作者
n 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.978-3-540-37713-9
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Book 20031st editionle 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.
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Vertical structure of temperature, composition, and clouds,
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Sources of remotely sensed data on the giant planets,
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