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Titlebook: Mercury; André Balogh,Leonid Ksanfomality,Rudolf Steiger Book 2008 Springer-Verlag New York 2008 Ionosphere.Planet.Solar.Solar wind.Sun.bo

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發(fā)表于 2025-3-21 18:31:37 | 只看該作者 |倒序瀏覽 |閱讀模式
書目名稱Mercury
編輯André Balogh,Leonid Ksanfomality,Rudolf Steiger
視頻videohttp://file.papertrans.cn/631/630917/630917.mp4
概述Only book on Mercury which balances the wide range of Earth-based observations, made under difficult conditions, with the only available space-based data from Mariner 10.Contains an in-depth review of
叢書名稱Space Sciences Series of ISSI
圖書封面Titlebook: Mercury;  André Balogh,Leonid Ksanfomality,Rudolf Steiger Book 2008 Springer-Verlag New York 2008 Ionosphere.Planet.Solar.Solar wind.Sun.bo
描述.Mercury, the planet closest to the Sun, is different in several respects from the other three terrestrial planets. In appearance, it resembles the heavily cratered surface of the Moon, but its density is high, it has a magnetic field and magnetosphere, but no atmosphere or ionosphere. This book reviews the progress made in Mercury studies since the flybys by Mariner 10 in 1974-75, based on the continued research using the Mariner 10 archive, on observations from Earth, and on increasingly realistic models of its interior evolution..
出版日期Book 2008
關鍵詞Ionosphere; Planet; Solar; Solar wind; Sun; book on Mercury; magnetosphere; planet Mercury; planetary dynamo
版次1
doihttps://doi.org/10.1007/978-0-387-77539-5
isbn_softcover978-1-4419-2655-5
isbn_ebook978-0-387-77539-5Series ISSN 1385-7525
issn_series 1385-7525
copyrightSpringer-Verlag New York 2008
The information of publication is updating

書目名稱Mercury影響因子(影響力)




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Plasma Waves in the Hermean Magnetosphere, Mercury. We further discuss a number of possible phenomena, including ULF pulsations, acceleration-related radiation, bow shock waves, bremsstrahlung (or braking radiation), and synchrotron radiation. Finally, some predictions are made as to the likelihood that some of these types of wave emission exist.
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The Origin of Mercury, on a proto-Mercury having roughly chondritic elemental abundances. We have extended the previous work on this hypothesis in two significant directions. First, we have considerably increased the resolution of the simulation of the collision itself. Second, we have addressed the fate of the ejecta fo
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