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Titlebook: Mars’ Magnetism and Its Interaction with the Solar Wind; Daniel Winterhalter,Mario Acu?a,Alexander Zakharov Book 2004 Springer Science+Bus

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發(fā)表于 2025-3-21 18:56:15 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書(shū)目名稱Mars’ Magnetism and Its Interaction with the Solar Wind
編輯Daniel Winterhalter,Mario Acu?a,Alexander Zakharov
視頻videohttp://file.papertrans.cn/625/624866/624866.mp4
概述A primary reference for the researcher studying solar wind/planet interactions.Includes supplementary material:
叢書(shū)名稱Space Sciences Series of ISSI
圖書(shū)封面Titlebook: Mars’ Magnetism and Its Interaction with the Solar Wind;  Daniel Winterhalter,Mario Acu?a,Alexander Zakharov Book 2004 Springer Science+Bus
描述.Given that the question of an internal magnetic field is of fundamental importance to the understanding of Mars‘ formation and thermal evolution, and of the evolution of Mars‘ atmosphere, surprisingly few of the many spacecraft sent to Mars were equipped with instrumentation for such investigations. Of the 9 or so orbiters that have successfully archived Mars orbit, even if for a short period of time, only two have returned useful data about the magnetic field and about the plasma environment near Mars: The Phobos 2 spacecraft, and more recently, Mars Global Surveyor (MGS). ..With the discovery by MGS that Mars has large remnant magnetic field structures indicating an internal dynamo long extinct, the true nature of the past and present interaction between Mars and the solar wind comes, for the first time, into sharp focus. This work, detailing the integration and new interpretation of the MGS and Phobos results, is a primary reference for the researcher studying solar wind/planet interactions. .
出版日期Book 2004
關(guān)鍵詞Planet; Solar wind; magnetic field; magnetism; solar
版次1
doihttps://doi.org/10.1007/978-0-306-48604-3
isbn_softcover978-90-481-6582-7
isbn_ebook978-0-306-48604-3Series ISSN 1385-7525
issn_series 1385-7525
copyrightSpringer Science+Business Media Dordrecht 2004
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沙發(fā)
發(fā)表于 2025-3-21 20:34:04 | 只看該作者
Daniel Winterhalter,Mario Acu?a,Alexander ZakharovA primary reference for the researcher studying solar wind/planet interactions.Includes supplementary material:
板凳
發(fā)表于 2025-3-22 01:27:17 | 只看該作者
Space Sciences Series of ISSIhttp://image.papertrans.cn/m/image/624866.jpg
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發(fā)表于 2025-3-22 05:46:22 | 只看該作者
978-90-481-6582-7Springer Science+Business Media Dordrecht 2004
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發(fā)表于 2025-3-22 09:02:12 | 只看該作者
Mars’ Magnetism and Its Interaction with the Solar Wind978-0-306-48604-3Series ISSN 1385-7525
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發(fā)表于 2025-3-22 14:38:15 | 只看該作者
The Plasma Environment of Marsservations. However, measurements by the Phobos-2 and Mars Global Surveyor (MGS) spacecraft, with different instrument complements and orbital parameters, led to a significant improvement of our knowledge about the regions and boundaries surrounding Mars.
7#
發(fā)表于 2025-3-22 17:55:48 | 只看該作者
1385-7525 an internal magnetic field is of fundamental importance to the understanding of Mars‘ formation and thermal evolution, and of the evolution of Mars‘ atmosphere, surprisingly few of the many spacecraft sent to Mars were equipped with instrumentation for such investigations. Of the 9 or so orbiters th
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發(fā)表于 2025-3-22 23:34:04 | 只看該作者
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發(fā)表于 2025-3-23 04:51:21 | 只看該作者
Mars Crustal Magnetism an inner core is likely. Thermal evolution models cannot yet distinguish between these two possibilities. The magnetic record contains a wealth of information on the thermal evolution of Mars and the Mars dynamo, but we have just begun to decipher its message.
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發(fā)表于 2025-3-23 09:15:08 | 只看該作者
Unusually Distant Bow Shock Encounters at Mars: Analysis of March 24, 1989 Eventystem of discontinuities observed in the solar wind between 18:42 and 19:36 UT was the consequence of unusually distant planetary bow shock excursions. The cause was unusually small ρV. and .. values in the solar wind flow.
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