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Titlebook: Magnetic Fields in the Solar System; Planets, Moons and S Hermann Lühr,Johannes Wicht,Matthias Holschneider Book 2018 Springer Internationa

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發(fā)表于 2025-3-21 19:44:56 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書目名稱Magnetic Fields in the Solar System
副標(biāo)題Planets, Moons and S
編輯Hermann Lühr,Johannes Wicht,Matthias Holschneider
視頻videohttp://file.papertrans.cn/622/621228/621228.mp4
概述Provides a broad overview of magnetic fields in our solar system and the modern methods employed to unravel their complexity.Results from a research program involving four leading planetary science in
叢書名稱Astrophysics and Space Science Library
圖書封面Titlebook: Magnetic Fields in the Solar System; Planets, Moons and S Hermann Lühr,Johannes Wicht,Matthias Holschneider Book 2018 Springer Internationa
描述.This book addresses and reviews many of the still little understood questions related to the processes underlying planetary magnetic fields and their interaction with the solar wind. With focus on research carried out within the German Priority Program ”PlanetMag”, it also provides an overview of the most recent research in the field. .Magnetic fields play an important role in making a planet habitable by protecting the environment from the solar wind. Without the geomagnetic field, for example, life on Earth as we know it would not be possible. And results from recent space missions to Mars and Venus strongly indicate that planetary magnetic fields play a vital role in preventing atmospheric erosion by the solar wind. However, very little is known about the underlying interaction between the solar wind and a planet’s magnetic field. . .The book takes a synergistic interdisciplinary approach that combines newly developed tools for data acquisition and analysis,computer simulations of planetary interiors and dynamos, models of solar wind interaction, measurement of ancient terrestrial rocks and meteorites, and laboratory investigations..
出版日期Book 2018
關(guān)鍵詞Earth magnetic field; planetary dynamo simulations; planetary interior dynamics; magnetic instability; J
版次1
doihttps://doi.org/10.1007/978-3-319-64292-5
isbn_softcover978-3-319-87765-5
isbn_ebook978-3-319-64292-5Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightSpringer International Publishing AG 2018
The information of publication is updating

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發(fā)表于 2025-3-21 23:13:34 | 只看該作者
Modeling the Interior Dynamics of Gas Planets,Zonal jet systems very similar to those observed on Jupiter or Saturn are found in simulations of the molecular hydrogen envelope. Dynamo simulations that include the whole gaseous envelope show strikingly Jupiter-like magnetic field configurations when the strong density stratification is combined
板凳
發(fā)表于 2025-3-22 01:18:02 | 只看該作者
Global Geomagnetic Field Reconstructions from Centuries to Excursions,and age uncertainties are the prerequisite for long-term geomagnetic field models. Upgrading the GEOMAGIA50 database for archeomagnetic and volcanic data spanning the past 50?ka years and adding a new part for sediments were important achievements in this regard. The database now offers possibilitie
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Modeling Magnetospheric Fields in the Jupiter System,ilar to most of the extrasolar planets which orbit their host stars within 0.1?AU. New numerical models of Jupiter’s and Ganymede’s magnetospheres presented here provide quantitative insight into these magnetospheres and the processes which maintain them. Jupiter’s magnetospheric field is time-varia
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發(fā)表于 2025-3-22 19:22:52 | 只看該作者
,Modeling of the Ionospheric Current System and Calculating Its Contribution to the Earth’s Magneticheric current system is the first aim of this investigation. For our study, we use the Potsdam version of the Upper Atmosphere Model (UAM-P). The UAM is a first-principle, time-dependent, and fully self-consistent numerical global model. The model includes the thermosphere, ionosphere, plasmasphere,
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發(fā)表于 2025-3-23 05:09:14 | 只看該作者
,Mars’ Crustal Magnetic Field,utline under which constraints paleopole positions can be determined from satellite measurements. In a second step, we use these insights to present a scheme to estimate paleopole positions including an assessment of their underlying uncertainties.
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