找回密碼
 To register

QQ登錄

只需一步，快速開(kāi)始

掃一掃，訪問(wèn)微社區(qū)

打印 上一主題 下一主題

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

[復(fù)制鏈接]
查看: 17752|回復(fù): 50
樓主
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(shū)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(shū)名稱Astrophysics and Space Science Library
圖書(shū)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 ”P(pán)lanetMag”, 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

書(shū)目名稱Magnetic Fields in the Solar System影響因子(影響力)




書(shū)目名稱Magnetic Fields in the Solar System影響因子(影響力)學(xué)科排名




書(shū)目名稱Magnetic Fields in the Solar System網(wǎng)絡(luò)公開(kāi)度




書(shū)目名稱Magnetic Fields in the Solar System網(wǎng)絡(luò)公開(kāi)度學(xué)科排名




書(shū)目名稱Magnetic Fields in the Solar System被引頻次




書(shū)目名稱Magnetic Fields in the Solar System被引頻次學(xué)科排名




書(shū)目名稱Magnetic Fields in the Solar System年度引用




書(shū)目名稱Magnetic Fields in the Solar System年度引用學(xué)科排名




書(shū)目名稱Magnetic Fields in the Solar System讀者反饋




書(shū)目名稱Magnetic Fields in the Solar System讀者反饋學(xué)科排名




單選投票, 共有 1 人參與投票
 

1票 100.00%

Perfect with Aesthetics
 

0票 0.00%

Better Implies Difficulty
 

0票 0.00%

Good and Satisfactory
 

0票 0.00%

Adverse Performance
 

0票 0.00%

Disdainful Garbage
您所在的用戶組沒(méi)有投票權(quán)限
沙發(fā)
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
地板
發(fā)表于 2025-3-22 05:33:05 | 只看該作者
5#
發(fā)表于 2025-3-22 11:36:22 | 只看該作者
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
6#
發(fā)表于 2025-3-22 16:18:00 | 只看該作者
7#
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,
8#
發(fā)表于 2025-3-23 00:37:05 | 只看該作者
9#
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.
10#
發(fā)表于 2025-3-23 09:28:12 | 只看該作者
 關(guān)于派博傳思  派博傳思旗下網(wǎng)站  友情鏈接
派博傳思介紹 公司地理位置 論文服務(wù)流程 影響因子官網(wǎng) 吾愛(ài)論文網(wǎng) 大講堂 北京大學(xué) Oxford Uni. Harvard Uni.
發(fā)展歷史沿革 期刊點(diǎn)評(píng) 投稿經(jīng)驗(yàn)總結(jié) SCIENCEGARD IMPACTFACTOR 派博系數(shù) 清華大學(xué) Yale Uni. Stanford Uni.
QQ|Archiver|手機(jī)版|小黑屋| 派博傳思國(guó)際 ( 京公網(wǎng)安備110108008328) GMT+8, 2025-10-5 20:16
Copyright © 2001-2015 派博傳思   京公網(wǎng)安備110108008328 版權(quán)所有 All rights reserved
快速回復(fù) 返回頂部 返回列表
垦利县| 武山县| 宁阳县| 汾阳市| 黄冈市| 辽中县| 钟祥市| 永登县| 东乡族自治县| 寿宁县| 嘉善县| 农安县| 拜泉县| 高阳县| 出国| 彰化市| 玉龙| 钟山县| 正阳县| 连云港市| 靖边县| 应城市| 舟曲县| 宝清县| 广汉市| 汶上县| 香港| 上犹县| 石棉县| 宁安市| 云梦县| 夹江县| 肃北| 巨鹿县| 怀安县| 班玛县| 拉孜县| 天津市| 密云县| 惠水县| 郴州市|