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Titlebook: Coronal Mass Ejections; H. Kunow,N. U. Crooker,R. Steiger Book 2006 Springer-Verlag New York 2006 Corona.Heliosphere.Planet.Solar System.S

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发表于 2025-3-21 19:33:05 | 显示全部楼层 |阅读模式
书目名称Coronal Mass Ejections
编辑H. Kunow,N. U. Crooker,R. Steiger
视频videohttp://file.papertrans.cn/239/238295/238295.mp4
概述The Solar and Heliospheric Observatory SOHO has revolutionized our knowledge of the generation, development and effects of coronal mass ejections (CMEs) and interplanetary CMEs (ICMEs). This book is t
丛书名称Space Sciences Series of ISSI
图书封面Titlebook: Coronal Mass Ejections;  H. Kunow,N. U. Crooker,R. Steiger Book 2006 Springer-Verlag New York 2006 Corona.Heliosphere.Planet.Solar System.S
描述.It is well known, that the Sun as central star of our solar system gravitationally controls the orbits of planets and minor bodies. Much less known is the domain of plasma fields and charged particles, however, in which the Sun with a radius of less than 0.7 Million km governs the heliosphere out to about 15 Billion km, a distance about 20 000 times larger in radius or nearly 10.13 .times bigger in volume. What forces activates the Sun to maintain this power? Coronal Mass Ejections (CMEs) and their descendants are the troops serving the Sun during high solar activity periods. ..This volume offers a comprehensive and integrated overview of our present knowledge and understanding of Coronal Mass Ejections (CMEs) and their descendants, Interplanetary CMEs (ICMEs). It results from a series of workshops held between 2000 and 2004. An international team of about sixty experimenters involved e.g. in the SOHO, ULYSSES, VOYAGER, PIONEER, HELIOS, WIND, IMP, and ACE missions, ground observers, and theoreticians worked jointly on interpreting the observations and developing new models for CME initiations, development, and interplanetary propagation...The book is intended to provide scientists
出版日期Book 2006
关键词Corona; Heliosphere; Planet; Solar System; Solar wind; coronal mass ejection; instruments; solar; space plas
版次1
doihttps://doi.org/10.1007/978-0-387-45088-9
isbn_softcover978-1-4419-2356-1
isbn_ebook978-0-387-45088-9Series ISSN 1385-7525
issn_series 1385-7525
copyrightSpringer-Verlag New York 2006
The information of publication is updating

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发表于 2025-3-21 21:21:05 | 显示全部楼层
Roaming Between Wireless ATM Lans,s understanding will remain incomplete until the relationship between CMEs and flares is determined and we know the topology of the associated magnetic fields. The paper also discusses the characteristics of interplanetary CMEs that may be probed using particle observations.
发表于 2025-3-22 03:23:43 | 显示全部楼层
Market Exchange and Optimality,on the development and structure of coronal mass ejections as they propagate from the solar corona into the interplanetary medium. In this paper we review the measurements of energetic particles in interplanetary space and discuss their implication for our understanding of the sources, and of acceleration and propagation processes.
发表于 2025-3-22 07:50:25 | 显示全部楼层
https://doi.org/10.1007/978-1-4615-8681-4the release of the CME as input parameters have been developed to treat the two types of environment. This chapter surveys efforts that have resulted in implementable (at least in principle) forecast algorithms for sheath and ICME disturbances and discusses uncertainties associated with both.
发表于 2025-3-22 12:36:55 | 显示全部楼层
发表于 2025-3-22 16:08:07 | 显示全部楼层
Plant Diseases and Their Pathogens,ent at the evolving CME-driven coronal/interplanetary shock and the origin of “impulsive” SEP events at flare sites of magnetic reconnection below CMEs. We argue that future developments in models require focused study of “campaign events” to best utilize the wealth of available CME and SEP observations.
发表于 2025-3-22 20:29:51 | 显示全部楼层
Wireless ATM Handover Protocol Design,ructure, and can compress the ambient solar wind, depending upon their relative speed. Their magnetic fields may reconnect with solar wind fields or those of other ICMEs with which they interact, creating complicated signatures in spacecraft data.
发表于 2025-3-22 23:57:40 | 显示全部楼层
发表于 2025-3-23 03:17:22 | 显示全部楼层
Solar Imprint on ICMEs, Their Magnetic Connectivity, and Heliospheric Evolution,ructure, and can compress the ambient solar wind, depending upon their relative speed. Their magnetic fields may reconnect with solar wind fields or those of other ICMEs with which they interact, creating complicated signatures in spacecraft data.
发表于 2025-3-23 07:24:02 | 显示全部楼层
An Introduction to CMEs and Energetic Particles,s understanding will remain incomplete until the relationship between CMEs and flares is determined and we know the topology of the associated magnetic fields. The paper also discusses the characteristics of interplanetary CMEs that may be probed using particle observations.
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