標題: Titlebook: Coronal Mass Ejections; H. Kunow,N. U. Crooker,R. Steiger Book 2006 Springer-Verlag New York 2006 Corona.Heliosphere.Planet.Solar System.S [打印本頁] 作者: FERAL 時間: 2025-3-21 19:33
書目名稱Coronal Mass Ejections影響因子(影響力)
書目名稱Coronal Mass Ejections影響因子(影響力)學科排名
書目名稱Coronal Mass Ejections網(wǎng)絡公開度
書目名稱Coronal Mass Ejections網(wǎng)絡公開度學科排名
書目名稱Coronal Mass Ejections被引頻次
書目名稱Coronal Mass Ejections被引頻次學科排名
書目名稱Coronal Mass Ejections年度引用
書目名稱Coronal Mass Ejections年度引用學科排名
書目名稱Coronal Mass Ejections讀者反饋
書目名稱Coronal Mass Ejections讀者反饋學科排名
作者: arboretum 時間: 2025-3-21 21:21
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.作者: 慷慨援助 時間: 2025-3-22 03:23
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.作者: 聯(lián)合 時間: 2025-3-22 07:50
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.作者: Catheter 時間: 2025-3-22 12:36 作者: guardianship 時間: 2025-3-22 16:08
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.作者: guardianship 時間: 2025-3-22 20:29
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.作者: 令人不快 時間: 2025-3-22 23:57 作者: 種族被根除 時間: 2025-3-23 03:17
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.作者: 忍耐 時間: 2025-3-23 07:24
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.作者: 鑲嵌細工 時間: 2025-3-23 13:00 作者: sundowning 時間: 2025-3-23 16:36
CME Disturbance Forecasting,the 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.作者: In-Situ 時間: 2025-3-23 20:49
Garden Chemicals and Their Application,r understanding of ICMEs is far from complete and formulate several challenges that, if addressed, would substantially improve our knowledge of the relationship between CMEs at the Sun and in the heliosphere.作者: Cardioversion 時間: 2025-3-24 00:45 作者: 遷移 時間: 2025-3-24 05:28
Spectral Analysis of Wave Motion,es occurring as the ICMEs propagate out through the inner heliosphere, interacting with the ambient solar wind. The solar and . observations are discussed as are efforts to model the evolution of ICMEs from the Sun out to 1 AU.作者: 踉蹌 時間: 2025-3-24 07:50 作者: 使更活躍 時間: 2025-3-24 14:08 作者: 狂怒 時間: 2025-3-24 16:38 作者: delusion 時間: 2025-3-24 19:47
ICMEs in the Outer Heliosphere and at High Latitudes: an Introduction,ction regions (MIRs) which dominate the structure of the outer heliosphere at solar maximum. The distribution of high-latitude ICMEs is solar cycle dependent. A few overexpanding ICMEs are observed at high-latitude near solar minimum. Near solar maximum ICMEs are observed at all latitudes, but those above 40? do not have high charge states.作者: Cultivate 時間: 2025-3-25 02:37 作者: 完整 時間: 2025-3-25 04:33
Coronal Observations of CMEs,f shock waves are seen, but the location of these shocks relative to the other structures and the occurrence rate at the heights where Solar Energetic Particles are produced remains controversial. The relationships among CMEs, Moreton waves, EIT waves, and EUV dimming are also cloudy. The close conn作者: microscopic 時間: 2025-3-25 11:33
CME Theory and Models,ey physical processes involved. The other is primarily numerical and illustrates the complexity of possible interactions between the CME and the ambient medium. The section on flux rope fitting reviews the accuracy and reliability of various methods. The section on shock formation considers the effe作者: 托運 時間: 2025-3-25 13:30 作者: 不如樂死去 時間: 2025-3-25 18:14 作者: Vaginismus 時間: 2025-3-25 23:11 作者: Pander 時間: 2025-3-26 03:43 作者: HARP 時間: 2025-3-26 04:46 作者: Mhc-Molecule 時間: 2025-3-26 10:07 作者: granite 時間: 2025-3-26 13:58
Wave Propagation in Structures,rona sustains the stresses that allow the magnetic energy to build up and how, later on, this magnetic energy is released during eruptive flares and CMEs. Multiwavelength observations have confirmed that reconnection plays a key role during the development of CMEs. Frequently, CMEs display a rather 作者: 話 時間: 2025-3-26 18:16
Plant Diseases and Their Pathogens,ture depressions, and magnetic clouds at the Voyager and Pioneer spacecraft have begun to provide comparable information regarding the behavior of ICMEs at extremely large heliocentric distances. At the same time, advances in modeling have provided new insights into the dynamics and evolution of ICM作者: 閃光東本 時間: 2025-3-27 00:41
Book 2006.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作者: diabetes 時間: 2025-3-27 05:11 作者: nonsensical 時間: 2025-3-27 05:55 作者: 違法事實 時間: 2025-3-27 12:56
An Introduction to CMEs and Energetic Particles,ss ejections. This paper reviews the status of our understanding of the ways in which particles are energised at the Sun in association with CMEs. This understanding will remain incomplete until the relationship between CMEs and flares is determined and we know the topology of the associated magneti作者: COMMA 時間: 2025-3-27 14:29
An Introduction to Theory and Models of CMEs, Shocks, and Solar Energetic Particles,nergetic particle (SEP) acceleration, and shock propagation. A brief review of the history of CME models demonstrates steady progress toward an understanding of CME initiation, but it is clear that the question of what initiates CMEs has still not been solved. For illustration, we focus on the flux 作者: 懲罰 時間: 2025-3-27 20:40 作者: anniversary 時間: 2025-3-27 22:22 作者: 含鐵 時間: 2025-3-28 03:11
ICMEs in the Outer Heliosphere and at High Latitudes: an Introduction,on of ICMEs out to large distances and ICME properties at high latitudes. The internal pressure of ICMEs initially exceeds the ambient solar wind pressure and causes the ICMEs to expand in radial width to about 15 AU. Large ICMEs and series of ICMEs compress the leading plasma and form merged intera作者: 燕麥 時間: 2025-3-28 10:01
Coronal Observations of CMEs,E morphology, velocity, acceleration and mass. Flares associated with CMEs are observed in X-rays, and several different radio signatures are also seen. Optical and UV spectra of CMEs both on the disk and at the limb provide velocities along the line of sight and diagnostics for temperature, density作者: voluble 時間: 2025-3-28 13:51 作者: 值得贊賞 時間: 2025-3-28 15:55 作者: Isthmus 時間: 2025-3-28 19:54 作者: 認識 時間: 2025-3-29 02:20 作者: Metastasis 時間: 2025-3-29 06:53
Multi-Wavelength Observations of CMEs and Associated Phenomena,avelength analysis. The combination of data obtained from space-based experiments and ground based instruments allows us to follow the space-time development of an event from the bottom of the corona to large distances in the interplanetary medium. Since CMEs originate in the low solar corona, under作者: 引導 時間: 2025-3-29 07:51 作者: echnic 時間: 2025-3-29 13:46
ICMEs at High Latitudes and in the Outer Heliosphere,on, and morphology of the solar wind, particularly during times of high solar activity. They are known to play an important role in cosmic ray modulation and the acceleration of energetic particles. ICMEs are also believed to be associated with the large global transient events that swept through th作者: 鞠躬 時間: 2025-3-29 18:47
CME Disturbance Forecasting,ely different in the sheath than within the ICME. Consequently two types of forecast procedures using solar observations of phenomena associated with the release of the CME as input parameters have been developed to treat the two types of environment. This chapter surveys efforts that have resulted 作者: 疏忽 時間: 2025-3-29 22:17 作者: 慷慨不好 時間: 2025-3-30 01:01
https://doi.org/10.1007/978-0-387-45088-9Corona; Heliosphere; Planet; Solar System; Solar wind; coronal mass ejection; instruments; solar; space plas作者: AUGUR 時間: 2025-3-30 06:52
978-1-4419-2356-1Springer-Verlag New York 2006作者: scotoma 時間: 2025-3-30 11:33 作者: 火花 時間: 2025-3-30 13:29
Water with One Simple Solute Particle,he CME process, the variability of these signatures and questions about mapping to observed CME features raise issues that remain on the cutting edge of ICME research. These issues are discussed in the context of traditional understanding, and recent results using innovative analysis techniques are reviewed.作者: frivolous 時間: 2025-3-30 17:55 作者: 過份 時間: 2025-3-30 23:06 作者: scoliosis 時間: 2025-3-31 03:50
Roaming Between Wireless ATM Lans,ss ejections. This paper reviews the status of our understanding of the ways in which particles are energised at the Sun in association with CMEs. This understanding will remain incomplete until the relationship between CMEs and flares is determined and we know the topology of the associated magneti作者: 指耕作 時間: 2025-3-31 06:10
Plant Diseases and Their Pathogens,nergetic particle (SEP) acceleration, and shock propagation. A brief review of the history of CME models demonstrates steady progress toward an understanding of CME initiation, but it is clear that the question of what initiates CMEs has still not been solved. For illustration, we focus on the flux 作者: Irrepressible 時間: 2025-3-31 09:17
Don H. Rasmussen,Alan P. MacKenziepted that the energy required to power a CME is contained in the pre-eruption coronal magnetic field, the pre-CME state of that field and the conditions leading up to the release of the magnetic energy are still not entirely clear. Recent studies point to various phenomena which are common to many, 作者: 廣口瓶 時間: 2025-3-31 15:30 作者: 嘲笑 時間: 2025-3-31 21:09 作者: AGGER 時間: 2025-4-1 01:21 作者: FOIL 時間: 2025-4-1 02:19
Water with One Simple Solute Particle,he CME process, the variability of these signatures and questions about mapping to observed CME features raise issues that remain on the cutting edge of ICME research. These issues are discussed in the context of traditional understanding, and recent results using innovative analysis techniques are 作者: 衣服 時間: 2025-4-1 07:29
Market Exchange and Optimality,articles, and the acceleration and propagation processes at the Sun and in interplanetary space. Furthermore, energetic particles provide information on the development and structure of coronal mass ejections as they propagate from the solar corona into the interplanetary medium. In this paper we re
