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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Isthmus

認(rèn)識

Metastasis

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

引導(dǎo)

echnic

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

鞠躬

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

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https://doi.org/10.1007/978-0-387-45088-9Corona; Heliosphere; Planet; Solar System; Solar wind; coronal mass ejection; instruments; solar; space plas

AUGUR

978-1-4419-2356-1Springer-Verlag New York 2006