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We present Ulysses Unified Radio and Plasma Wave (URAP) observations of ion-acoustic waves associated with magnetic clouds and ejecta. The peak intensities of these waves, which usually occur inside CMEs when T
e/T
i≫1, are not correlated with heliocentric distance or electron to ion temperature ratio inside the CMEs.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
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