Titlebook: Coronal Physics from Radio and Space Observations; Proceedings of the C Gérard Trottet Conference proceedings 1997 Springer-Verlag Berlin H

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Observations of the 3D distributions of thermal to near-relativistic electrons in the interplanetar observed at 1 AU are found to have power-law spectra often extending down to ?1 keV, implying a source region at 0.2-1. . altitude. At solar quiet times, a nonthermal, “super-halo” component extending from ～2 to ?10. keV is found to be always present. For impulsive events which produce solar type I

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Coronal and interplanetary particle beams,leration in the solar corona and in interplanetary space. We start our discussion of coronal beams with a standard flare scenario, established on recent X-ray (.) and radio observations, which constitutes a framework for the understanding of upward and downward accelerated electron beams and their s

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Coronal mass ejections and type II radio bursts,vers of type II burst emitting super-Alfvénic disturbances. The paper focuses on the available experimental evidence for this assumption. For instance, the apparent contradiction is discussed between measured speeds of potential shock drivers and their observed type II burst association. Further, se

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