Physical mechanisms for turbulent dissipation in collisionless shock waves |
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Authors: | C S Wu |
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Institution: | (1) Lehrstuhl für Theoretische Astrophysik der Universität Tübingen, F.R.G. |
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Abstract: | Temporal and spectral characteristics of solar hard X-ray bursts are briefly reviewed. The merits of non-thermal and thermal flare models are discussed. The validity of these models may be checked by future measurements of X-ray polarization. Finally, some important results of recent satellite experiments are described providing information on the spatial distribution of hard X-ray sources: the multi-spacecraft observation of X-ray bursts and the imaging of X-ray sources by means of the HXIS instrument.Paper presented at the IX-th Lindau Workshop The Source Region of the Solar Wind . |
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