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Frequency response of magnetic flux sheaths
Authors:P Venkatakrishnan
Institution:(1) The Astronomical Institute at Utrecht, Utrecht, The Netherlands
Abstract:We suggest to identify the elementary flare bursts with the excitation of the small kernels that occur in flare loops that are observed in soft X-ray pictures of flares. We stress the need of simultaneous observations of spatial structure and time variations of hard X-ray bursts sources in various wavelength regions.
Keywords:
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