Abstract
Type III bursts are detected in association with dynamic coronal X-ray jets observed by Yohkoh/SXT. The type III bursts are spatially and temporally coincident with the X-ray jets.
The association of type III bursts with X-ray jets implies the acceleration of electrons to several tens of keV, along with the heating responsible for the production of soft X-rays.
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© 1996 Kluwer Academic Publishers
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Kundu, M.R. et al. (1996). Detection of Nonthermal Radio Emission from Coronal X-ray Jets. In: Uchida, Y., Kosugi, T., Hudson, H.S. (eds) Magnetodynamic Phenomena in the Solar Atmosphere. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0315-9_89
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DOI: https://doi.org/10.1007/978-94-009-0315-9_89
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