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Nonthermal Emissions In The Hard X-Ray And Microwave Ranges From Flaring Loops

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Magnetodynamic Phenomena in the Solar Atmosphere
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Abstract

We have studied a flare (GOES class: M2.3) on the west limb (H- alpha: N18, W78) on 1993 March 23 using microwave (17GHz) and Soft X-ray imaging data and also hard X-ray spectrum data. This flare has typical properties of “gradual-hard flares”.

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© 1996 Kluwer Academic Publishers

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Yaji, K., Kosugi, T., Nishio, M. (1996). Nonthermal Emissions In The Hard X-Ray And Microwave Ranges From Flaring Loops. 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_130

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  • DOI: https://doi.org/10.1007/978-94-009-0315-9_130

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-6627-3

  • Online ISBN: 978-94-009-0315-9

  • eBook Packages: Springer Book Archive

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