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Magnetic Field Structure and Accelerated Electrons in a Gradual Microwave/Hard X-ray Flare

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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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References

  • Nakajima, H. and Schwarts, R. A. 1995, Ap. J., to be submitted.

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Author information

Authors and Affiliations

  1. Nobeyama Radio Observatory, NAOJ Nobeyama, 384-13, Minamisaku, Nagano, Japan

    H. Nakajima

  2. Laboratory for Astronomy and Solar Physics, NASA/GSFC, 20771, Greenbelt, MD, USA

    R. A. Schwartz

  3. Laboratory for Astronomy and Solar Physics, Hughes STX, 20706, Lanham, MD, USA

    R. A. Schwartz

Authors
  1. H. Nakajima
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  2. R. A. Schwartz
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Editor information

Editors and Affiliations

  1. Science University of Tokyo, Japan

    Yutaka Uchida

  2. National Astronomical Observatory, Tokyo, Japan

    Takeo Kosugi

  3. University of Hawaii, Honolulu, HI, USA

    Hugh S. Hudson

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© 1996 Kluwer Academic Publishers

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Nakajima, H., Schwartz, R.A. (1996). Magnetic Field Structure and Accelerated Electrons in a Gradual Microwave/Hard X-ray Flare. 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_127

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  • DOI: https://doi.org/10.1007/978-94-009-0315-9_127

  • 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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