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

  • K. Yaji
  • T. Kosugi
  • M. Nishio

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”.

Keywords

Circular Polarization Energetic Electron Microwave Source Solar Activity Maximum Nonthermal Emission 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

References

  1. Kosugi, T. et al. (1991) Solar Phys., 136, 17Google Scholar
  2. Kundu, M. et aI. (1984) Adv. Space Res., 4, No.7,157Google Scholar
  3. Nakajima, H. et aI. (1991) in Flare Physics in Solar Activity Maximum, 22, 77Google Scholar
  4. Nakajima, H. et aI. (1994) Pmc. IEEE, 82,705Google Scholar

Copyright information

© Kluwer Academic Publishers 1996

Authors and Affiliations

  • K. Yaji
    • 1
  • T. Kosugi
    • 1
    • 2
  • M. Nishio
    • 1
  1. 1.National Astronomical ObservatoryMitaka 181Japan
  2. 2.Nobeyama Radio ObservatoryNAOJapan

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