Advertisement

Solar Physics

, Volume 86, Issue 1–2, pp 247–252 | Cite as

A flare model deduced from Hinotori and millimeterwave interferometer observations

  • Kin-aki Kawabata
  • Hideo Ogawa
  • Ikuro Suzuki
V. Emission Processes and Source Structure

Abstract

The γ-ray and white-light flare of 13 May, 1981 is used for a study of spatial distributions of energetic electrons and high-temperature plasma.

Keywords

Spatial Distribution Flare Energetic Electron Interferometer Observation Flare Model 
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.

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References

  1. Hiei, E., Takanka, K., Watanabe, T.,and Akita, K.: 1982, Proc.Hinotori Symposium on Solar Flares, Institute of Space and Astronautical Science, Tokyo, p.208.Google Scholar
  2. Kawabata, K., Ogawa, H., Takakura, T., Tsuneta, S., Ohki, K., Yoshimori, M., Okudaira, K., Hirasima, Y.,and Kondoh, I.:1982, Proc. Hinotori Symposium on Solar Flares, Institute of Space and Astronautical Science, Tokyo,p.168.Google Scholar
  3. Nitta,N.,Takakura,T.,Ohki,K.,and Yoshimori,M.:1983,These Proceedings.Google Scholar
  4. Sakurai,T.:1983,These Proceedings.Google Scholar
  5. Takakura, T., Ohki, K., Tsuneta, S., Nitta, N., Makishima, K., Murakami, T., Ogawara, Y., and Oda, M.: 1982, Proc. Hinotori Symposium on Solar Flares, Institute of Space and Astronautical Science, Tokyo, p.142.Google Scholar
  6. Tsuneta,S.,Takakura,T.,Nitta,N.,Ohki,K.,Ogawara,Y.,Murakami,T., Makishima,K., and Oda, M.: 1983,These Proceedings.Google Scholar

Copyright information

© D. Reidel Publishing Co 1983

Authors and Affiliations

  • Kin-aki Kawabata
    • 1
  • Hideo Ogawa
    • 1
  • Ikuro Suzuki
    • 1
  1. 1.Department of Physics and AstrophysicsNagoya UniversityChikusa-ku NagoyaJapan

Personalised recommendations