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Solar Physics

, Volume 142, Issue 2, pp 391–394 | Cite as

Plans for a new radioheliograph in Belgium

  • Pierre Cugnon
  • Roger Gonze
  • Fréderic Clette
Article
  • 27 Downloads

Abstract

The existence of “spikes” with very short time scales (1 to 10 ms) in the decimetric radio spectrum emphasizes the necessity of building radio instruments with very high time resolution. Therefore, we are planning to build a multi-frequency decimetric radioheliograph at the radioastronomical station of the Observatoire Royal de Belgique (Humain, Belgium). The existing array primarily devoted to observe at 408 MHz will constitute the starting structure of the project.

Keywords

Time Resolution Short Time Scale High Time Radio Spectrum High Time Resolution 
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.

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Reference

  1. Delaboudinière, J.-P. et al.: 1989, EIT-Solar corona synoptic observations from SOHO with an Extreme-Ultraviolet Imaging Telescope, in The SOHO Mission, Scientific and Technical Aspects of the instruments, ESA SP-1104.Google Scholar
  2. Gonze, R.: 1973, in the Proceedings of the third meeting of the Committee of European Solar Radio Astronomers - Eds. J. Delannoy and F. Poumeyrol, Bordeaux-Floirac, p. 190.Google Scholar
  3. Gopalswamy, N., 1988: in Basic Plasma Process on the Sun, Proceedings of the IAU Symposium 142, Eds. E. R. Priest and V. Krishnan, Kluwer Academic Publishers, p. 495.Google Scholar
  4. Güdel, M., and Benz, A. O.: 1990, Astron. Astrophys. 231, p. 202.Google Scholar
  5. Hurford, G. J., and Gary, D. E.: 1989, in MAX '91 Workshop #2, Developments in Observations and Theory for Solar Cycle 22, Eds. R.M. Winglee and B.R. Dennis, p. 328.Google Scholar
  6. Mercier, C.: 1990, Solar Phys. 130, p. 119.Google Scholar
  7. Napier, P. J., Thompson, R. A., and Ekers, R.D.: 1983, Proceedings of the IEEE 71, p. 1295.Google Scholar
  8. Nishio, M., Tsukiji, Y., Kobayashi, S., Shibasaki, K., and Enome, S.: 1988, Astron. Astrophys. 198, p. 370.Google Scholar
  9. Pick, M., Klein, K.-L., and Trottet, G.: 1990, Astrophys. J. Suppl. 73, p. 165.Google Scholar
  10. The radioheliograph group: 1989, Solar Physics 120, p. 193.Google Scholar
  11. Raulin, J. P., Willson, R. P., Kerdraon, A., Klein, K.-L., Lang, K. R., and Trottet, G.: 1991, Astron. Astrophys. 251, p. 298.Google Scholar
  12. Zhao, R.-y., Mangeney, A., and Pick, M.: 1991, Astron. Astrophys. 241, p. 183.Google Scholar

Copyright information

© Kluwer Academic Publishers 1992

Authors and Affiliations

  • Pierre Cugnon
    • 1
  • Roger Gonze
    • 1
  • Fréderic Clette
    • 1
  1. 1.Observatoire Royal de BelgiqueBruxellesBelgium

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