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Role of Plasma Instabilities in Auroral Phenomena
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  • Letter
  • Published: 01 March 1965

Role of Plasma Instabilities in Auroral Phenomena

  • BRUNO COPPI1 na1 

Nature volume 205, page 998 (1965)Cite this article

  • 328 Accesses

  • 6 Citations

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Abstract

RECENTLY it was proposed that plasma instabilities are responsible for the auroral precipitation of particles trapped inside the magnetosphere1. The entire event would be a two-step process, one which takes particles inside the magnetosphere and one which dumps the trapped particles. Responsible for the second step would be plasma micro-instabilities of the type outlined by Krall and Rosenbluth2.

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References

  1. Chamberlain, J. W., J. Geophys. Res., 68, 5667 (1963).

    Article  ADS  Google Scholar 

  2. Krall, N., and Rosenbluth, M. N., Phys. Fluids, 6, 254 (1963).

    Article  ADS  MathSciNet  Google Scholar 

  3. Wentworth, R. (personal communication).

  4. Rosenbluth, M. N., in Report CLM–M21, 26 (Culham, 1963).

  5. Stix, T. H., Report Matt–219 (Princeton University, 1964).

  6. Coppi, B., Physics Letters, 11, 226 (1964); 12, 213 (1964).

    Article  ADS  MathSciNet  Google Scholar 

  7. Coppi, B., Report M.L. 1278 (Stanford University, 1964).

  8. Anderson, K. A., and Milton, D. W., Report UCB–64/5 (University California, Berkeley, 1964).

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Author information

Author notes
  1. BRUNO COPPI: On leave of absence at the University of California, San Diego, La Jolla.

Authors and Affiliations

  1. Institute for Plasma Research, Stanford University, Stanford, California

    BRUNO COPPI

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  1. BRUNO COPPI
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COPPI, B. Role of Plasma Instabilities in Auroral Phenomena. Nature 205, 998 (1965). https://doi.org/10.1038/205998a0

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  • Published: 01 March 1965

  • Issue date: 06 March 1965

  • DOI: https://doi.org/10.1038/205998a0

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