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Ion Acoustic Waves in the Heliosphere

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The 3-D Heliosphere at Solar Maximum

Abstract

Observations of ion acoustic waves in the solar wind during the first and second orbit of the Ulysses spacecraft are presented. The observations show variations of the wave activity with the heliolatitude and with the phase of the solar cycle. The interrelationships between the wave intensity and the electron heat flux and the ratio of electron to proton temperature, T e /T p , are examined.

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References

  • Gary, S. P.: 1978, `Ion-Acoustic-Like Instabilities in the Solar Wind’, J. Geophys. Res. 83, 2504.

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  • Lin, N. etal.: 2001, `Ion Acoustic Waves and Their Source Regions in the Solar Wind’, J. Geophys. Res.,submitted.

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© 2001 Springer Science+Business Media Dordrecht

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Lin, N., Kellogg, P.J., MacDowall, R.J., Gary, S.P. (2001). Ion Acoustic Waves in the Heliosphere. In: Marsden, R.G. (eds) The 3-D Heliosphere at Solar Maximum. Springer, Dordrecht. https://doi.org/10.1007/978-94-017-3230-7_29

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  • DOI: https://doi.org/10.1007/978-94-017-3230-7_29

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-90-481-5723-5

  • Online ISBN: 978-94-017-3230-7

  • eBook Packages: Springer Book Archive

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