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NASA NTRS · 19790052174

The source of electrostatic fluctuations in the solar-wind

Abstract

Solar wind electron and ion distribution functions measured simultaneously with or close to times of intense electrostatic fluctuations are subjected to a linear Vlasov stability analysis. Although all distributions tested were found to be stable, the analysis suggests that the ion beam instability is the most likely source of the fluctuations.

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Lemons, D. S., Asbridge, J. R., Bame, S. J., Feldman, W. C., Gary, S. P., Gosling, J. T.. 1979-05-01. The source of electrostatic fluctuations in the solar-wind. https://ntrs.nasa.gov/citations/19790052174

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