Quasi-thermal noise in a drifting plasma: Theory and application to solar wind diagnostic on Ulysses

Journal of Geophysical Research: Space Physics

Volumn 104, Issue A4, 1999, Pages 6691-6704

  Issautier, Karine ^a  

^a OBSERVATOIRE DE PARIS   (France)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0001749162     PISSN: None     EISSN: 21699402     Source Type: Journal    
DOI: None     Document Type: Article

References (5)

1. Bame, S. J., et al., The Ulysses solar wind plasma experiment, Astron. Astrophys. Suppl. Ser., 92, 237, 1992.
2. Chateau, Y. F., and N. Meyer-Vernet, Electrostatic noise in non-Maxwellian plasmas: Generic properties and "kappa" distributions, J. Geophys. Res., 96, 5825, 1991.
3. Couturier, P., S. Hoang, N. Meyer-Vernet, and J.-L. Steinberg, Measurements and interpretation of the quasi-thermal noise spectrum in the solar wind: Solar Wind Five, NASA Conf. Publ., CP-2280, 377, 1983.
4. Feldman, W. C., J. R. Asbridge, S. J. Bame, M. D. Montgomery, and S. P. Gary, Solar wind electrons, J. Geophys. Res., 80, 4181, 1975.
5. Feldman, W. C., B. L. Barraclough, J. L. Phillips, and Y.-M. Wang, Constraints on high-speed solar wind structure near coronal base: A Ulysses perspective, Astron. Astrophys., 316, 355, 1996.