Foreshock Langmuir waves for unusually constant solar wind conditions: Data and implications for foreshock structure

Journal of Geophysical Research: Space Physics

Volumn 102, Issue A11, 1997, Pages 24249-24264

  Cairns, Iver H ^a   Robinson, P A ^b   Anderson, Roger R ^a   Strangeway, R J ^c  

^a UNIVERSITY OF IOWA   (United States)

^b UNIVERSITY OF SYDNEY   (Australia)

^c UNIVERSITY OF CALIFORNIA   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 37149028189     PISSN: 01480227     EISSN: None     Source Type: Journal    
DOI: 10.1029/97JA02168     Document Type: Article

References (5)

1. Anderson, R. R., G. K. Parks, T. E. Eastman, D. A. Gurnett, and L. A. Frank, Plasma waves associated with energetic particles streaming into the solar wind from the Earth's bow shock, J. Geophys. Res., 86, 4493, 1981.
2. Bale, S. D., D. Burgess, P. J. Kellogg, K. Goetz, R. L. Howard, and S. J. Monson, Phase coupling in Langmuir wave packets: Possible evidence of three-wave interactions in the upstream solar wind, Geophys. Res. Lett., 23, 109, 1996.
3. Bale, S. D., D. Burgess, P. J. Kellogg, K. Goetz, and S. J. Monson, On the amplitude of intense Langmuir waves in the terrestrial electron foreshock, J. Geophys. Res., 102, 11,281, 1997.
4. Spreiter, J. R., A. L. Summers, and A. Y. Alksne, Hydromagnetic flow around the magnetosphere, Planet. Space Sci., 14, 223, 1966.
5. Strangeway, R. J., and G. K. Crawford, Comparison of upstream phenomena at Venus and Earth, Adv. Space Res., 16(4), 125, 1995.