Helium abundance and dynamics in different types of solar wind streams: The Prognoz 7 observations

Journal of Geophysical Research: Space Physics

Volumn 102, Issue A2, 1997, Pages 2125-2136

  Yermolaev, Yuri I ^a   Stupin, Vitaly V ^a  

^a Russian Academy of Sciences   (Russian Federation)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 37149036548     PISSN: 01480227     EISSN: None     Source Type: Journal    
DOI: 10.1029/96JA01635     Document Type: Article

References (4)

1. Asbridge, J. R., S. J. Bame, W. C. Feldman, and M. D. Montgomery, Helium and hydrogen velocity differences in the solar wind, J. Geophys. Res.,81 (16), 2719, 1976.
2. Avanov, L., N. Borodkova, Z. Nemecek, A. Omeltchenko, J. Safrankova, A. Skalski, Y. Yermolaev, and G. Zastenker, Some features of solar wind protons, a particles and heavy ions behaviour: the Prognoz 7 and Prognoz 8 experimental results, Czechoslovak J. Phys.,37 (6), 759, 1987.
3. Bame, S. J., J. R. Asbridge, W. C. Feldman, and J. T. Gosling, Evidence for a structure-free state at high solar wind speeds, J. Geophys. Res.,82 (10), 1487, 1977.
4. Bochsler, P., Minor ions - tracers for physical processes in the heliosphere, in Proceedings of Solar Wind Seven Conference, COSPAR Colloquia, vol.3, edited by E. Marsch and R. Schwenn, p. 323, Pergamon, Tarrytown, N. Y., 1992.