Abstract
The EGD plasma experiment, launched on board of the ISEE-2 spacecraft, is briefly described. Preliminary results concerning three bow shock crossings occurred in November 1977 are discussed. Our attention is focused on some non-thermal features of the distribution function of proton velocities: in particular, we discuss double peaked structures of solar wind spectra and flows of particles backstreaming from the bow shock.
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© 1979 D. Reidel Publishing Co., Dordrecht, Holland, and Boston, U.S.A.
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Bavassano-Cattaneo, M.B. et al. (1979). Preliminary Results from the Solar Wind Experiment on the ISEE-2 Satellite. In: Knott, K., Durney, A., Ogilvie, K. (eds) Advances in Magnetosperic Physics with GEOS-1 and ISEE. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-9527-7_35
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DOI: https://doi.org/10.1007/978-94-009-9527-7_35
Publisher Name: Springer, Dordrecht
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