Abstract
Through the analysis of data returned from the three Rice Suprathermal Ion Detectors we have obtained information on the particle regimes present in the geomagnetic tail at lunar distances. We are able to distinguish the existence of two distinct particle populations and to quantify many of their spatial and plasma characteristics.
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© 1976 D. Reidel Publishing Company, Dordrecht-Holland
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Hardy, D.A., Freeman, J.W., Hills, H.K. (1976). Plasma Observations in the Magnetotail. In: McCormac, B.M. (eds) Magnetospheric Particles and Fields. Astrophysics and Space Science Library, vol 58. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-1503-5_9
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DOI: https://doi.org/10.1007/978-94-010-1503-5_9
Publisher Name: Springer, Dordrecht
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