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Alfv鮠Waves, Alpha Particles, and Pickup Ions in the Solar Wind

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dc.contributor.author Goldstein, B. E. en_US
dc.contributor.author Neugebauer, M. en_US
dc.contributor.author Smith, E. J. en_US
dc.date.accessioned 2004-09-30T05:18:22Z
dc.date.available 2004-09-30T05:18:22Z
dc.date.issued 1996-06-26 en_US
dc.identifier.citation Dana Point, California en_US
dc.identifier.clearanceno 96-0698 en_US
dc.identifier.uri http://hdl.handle.net/2014/25050
dc.description.abstract The alpha particles at high latitudes are traveling significantly faster than the effective wave speed, unlike the in-ecliptic situation and the discrepancy between effective wave speed and the Alfv鮠speed calculated with all known corrections is also larger than in the ecliptic. en_US
dc.format.extent 79204 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other amplitude of velocity fluctuations amplitude of field fluctuations anisotropy of the plasma Ulysses plasma and magnetic field experiments en_US
dc.title Alfv鮠Waves, Alpha Particles, and Pickup Ions in the Solar Wind en_US


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