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

Goldstein, B. E.; Neugebauer, M.; Smith, E. J.

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