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 |
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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 |