The Latitudinal Distribution of Solar Wind Magnetic Holes
Using the fast latitude scan period of the Ulysses spacecraft, the occurrence of magnetic holes in the solar wind is investigated from -80 degrees to +80 degrees helio-latitude.
Engineering topics
Publications and source records attributed to Tsurutani, B..
Using the fast latitude scan period of the Ulysses spacecraft, the occurrence of magnetic holes in the solar wind is investigated from -80 degrees to +80 degrees helio-latitude.
The interplanetary solar wind depletion (SWD) event of 26 April 1999 and its magnetospheric consequences are examined. The SWD event is characterized by a solar wind density decrease from [similar to] 3.0 to 0.7 cm(sup -3) leading to a solar wind ram pressure decrease from [similar to] 2.0 to 0.2 nPa. This SWD onset is followed by a dipolarization of nightside magnetospheric fields.
We show evidence for mirror mode structures at comet Giacobini-Zinner.
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Energetic ***sup3***He particle mean free paths are calculated using in-situ wave amplitudes. The wave polarization and wave k directions are included in a first order cyclotron resonant calculation.
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Explore the source record for details and available documents.
Explore the source record for details and available documents.
Explore the source record for details and available documents.
Ulysses recently completed a second slow latitude scan of the northern heliosphere, a descent from 80.2 degrees North in July 1995 to the solar equator in December 1997.
Nonlinear evolution equation for Alfven waves, propagating in streaming plasmas with nonuniform densities and inhomogeneous magnetic fields, is obtained by using the reductive perturbation technique.
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One of the oldest mysteries in geomagnetism is the linkage between solar and geomagnetic activity.