Three-Dimensional Velocity Structure of the Polar Wind

Details Three-Dimensional Velocity Structure of the Polar Wind Three-Dimensional Velocity Structure of the Polar Wind

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agufmsa32a0672d&link_type=abstract

American Geophysical Union, Fall Meeting 2001, abstract #SA32A-0672

Physics

2431 Ionosphere/Magnetosphere Interactions (2736), 2447 Modeling And Forecasting, 2475 Polar Cap Ionosphere

Scientific paper

A time-dependent, global, fluid model has been used to study the three-dimensional velocity structure of the polar wind for a variety of geophysical conditions. In particular, variations in the thermal plasma flow have been examined for a full range of solar-cycle, seasonal, and geomagnetic conditions. Regions of upflow and downflow have been charted for both the H+ and O+ components of the polar wind, including regions where these populations undergo counterstreaming. The theoretical results of this investigation have been compared with the findings of several relevant experimental studies.

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