The Behavior of Ionospheric Plasma in Topside Equatorial Plasma Structures

Details The Behavior of Ionospheric Plasma in Topside Equatorial Plasma Structures The Behavior of Ionospheric Plasma in Topside Equatorial Plasma Structures

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006agusmsa33a..05v&link_type=abstract

American Geophysical Union, Fall Meeting 2007, abstract #SA33A-05

Physics

2439 Ionospheric Irregularities, 2481 Topside Ionosphere

Scientific paper

The DMSP spacecraft provides a unique view of topside plasma structures by frequently passing through a single depletion spanning a range of magnetic flux tube apex heights within it. This allows us to investigate the relationships between the evolving envelope of the structure and the plasma within it. In this report we describe the results of initial investigations where the angle between the satellite trajectory and plasma depletion allows different regions inside a bubble to be sampled. In particular we examine the relationships between the gradient in the vertical flow inside a bubble and the bubble width in longitude at different magnetic field apex heights.

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