Multi-satellite Observations of Magnetic Holes in the Solar Wind

Details Multi-satellite Observations of Magnetic Holes in the Solar Wind Multi-satellite Observations of Magnetic Holes in the Solar Wind

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004agufmsh12a..04s&link_type=abstract

American Geophysical Union, Fall Meeting 2004, abstract #SH12A-04

Physics

2134 Interplanetary Magnetic Fields, 2149 Mhd Waves And Turbulence, 2164 Solar Wind Plasma, 0639 Nonlinear Electromagnetics, 0689 Wave Propagation (4275)

Scientific paper

A record of magnetic holes observed by the WIND satellite in the solar wind from 1994 to 2004 was recently compiled. When permitted by the relative positions of the two satellites, ACE observed many of the same magnetic holes. By comparing the shape and plasma parameters at each satellite, the geometry and propagation of the holes are constained. The coherence of each hole and the associated pressure balance also help us to distinguish the sources of magnetic holes in the ecliptic and discern possible MHD solitons.

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