The Formation of Magnetic Decreases \(MDs\) in Interplanetary Space: Ulysses

Details The Formation of Magnetic Decreases \(MDs\) in Interplanetary Space: Ulysses The Formation of Magnetic Decreases \(MDs\) in Interplanetary Space: Ulysses

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007agufmsh31b..04t&link_type=abstract

American Geophysical Union, Fall Meeting 2007, abstract #SH31B-04

Physics

2102 Corotating Streams, 2134 Interplanetary Magnetic Fields, 2159 Plasma Waves And Turbulence

Scientific paper

Magnetic Decreases are decreases in the magnitude of the ambient magnetic field. The displaced plasma pressure is supplanted by anisotropic \(Tperp/Tpar > 1\), locally heated plasma so that there is pressure balance across the MD structures. Anisotropic spatial distributions of MDs are identified to further understand the conditions under which MDs form/evolve. We will show that Ulysses fast-latitude scans through corotating solar wind streams are good places to search for such spatial anisotropies. The properties of MDs within CIRs and high speed streams will be reported. A general generation mechanism will be described.

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