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CORRELATIONS OF PLASMA DENSITY AND MAGNETIC FIELD STRENGTH IN THE HELIOSHEATH

Author(s)
Gutynska, O.; Šafránková, J.; Němeček, Z.; Richardson, John D.
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Abstract
The crossing of the termination shock (TS) by Voyager 2 in 2007 at 84 AU allows a comparison of fluctuations in different heliosheath regions. The Letter concentrates on MHD waves that exhibit a significant correlation between the magnetic field strength and plasma density. The correlations between both quantities were computed on 2?hr time intervals in the frequency range of 1 × 10[superscript -4] to 4 × 10[superscript -3] Hz. We separate the data into two regions with different magnetic field behavior; the post-TS region with many crossings of the current sheet and the unipolar region where the magnetic field direction remains nearly constant. We find that typical correlation coefficients in these regions are about 0.55-0.65, larger than in Earth's magnetosheath. The largest correlations occur when the spectrum of magnetic field fluctuations is dominated by low frequencies.
Date issued
2010-10
URI
http://hdl.handle.net/1721.1/95817
Department
MIT Kavli Institute for Astrophysics and Space Research
Journal
Astrophysical Journal. Letters
Publisher
IOP Publishing
Citation
Gutynska, O., J. Šafránková, Z. Němeček, and J. D. Richardson. “CORRELATIONS OF PLASMA DENSITY AND MAGNETIC FIELD STRENGTH IN THE HELIOSHEATH.” The Astrophysical Journal 722, no. 2 (October 5, 2010): L228–L232. © 2010 The American Astronomical Society
Version: Final published version
ISSN
2041-8205
2041-8213

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