Magnetic Draping and the Source Region for the Outer Heliospheric Radio Emissions

Details Magnetic Draping and the Source Region for the Outer Heliospheric Radio Emissions Magnetic Draping and the Source Region for the Outer Heliospheric Radio Emissions

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aipc..719..381c&link_type=abstract

PHYSICS OF THE OUTER HELIOSPHERE. AIP Conference Proceedings, Volume 719, pp. 381-386 (2004).

Physics

3

Particle Emission, Solar Wind, Solar Wind Plasma, Sources Of Solar Wind, Radio, Microwave

Scientific paper

Magnetic draping is an important element of the Priming/GMIR theory for the 2-3 kHz outer heliospheric radiation observed by the Voyager spacecraft. More detailed consideration of draping leads to the qualitative prediction that the source region should be a linear band on the sky that includes the direction to the heliopause nose and is aligned with the magnetic field B. This is consistent with the observed source locus, supporting the theory and suggesting that the plane-of-sky component of B in the outer heliosheath is parallel to the galactic plane.

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