Radial Variation of Magnetic Flux Ropes: Case Studies with ACE and NEAR

Details Radial Variation of Magnetic Flux Ropes: Case Studies with ACE and NEAR Radial Variation of Magnetic Flux Ropes: Case Studies with ACE and NEAR

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aipc..679..121r&link_type=abstract

SOLAR WIND TEN: Proceedings of the Tenth International Solar Wind Conference. AIP Conference Proceedings, Volume 679, pp. 121-1

Physics

2

Particle Emission, Solar Wind, Interplanetary Magnetic Fields

Scientific paper

Multiple spacecraft observations are used to examine the spatial variation of magnetic flux ropes in the interplanetary medium near 1 AU. When the observing spacecraft are close and radially aligned they observe nearly the same structure. When they are radially aligned and far apart they reveal the expansion of the ropes with heliocentric distance. When the spacecraft are azimuthally separated and the separation vector is along the rope axis, this axis is shown to be bent. The observed radial expansion is consistent with earlier Helios results.

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