Why Is Reconnection in the Solar Wind so Different than in Other Environments?

Details Why Is Reconnection in the Solar Wind so Different than in Other Environments? Why Is Reconnection in the Solar Wind so Different than in Other Environments?

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1302..198k&link_type=abstract

PICKUP IONS THROUGHOUT THE HELIOSPHERE AND BEYOND: Proceedings of the 9th Annual International Astrophysics Conference. AIP Con

Astronomy and Astrophysics

Astrophysics

Solar Wind, Magnetic Field Effects, Spacecraft, Magnetohydrodynamics, Particle Emission, Solar Wind, Magnetic Reconnection, Spacecraft/Atmosphere Interactions, Magnetohydrodynamics And Plasmas

Scientific paper

Studies of reconnection in the solar wind led by Gosling and collaborators have revealed surprising results that are posing serious challenges to current theoretical understanding of the reconnection process. These include presence of prolonged quasi-steady reconnection, low magnetic shear angles, and no substantial particle acceleration. Here we put forth the conjecture that many of the solar wind exhaust events may be fossil sites. We explore the viability of this possibility using full particle simulations.

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