Simulation of turbulent magnetic reconnection in the small-scale solar wind.

Details Simulation of turbulent magnetic reconnection in the small-scale solar wind. Simulation of turbulent magnetic reconnection in the small-scale solar wind.

Jun 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000sccha..43..629w&link_type=abstract

Science in China, Series A, Vol. 43, No. 6, p. 629 - 637

Computer Science

2

Solar Wind: Magnetic Reconnection

Scientific paper

Some observational examples for the possible occurrence of the turbulent magnetic reconnection in the solar wind are found by analysing Hellos spacecraft's high resolution data. The phenomena of turbulent magnetic reconnections in small scale solar wind are simulated by introducing a third order accuracy upwind compact difference scheme to the compressible two-dimensional MHD flow. Numerical results verify that the turbulent magnetic reconnection process could occur in small scale interplanetary solar wind, which is a basic feature characterizing the magnetic reconnection in high-magnetic Reynolds number solar wind.

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