Physics – Plasma Physics
Scientific paper
Dec 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011agufmsh43a1926y&link_type=abstract
American Geophysical Union, Fall Meeting 2011, abstract #SH43A-1926
Physics
Plasma Physics
[7526] Solar Physics, Astrophysics, And Astronomy / Magnetic Reconnection, [7835] Space Plasma Physics / Magnetic Reconnection, [7863] Space Plasma Physics / Turbulence
Scientific paper
Magnetic reconnection is viewed from the interaction between the large-scale inhomogeneous structure and turbulence. On the one hand, turbulence determines large-scale structures through the turbulent transport coefficients. On the other hand, large-scale inhomogeneous structure determines the statistical properties of turbulence through the production rates of turbulent quantities. In the context of magnetic reconnection, this mutual interaction between the large-scale structures and turbulence is modeled with special emphasis on the pseudo-scalar effects, which represents some symmetry breakage in turbulence. In addition to the magnetic reconnection, magnetic-flux freezing in turbulence media, turbulent dynamo, transport suppression are also discussed.
Hoshino Masahiro
Yokoi Naoto
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