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Large resistivity in numerical simulations of radially self-similar outflows

Published online by Cambridge University Press:  12 August 2011

Miljenko Čemeljić
Affiliation:
Academia Sinica Institute of Astronomy and Astrophysics and Theoretical Institute for Advanced Research in Astrophysics, P.O. Box 23-141, Taipei, Taiwan email: [email protected]
Nektarios Vlahakis
Affiliation:
IASA and Section of Astrophysics, Astronomy and Mechanics, Department of Physics, University of Atens, Panepistemiopolis 15784, Zografos, Athens, Greece email: [email protected], [email protected]
Kanaris Tsinganos
Affiliation:
IASA and Section of Astrophysics, Astronomy and Mechanics, Department of Physics, University of Atens, Panepistemiopolis 15784, Zografos, Athens, Greece email: [email protected], [email protected]
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Abstract

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We investigate conditions in a radially self-similar outflow in the regime of large resistivity. Using the PLUTO code, we performed simulations with proper choice of boundary conditions, relaxed at the footpoints of critical surfaces in the flow. We investigate outflow propagation in a high-resistive disk corona, and compare it to the results with small or vanishing resistivity.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2011

References

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