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Collimation of Magnetically Driven Outflows from Accretion Disks

Published online by Cambridge University Press:  25 May 2016

T. Kudoh ,
R. Matsumoto  and
K. Shibata
T. Kudoh
Affiliation:
Solar Physics Division, National Astronomical Observatory, Mitaka, Tokyo 181-8588, Japan
R. Matsumoto
Affiliation:
Department of Physics, Faculty of Science, Chiba University, Inageku, Chiba 263-8522, Japan
K. Shibata
Affiliation:
Kwasan and Hida Observatories, Kyoto University, Yamashina, Kyoto 607-8471, Japan

Abstract

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We performed 2.5-dimensional, nonsteady MHD numerical simulations to investigate the acceleration and collimation of magnetically driven outflows from accretion disks, including the accretion process itself, consistently. As an initial condition, we used a paraboloidal magnetic field line that is produced by electric current on the equatorial plane. We found that the outflow ejected from the accretion disk is collimated by the pinch effect of the toroidal component of the magnetic field that is produced by the rotation of the disk.

Information

Type
Part II: Posters
Information
Symposium - International Astronomical Union , Volume 195: Highly Energetic Physical Processes and Mechanisms , 2000 , pp. 407 - 408
Copyright
Copyright © Astronomical Society of the Pacific 2000 

References

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