Magnetic launching and collimation of jets from the disc–magnetosphere boundary: 2.5D MHD simulations
Article first published online: 23 JAN 2012
© 2012 The Authors Monthly Notices of the Royal Astronomical Society © 2012 RAS
Monthly Notices of the Royal Astronomical Society
Volume 420, Issue 3, pages 2020–2033, March 2012
How to Cite
Lii, P., Romanova, M. and Lovelace, R. (2012), Magnetic launching and collimation of jets from the disc–magnetosphere boundary: 2.5D MHD simulations. Monthly Notices of the Royal Astronomical Society, 420: 2020–2033. doi: 10.1111/j.1365-2966.2011.20133.x
- Issue published online: 16 FEB 2012
- Article first published online: 23 JAN 2012
- Accepted 2011 November 3. Received 2011 November 2; in original form 2011 April 20
Animation. The animation shows the reference simulation between t = 300 and 900, during which the jet is launched and collimated. The top panel shows the poloidal matter flux and magnetic flux contours in the entire simulation region. The bottom three panels show the poloidal matter flux, current and kinetic plasma parameter β1 near the star. An animation of the full simulation is available at http://astro.cornell.edu/~pslii/research.htm.
|MNR_20133_sm_animation.zip||13142K||Supporting info item|
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