Published July 22, 2005
| Submitted + Published
Journal Article
Open
Dynamic and Stagnating Plasma Flow Leading to Magnetic-Flux-Tube Collimation
- Creators
- You, S.
- Yun, G. S.
- Bellan, P. M.
Abstract
Highly collimated, plasma-filled magnetic-flux tubes are frequently observed on galactic, stellar, and laboratory scales. We propose that a single, universal magnetohydrodynamic pumping process explains why such collimated, plasma-filled magnetic-flux tubes are ubiquitous. Experimental evidence from carefully diagnosed laboratory simulations of astrophysical jets confirms this assertion and is reported here. The magnetohydrodynamic process pumps plasma into a magnetic-flux tube and the stagnation of the resulting flow causes this flux tube to become collimated.
Additional Information
© 2005 The American Physical Society. (Received 6 February 2005; published 22 July 2005) This work was supported by the U.S. DoE and NSF.Attached Files
Published - YOUprl05.pdf
Submitted - 0506221.pdf
Files
YOUprl05.pdf
Files
(1.3 MB)
Name | Size | Download all |
---|---|---|
md5:1de97e351e1d6dd9a7d57f1b0d3b81bd
|
527.3 kB | Preview Download |
md5:81c86849a8a1874e18f9d28016d20b38
|
810.4 kB | Preview Download |
Additional details
- Eprint ID
- 7372
- Resolver ID
- CaltechAUTHORS:YOUprl05
- Department of Energy (DOE)
- NSF
- Created
-
2007-02-06Created from EPrint's datestamp field
- Updated
-
2021-11-08Created from EPrint's last_modified field