Loading [MathJax]/jax/output/HTML-CSS/jax.js

ART

In plasma physics, the Lundquist number (denoted by S) is a dimensionless ratio which compares the timescale of an Alfvén wave crossing to the timescale of resistive diffusion. It is a special case of the magnetic Reynolds number when the Alfvén velocity is the typical velocity scale of the system, and is given by

{\displaystyle S={\frac {Lv_{A}}{\eta }},}

where L is the typical length scale of the system, \eta is the magnetic diffusivity and v_{A} is the Alfvén velocity of the plasma.

High Lundquist numbers indicate highly conducting plasmas, while low Lundquist numbers indicate more resistive plasmas. Laboratory plasma experiments typically have Lundquist numbers between {\displaystyle 10^{2}-10^{8}} , while in astrophysical situations the Lundquist number can be greater than 10^{{20}} . Considerations of Lundquist number are especially important in magnetic reconnection.
See also

Magnetic Reynolds number

References
Priest, Eric; Forbes, Terry (2000), Magnetic Reconnection (PDF), Cambridge University Press, ISBN 978-0-521-48179-3

Physics Encyclopedia

World

Index

Hellenica World - Scientific Library

Retrieved from "http://en.wikipedia.org/"
All text is available under the terms of the GNU Free Documentation License