In plasma physics, the Lundquist number (denoted by S {\displaystyle 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
S = L v A η , {\displaystyle S={\frac {Lv_{A}}{\eta }},}
where L {\displaystyle L} is the typical length scale of the system, η {\displaystyle \eta } is the magnetic diffusivity and v A {\displaystyle 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 102–108, while in astrophysical situations the Lundquist number can be greater than 1020. Considerations of Lundquist number are especially important in magnetic reconnection.
See also Magnetic Prandtl number Péclet number Stuart number
References Priest, Eric; Forbes, Terry (2000), Magnetic Reconnection (PDF), Cambridge University Press, ISBN 978-0-521-48179-3
