Cj. Lamb, MAGNETIC INSTABILITY IN A RAPIDLY ROTATING CYLINDRICAL ANNULUS WITH AFINITELY CONDUCTING INNER-CORE, Geophysical and astrophysical fluid dynamics, 75(2-4), 1994, pp. 227-250
We consider the stability of a toroidal magnetic field B = B(s)phi (w
here(s,phi,z*) are cylindrical polar coordinates) in a cylindrical an
nulus of conducting fluid with inner and outer radii s(i) and s(o) rot
ating rapidly about its axis. The outer boundary is taken to be either
insulating or perfectly conducting, and the effect of a finite magnet
ic diffusivity in the inner core is investigated. The ratio of magneti
c diffusivity in the inner core to that of the outer core is denoted b
y eta; eta --> 0 corresponding to a perfectly conducting inner core an
d eta --> infinity to an insulating one. Comparisons with the results
of Fearn (1983b, 1988) were made and a good match found in the limits
eta --> 0 and eta --> infinity with his perfectly conducting and insul
ating results, respectively. In addition a new mode of instability was
found in the eta --> 0 regime. Features of this new mode are low freq
uency (both the frequency and growth rate --> 0 as eta --> 0) and pene
tration deep into the inner core. Typically it is unstable at lower ma
gnetic field strengths than the previously known instabilities.