The linear stability of a Harris current sheet is examined using the Vlasov
description for both ions and electrons. Orbit integrals are treated numer
ically using the exact particle orbits and including the global structure o
f the perturbation inside the integral. Both electromagnetic and electrosta
tic contributions to the field perturbation are retained and the eigenvalue
problem for the system of integro-differential equations is solved using a
Hermite expansion of the eigenfunction. For the tearing mode, results are
in excellent agreement with established theory. For the recently discovered
kink mode, results are consistent with kinetic simulations at low mass rat
io m(i)/m(e) less than or equal to 16. However, in the limit of realistic e
lectron mass, the growth rate of the kink mode is substantially reduced in
contrast to results from kinetic simulations. It is demonstrated that a bac
kground population may dramatically alter the growth rate of the kink mode
at realistic values of the mass ratio. This result may have relevance to th
e stability of the Earth's geomagnetic tail. (C) 1999 American Institute of
Physics. [S1070-664X(99)02404-0].