We present a simple and systematic method to calculate Rindler noise, which
is relevant to an analysis of the Unruh effect, by using the fluctuation-d
issipation theorem. To do this, we calculate the dissipative coefficient ex
plicitly from the equations of motion of the: detector and the field. This
method gives not only the correct answer but also a hint as to the origin o
f the apparent statistics inversion effect. Moreover, this method is genera
lized to the Dirac field by using the fermionic fluctuation-dissipation the
orem. We can thus confirm that the fermionic fluctuation-dissipation theore
m is working properly. [S0556-2821(99)00518-4].