Anisotropic YBCO film resistivity data of Iye et al. [Physica C 166 (1
990) 62] have been analyzed in terms of conventional flux-flow and pha
se-slip resistivities. Iye et al. systematically varied the angle thet
a of the magnetic field relative to the c-axis for a number of fields
ranging from 0.3 to 5 T. It is shown that the data exhibit no evidence
for conventional Bardeen-Stephen flux-flow; the data are interpreted
using an expression for anisotropic phase-slip resistivity. The phenom
enological expression for the resistivity given by Tinkham has been ex
tended to include the dependence on the polar angle theta; the phase-s
lip resistivity varies approximately as o(ps)(H,T,theta)=rho(n)/[I0(ga
mma(H,T,theta)/2)]2. Although the mass anisotropy parameter GAMMA=5.3
(the ratio H(c2)(theta=pi/2)/(H(c2)(theta=0)), for low fields, the dat
a for the ratio rho(H parallel-to c)/p(H perpendicular-to c) is as lar
ge as 160 and the field and angular dependent resistivity does not sca
le with H/H(c2)(theta); the variation is easily accommodated by the pr
oposed model.