Image intensified video detection systems were used to observe the 199
1 Perseid meteor shower from two locations in eastern Canada. In 29.6
hours of total observing time a total of 668 meteors were detected, of
which 403 were Perseids. We derived a profile of TVZHR (television ze
nithal hourly rate) values for the 1991 Perseid shower over the solar
longitude (epoch 2000) interval 138 degrees 51' to 141 degrees 01'. Th
e apparent limiting stellar magnitudes of the observing systems were 9.4 and +8.8 (corresponding to limiting meteor magnitudes for our geom
etry ranging from +8.7 to +7.0). Within the observing period, the maxi
mum TVZHR rate was approximately 1600, and occurred at solar longitude
139.9 degrees. This is in good agreement with the second peak observe
d by visual observers. The data suggest that TVZHR values should be di
vided by a factor of approximately 5 to compare TVZHR and ZHR values.