  The mass ranges of meteors, imaged by electro-optical (EO) cameras and
backscatter radar receivers, for the most part do not overlap. Typical EO
systems detect meteoroid masses down to 10$^{-5}$ kg or roughly magnitude +2
meteors when using moderate field of view optics, un-intensified optical
components, and meteor entry velocities around 45 km/sec. This is near the high
end of the mass range of typical meteor radar observations. Having the same
mass meteor measured by different sensor wavelength bands would be a benefit in
terms of calibrating mass estimations for both EO and radar. To that end, the
University of Western Ontario (UWO) has acquired and deployed a very low light
imaging system based on an electron-multiplying CCD camera technology. This
embeds a very low noise, per pixel intensifier chip in a cooled camera setup
with various options for frame rate, region of interest and binning. The EO
system of optics and sensor was optimally configured to collect 32 frames per
second in a square field of view 14.7 degrees on a side, achieving a
single-frame stellar limiting magnitude of m$_G$ = +10.5. The system typically
observes meteors of +6.5. A key development in this pipeline has been the first
true application of matched filter processing to process the faintest meteors
possible in the EMCCD system while also yielding high quality automated metric
measurements of meteor focal plane positions. With pairs of EMCCD systems
deployed at two sites, triangulation and high accuracy orbits are one of the
many products being generated by this system. These measurements will be
coupled to observations from the Canadian Meteor Orbit Radar (CMOR) used for
meteor plasma characterization and the Canadian Automated Meteor Observatory
(CAMO) high resolution mirror tracking system.
