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The Southern Ontario All-sky Meteor Camera Network
Authors:R. J. Weryk  P. G. Brown  A. Domokos  W. N. Edwards  Z. Krzeminski  S. H. Nudds  D. L. Welch
Affiliation:(1) Department of Physics and Astronomy, University of Western Ontario, London, ON, Canada, N6A 3K7;(2) Department of Earth Science, University of Western Ontario, London, ON, Canada, N6A 5B7;(3) Department of Physics and Astronomy, McMaster University, Hamilton, ON, Canada, L8S 4M1
Abstract:We have developed an automated network of all-sky CCD video systems to detect medium–large meteoroids ablating over Southern Ontario, Canada. The system currently consists of five stations with the largest baseline being 180 km. Each site runs a video rate recorder with sufficient resolution to determine meteoroid trajectories with a typical precision of about 300 m but no worse than 1 km. The sensitivity of the camera is close to a stellar visual magnitude of +1 which allows for astrometric calibrations using field stars. Photometric procedures have also been developed and tested. The system has a limiting magnitude for meteors of about −2 with the current detection algorithm.
Keywords:Meteors  All-sky  Detection  Real-time
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