Welcome to the British Columbia Meteor Network

The British Columbia Meteor Network and its associate members are dedicated volunteers who have worked together to advance knowledge of meteor science. Some of our members are professionals although most are devoted amateurs.

The network is comprised of a video detection component as well as a radio detection component. We  share our data with multinational governments and astronomy groups.

Data collection is only one goal of the the network. We also hope to promote a strong educational program in open cooperation with the school districts and community colleges of British Columbia.

Feel free to browse our site. Likewise, feel free to contact us if you have any questions or would like to know more.

British Columbia Meteor Network Coverage Map



Click here to see the full resolution map.

For a brief history of how the network got started please read Ed’s article.


ABMO Radio Page

ABMO Radio Page

Latest radio meteor echoes from W Kelowna, B.C.

Highest none shower counts are at local sunrise and the lowest are at sunset.


The observatory is located in West Kelowna and it uses the forward scatter technique of meteor echo detection. The receiver is tuned to TV channel 4’s video carrier frequency (negative offset) at 64.240 MHz. The echoes are from the video carriers of the two station listed below:


Station QTH Bearing km kW
CITL-TV Lloydminster, AB 56 770 130
CBKT-1 Moose Jaw, SK 81 975 100


When a meteor has the proper geometry between the transmitting TV station and the receiving station an echo is produced as the receiver as the signal is reflected off the ionized plasma produce while the meteor ablates in the earth’s upper atmosphere. The ionization usually occurs between 110 down to 60 km up, thus giving a radio coverage out to about 1400 km radius of the receiver.

The station consist of an Icom PCR-1000 to a seven element log periodic antenna. The antenna is installed in the attic and pointing 70 degrees or towards the northeast. A fifty foot piece of RG-58 coax connects the antenna to the receiver. No pre-amps are used. The PCR-1000 is a software controlled receiver; a small black box with only an on and off switch on the front.



In the back of the PCR-1000 are:

BNC Antenna connector, a ground post, DC Input, Audio Out, a RS-238 connector for communication with the computer, and a special 9600 bps audio filtering bypass for high speed digital packet radio used on amateur built satellites (AMSAT).

Pin outs of the ICOM PCR-1000



























During the major showers the observatory employs several different programs on several different computers on the LAN. Audio is split off the PCR-1000 as seen above (Y-adapter audio out) and shared among the computers during the showers. Alternatively, I use a second receiver, the ICOM R-8500 that runs in parallel with the PCR-1000 but on a different frequency, and run the audio from it to separate computer for real time analysis.

If a shower is predicted to show once in a lifetime activity I will also run an ICOM IC-746 transceiver. I usually devote the IC-746 to listening to 40.530 MHz, the US SNOTEL meteor system. SNOTEL has two master stations (transmitters) located in Utah and in Idaho which put in strong meteor burst signals into BC.

R8500 bottom and IC-746 middle HF homemade transceiver on top


The software does the actual detection, counting, data filing and display work.  Software in use includes Spectrum Lab, mAnalyzer, HROfft, all capable Windows programs. Watch for a software discussion in the Radio   Detection Basics in the Radio Methods section of the site. In addition to the above programs the observatory runs Janalyzer and a self written code. Which program is used is dependent on the subject understudy or nature of the shower.

Note: I do run the above programs on both Windows XP and on Linux machines. To see how I run it on a Linux machine please go to the RMOB site and read the article. Janalyzer is written in Java so is cross platform ready.

I set my software to output data at ten minute periods and on the hour. Depending on what software is running, duration for each 10 minute and hourly interval is recorded along with signal strengths in several bins of approximately 10 dB, 20 dB, 30 dB, and greater than 30 dB. Total time in seconds per period for each power level is also recorded.

A FFT spectrogram for each five minute period is ftp to an external site as well as saved on a local hard drive for study later or for the correlation with video fireballs

To be continued…