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BRAMS: The Belgian RAdio Meteor StationsIn the last months, the Belgian Institute for Space Aeronomy has been developing a Belgian network for observing radio meteors using forward scattering technique. This network is called BRAMS for Belgian RAdio Meteor Stations. Two beacons emitting a circularly polarized pure sine wave toward the zenith act as the transmitters at frequencies of 49.97 and 49.99 MHz. The first one located in Dourbes (Southern Belgium) emits a constant power of 150 Watts while the one located in Ieper (Western Belgium) emits a constant power of 50 Watts. The receiving network consists of about 20 stations hosted mainly by radio amateurs. Two stations have crossed-Yagi antennas measuring horizontal and vertical polarizations of the waves reflected off meteor trails. This will enable a detailed analysis of the meteor power profiles from which physical parameters of the meteoroids can be obtained. An interferometer consisting of 5 Yagi-antennas will be installed at the site of Humain in order to determine the angular detection of one reflection point, allowing us to determine meteoroid trajectories. We describe this new meteor observing facility and present the goals we expect to achieve with the network.
Document ID
20110016622
Acquisition Source
Marshall Space Flight Center
Document Type
Conference Paper
Authors
Lamy, H.
(Institut d'Aeronomie Spatiale de Belgique Brussels, Belgium)
Ranvier, S.
(Institut d'Aeronomie Spatiale de Belgique Brussels, Belgium)
De Keyser, J.
(Institut d'Aeronomie Spatiale de Belgique Brussels, Belgium)
Calders, S.
(Institut d'Aeronomie Spatiale de Belgique Brussels, Belgium)
Gamby, E.
(Institut d'Aeronomie Spatiale de Belgique Brussels, Belgium)
Verbeeck, C.
(Royal Observatory Brussels, Belgium)
Date Acquired
August 25, 2013
Publication Date
July 1, 2011
Publication Information
Publication: Meteoroids: The Smallest Solar System Bodies
Subject Category
Space Sciences (General)
Distribution Limits
Public
Copyright
Public Use Permitted.
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