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As RMG beacons are put into
service, information will be entered here to provide details.
Freq.
(MHz)
+/- 10KHz
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Locator
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Pwr
(W)
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Antenna
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Elevation
Gnd ASL / Ant AGL
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Callsign
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Status
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903.100
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EM00xh
Austin area
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0.2
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tri-delta loop 6dBi omni
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1350' / 22'
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"K5RMG"
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active
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903.106
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DM80nv
Ft Stockton
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3+
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9.9dBi uda twd East
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3000' / 60'
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"NN5DX"
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active
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1296.250*
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EL09qp
San Antonio
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3(-)
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tri-delta loop 6dBi omni
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updating
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inactive
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1296.360
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EL07wu
Alice, TX area
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2
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tri-delta loop 6dBi omni
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234' / 90'
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"K5DYY"
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active
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1296.900
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EM00xh
Austin area
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2.4
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tri-delta loop 6dBi omni
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1350' / 22'
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"K5RMG"
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inactive
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2304.045
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EM00xh
Austin area
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1.5
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tri-delta loop 6dBi omni
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1350' / 22'
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"K5RMG"
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inactive
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2304.250
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EL09pq
San Antonio
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1.1
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tri-delta loop 6dBi omni
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1440' / 35'
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updating
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inactive
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3456.240
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EM00xh
Austin area
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0.2
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tri-delta loop 6dBi omni
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1350' / 22'
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"K5RMG"
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inactive
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5760.175
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EM00xh
Austin area
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0.2
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tri-delta loop 6dBi omni
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1350' / 22'
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"K5RMG"
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inactive
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10368.180
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EM00xh
Austin area
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1.2
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180 deg horn pointed E
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1350' / 22'
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"K5RMG"
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inactive
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*This beacon is very temperature sensitive.
When cold, it has been heard as high as 1296.290; when hot, it has been heard as low as 1296.222.
The San Antonio beacons are being reprogrammed with K5HY callsign since N5GO is SK. We are looking
for a suitable location at which to install these beacons in the San Atnonio area.
Most of the Austin area beacons are down for upgrade and reinstallation. They will be restored to operation
as quickly as possible.
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The following are links to sites
showing lists of beacons on frequencies above 222MHz. Some sites are for areas outside of
CONUS, but the goal here is to become a "clearing house" for information regarding Amateur
Radio Microwave Operations. New links will be added as they are discovered. Use your browser
"Back" button to return to this page.
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The following are links to
sites showing lists to propagation information. Much of the information is directed, for
the greater part, toward much lower frequencies than those on which we focus here, but there
may be some correllations to be identified between some of these factors and propagation above
900 MHz! Use browser "Back" button to return to this page.
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