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M2 Antennas 222-10EZ 222 MHz Yagi Antennas are used by operators who want more than a basic beam antenna. Featuring a balanced, top-of-the-line feeder matching system, these 10 element antennas handle full legal limit and deliver weak-signal or distant repeater and simplex performance that is far beyond the capabilities of small end-mount beams or base station verticals.
M2 Antennas 222-10EZ are, as their name implies, easily assembled. Built on very easy to handle and turn 10 ft. booms, these medium-sized, computer designed Yagis cover 222 to 226 MHz with flat gain and low SWR. Strong, yet lightweight and streamlined, they complement any VHF system. The heart of each 222-10EZ is their unique Driven Element Module, offering a balanced feeder for excellent pattern. Superior weather resistance and power handling abilities are achieved with all connectors that are O-ring sealed to the CNC machined block and internal connections are sealed in a space-age silicone gel with a dielectric strength nearly 4 times greater than air. The coaxial cable balun connectors are triple sealed. Other key mechanical and electrical parts are CNC machined from 6061-T6 aluminum and all hardware except the U-bolts is stainless steel.
These balanced feeder beams are suitable for operations into distant FM repeaters or on simplex when mounted vertically, as shown, on a fiberglass mast. For weak-signal work on SSB, CW and digital modes, this beam may be mounted horizontally on a metal mast. In either case, since M2 Antennas 222-10EZ 222 MHz Yagi Antennas have very clean patterns, they are perfect for stacking vertically or horizontally, to bring your 1.25 meter band operations to a new level. Get all of your VHF/UHF antenna system components right here at DX Engineering.
Yagi, 222 MHz, 10 el., 9 ft. 9 in. Boom, 14.1 dBi, 23 dB F/B, T-match, 1.5 kW, N female, Each
Part Number: MSQ-22210EZ
Availability: In Stock
Estimated Ship Date: Today
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The part MSQ-22210EZ has an additional shipping charge of $8.00 per item due to its large size and/or weight.