The 3115 is a 18 GHz horn antenna from EMCO. Antennas boost signals and can overcome signal losses related to splitters and junctions. Used and refurbished antennas and antenna preamplifiers can save you money while delivering the same high quality as new products.
Additional Features:
Ultra Broadband: 750 MHz - 18 GHz
VSWR (avg): < 1.5:1
Maximum Continuous Power: 300 W
Peak Power: 500 W
Impedance: 50 ohm
Connector Type: N female (precision)
Optimized High Frequency Gain
Low VSWR
Antenna Assembly
Mounting bracket drilled to accept ETS-Lindgren or other tripod mounts with 1/4 in x 20 threads
The Model 3115 sweeps from 750 MHz to 18 GHz without stopping for band breaks, making it ideal for automated testing. It has the widest usable frequency range of any antenna in its class. The Model 3115 uses a Type N precision connector and accepts up to 500 watts of continuous input power. The antenna’s high gain and low VSWR over its operatingfrequency translates into efficient amplifier use and higher field strengths.
The 3115 is a 18 GHz horn antenna from EMCO. Antennas boost signals and can overcome signal losses related to splitters and junctions. Used and refurbished antennas and antenna preamplifiers can save you money while delivering the same high quality as new products.
Additional Features:
- Ultra Broadband: 750 MHz - 18 GHz
- VSWR (avg): < 1.5:1
- Maximum Continuous Power: 300 W
- Peak Power: 500 W
- Impedance: 50 ohm
- Connector Type: N female (precision)
- Optimized High Frequency Gain
- Low VSWR
- Antenna Assembly
- Mounting bracket drilled to accept ETS-Lindgren or other tripod mounts with 1/4 in x 20 threads
The Model 3115 sweeps from 750 MHz to 18 GHz without stopping for band breaks, making it ideal for automated testing. It has the widest usable frequency range of any antenna in its class.
The Model 3115 uses a Type N precision connector and accepts up to 500 watts of continuous input power. The antenna’s high gain and low VSWR over its operatingfrequency translates into efficient amplifier use and higher field strengths.