WR-28 Standard Gain Horn Antennas | 25 dBi Gain

26.5 – 40 GHz

Description:

Mi-Wave’s Ka-Band Horn Antennas | WR-28 | 26.5 – 40 GHz are created with the end consumer in mind. We know you need and demand the absolute best when it comes to ka-band horn antennas and look to provide you with the best solutions possible. Some of the highlights of our ka-band horn antennas are:

Features

• Nominal Gain of 25 dB

• Available from 12.4 to 500 GHz

• Made with precise dimensional tolerance control

• Gain calibration is accurate to 0.5 dB over full waveguide bandwidth

Applications

• Low F/D Antennas

• Surveillance Systems

• Offset Feed Antenna

*All data presented is collected from a sample lot.
* Actual data may vary unit to unit, slightly.
*All testing was performed under +25 °C case temperature.
*Consult factory to confirm if material, plating, size, shape, orientation and any electrical parameter is critical for the application as website information is for reference only.
*Millimeter Wave Products, Inc. reserves the right to change the information presented on website without notice as we continue to enhance the performance and design of our products.

Ka-Band Horn Antennas | WR-28 | 26.5 – 40 GHz

If you are looking for  ka-band standard gain horn antennas, then you’ve come to the right place. At Millimeter wave products Inc. (Mi-Wave) we specialize in manufacturing the highest quality standard gain horn antennas for many needs.

What makes our standard gain horns the preferred choice?

Mi-Wave’s 261 ka-band Series standard gain horn antennas are fabricated with very close tolerances to ensure the precision of every horn manufactured by Mi-Wave. Each unit is joined to a short section of rectangular wave-guide and terminated in a standard flange. This is critical when you need the best quality millimeter wave products all doing their part in your application.

Frequently Asked Questions for standard gain horn antennas.

The gain increases with frequency, which is typical for aperture antennas. However, the curve shows saturation at higher frequencies.

This is due to the decrease of the aperture efficiency, which is a result of an increased phase difference in the field distribution at the aperture.

Hence with formula when we see 0.5 degree change but practically it is not at higher frequency. Aperture efficiency of pyramidal horn is 0.511.

The data for the standard gain horns is provided in far field.