Breakthrough Broadband Power Solution: 2-6GHz/100W/±1.5dB Amplifier
In the fields of high-speed communications and precision testing, the flatness and stability of wideband RF power amplifiers directly determine the upper limit of system performance. Mars RF's newly launched MM2060P50B gallium nitride (GaN) power amplifier module, with its core advantage of industry-leading ±1.5dB gain flatness, provides a 100W-class, highly reliable power solution for applications in the 2-6 GHz band, redefining the standard for wideband amplification.
Core Technology Breakthroughs
*Ultra-Flat Gain Characteristics: Achieves a typical power gain fluctuation of ±1.5dB across the entire 2-6 GHz band, significantly outperforming traditional solutions (typically >±3dB).
*100W Stable Output: Based on third-generation GaN-on-SiC material, it continuously guarantees ≥100W saturated output power at rated operating temperature.
*Intelligent Monitoring Architecture: Forward and reverse power detection and RS422 serial interface. RS422 serial interface includes: ENABLE (Switching On/Off Time); CURRENT SENSE, TEMP SENSE, VOLTAGE SENSE, FORWARD SENSE, REVERSE SENSE, CURRENT ALARM, TEMP ALARM, VOLTAGE ALARM, VSWR ALARM
Typical Application Scenarios
- Test and Measurement: 5G terminal/base station testers, vector signal source driver amplifiers
-Communication Infrastructure: Microwave backhaul systems, multi-band combiner preamplifiers
- Defense Electronics: Electronic countermeasure jammers, phased array radar T/R modules
- Satellite Communications: High-linearity power amplifier chains for L/S-band ground stations
Upgrade your RF front-end now
➤ Get the full product brochure
➤ Request an engineering prototype and customized cooling solution.
Please contact:
Phone:+86-28-87882380
Mob./WhatsApp:+86 18113158334
E-mail: info@marsrf.com
Reshaping power boundaries with GaN technology and delivering on performance promises through precision engineering—the MM2060P50B provides a cornerstone amplification platform for next-generation broadband systems.



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