MI-WAVE

Low Noise Amplifiers (LNA)

Overview, specifications and how to request a quote

Mi-Wave · Low Noise Amplifiers

Low Noise Amplifiers (LNA)

Low-noise, high-gain front-end amplification from microwave to millimeter-wave bands

The Mi-Wave 955 series low noise amplifiers (LNAs) are built for sensitive receivers and signal conditioning, covering 1 GHz to 110 GHz across the Ka, Q, U, V, E and W bands. Models offer 10 to 40 dB small-signal gain with a low noise figure, and serve satellite downlinks, millimeter-wave radar front ends, 5G FR2 development platforms and RF test systems. Integrated waveguide ports and regulated bias keep gain flat across the band, so the front end behaves predictably in a crowded spectrum.

Overview

The Mi-Wave 955 series LNAs form a complete millimeter-wave line from 1 GHz to 110 GHz, with models for Ka-band (26.5 to 40 GHz), Q-band (33 to 50 GHz), U-band (40 to 60 GHz), V-band (50 to 75 GHz) and E/W band (60 to 110 GHz). Each model comes with an integrated rectangular waveguide port (WR-28, WR-22, WR-19, WR-15, WR-12 or WR-10 with standard flanges) or, on the wideband versions, a 1.85 mm coaxial connector, for direct mounting at a receiver front end or in a test fixture. The design puts noise figure first while keeping useful large-signal headroom: Psat runs from +10 dBm to +22 dBm by model, enough for satellite downlink chains, radar receivers, point-to-point microwave links and 5G FR2 beamforming systems. All models use regulated bias (+6 V to +15 V by model, most at +6 V or +8 V), specify a maximum RF input, and operate with the case at or below +60 °C. Before ordering, check the noise figure at your band edge, the input power your source can present, and whether the flange is standard or miniature. Custom frequency ranges, gain and interfaces are available.

Low Noise Amplifiers (LNA)

Key specifications

Frequency range1 GHz to 110 GHz (by model; representative model 955UF-30/383: 40 to 60 GHz)
Small-signal gain10 to 40 dB (by model; 955UF-30/383 typical 30 dB)
Noise figure3 to 6 dB (by model; 955UF-30/383 typical 5 dB; the high-power 955WF-20/11.5/387H is 12 dB)
Saturated output power (Psat)+10 dBm to +22 dBm (by model; 955UF-30/383 typical +12 dBm, +15 dBm over the band)
Maximum RF input (CW)0 dBm (955UF-30/383 / 955VF-35/15/385); +5 dBm (955EF-30/15/387)
Bias voltage+6 V to +15 V by model; the 955UF-30/383 is +6 V to +8 V typical (+12 V maximum)
Operating current119 mA typical (955UF-30/383); 129 mA typical (955VF-35/15/385); 204 mA typical (955EF-30/15/387)
RF interfaceRectangular waveguide (WR-28 / WR-22 / WR-19 / WR-15 / WR-12 / WR-10); 1.85 mm coaxial (wideband models)
VSWR2:1 typical (955V-50/68/35/18/385)
Maximum operating temperature (case)Up to +60 °C
Representative models955UF-30/383, 955VF-35/15/385, 955V-50/68/35/18/385, 955EF-30/15/387 (listed as 955EF-30/8/387 in the factory catalogue table), 955WF-30/387, 955-01/60/30/1.85mmF
Custom optionsFrequency range, gain and interface can be built to order

Features

Wide band coverage

The 955 series runs from 1 GHz to 110 GHz, covering Ka, Q, U, V, E and W bands from one line for satellite, radar and millimeter-wave systems.

Low noise figure

Noise figure between 3 and 6 dB on most models, optimized for receiver sensitivity so weak signals keep a usable SNR.

High gain, flat response

Small-signal gain of 10 to 40 dB by model with flat gain across the band gives the mixer, filter or converter behind it a consistent, predictable front end.

Integrated waveguide ports

WR-10 to WR-28 standard waveguide flanges (UG series) and 1.85 mm coaxial versions mount directly in test fixtures or system modules without adapters.

Regulated bias and input limits

Built-in bias regulation at +6 V to +15 V by model (most at +6 V or +8 V), with a specified maximum RF input (0 dBm or +5 dBm by model) to guard against overdrive.

Many uses

Satellite downlink chains (VSAT, SatCom), millimeter-wave radar front ends, 5G FR2 beamforming, point-to-point microwave links and RF test benches, with custom specifications available.

Typical applications

Low noise amplifier (LNA) in satellite downlink reception at ground stations and user terminals

Satellite communications

Satellite downlink reception at ground stations and user terminals

On a Ka/Q/V-band downlink the signal arrives weak after tens of thousands of kilometers of path loss and atmospheric attenuation. The LNA is the first stage of the receive chain and sets the sensitivity that makes the link budget close. Gateway stations, VSAT terminals, LEO/MEO user terminals and airborne SatCom all rely on its low noise figure to keep the satellite signal above the system noise floor before further processing.

Radar and defense

Receive front end for surveillance, tracking radar and electronic detection

In surveillance radar, FMCW ranging radar and electronic reconnaissance receivers, the LNA is the first active device after the antenna feed. Its noise figure sets the system noise temperature of the whole chain, so engineers can extend detection range or sharpen resolution without adding transmit power. At W/E-band the same front ends serve high-resolution imaging radar and short-range sensing, where gain stability over temperature is tightly specified.

Low noise amplifier (LNA) as the receive front end of surveillance and tracking radar and ESM systems
Low noise amplifier (LNA) boosting signals in millimeter-wave system validation and RF test benches

R&D measurement

Signal boosting for millimeter-wave system validation and RF test benches

RF and millimeter-wave labs measuring receiver sensitivity, validating beamforming or MIMO systems, or testing 5G FR2 base station prototypes often need to lift the signal under test into the instrument's range without letting the amplifier's own noise hide the device's behavior. The LNA is built into automated test equipment (ATE) or a bench setup as the instrument-side signal conditioner, so engineers can measure receive chain noise figure (NF) and dynamic range with confidence.

Options and configuration

Choose the band, gain and interface your application needs; we compile the list and carry it into the quote form.

Band and model

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Interface / flange

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