Low-Noise MMIC Amplifiers for 120 to 180 GHz
NASA’s Jet Propulsion Laboratory
Thursday, October 01 2009
Potential applications include radar, communications, radiometry, and millimeter-wave imaging.

Figure 1. This MMIC contains three InP amplifier stages plus coplanar waveguide transmission lines for input and output impedance matching and DC biasing.
Three-stage monolithic millimeter-wave
integrated-circuit (MMIC) amplifiers
capable of providing useful
amounts of gain over the frequency
range from 120 to 180 GHz have been
developed as prototype low-noise
amplifiers (LNAs) to be incorporated
into instruments for sensing cosmic
microwave background radiation.
There are also potential uses for such
LNAs in electronic test equipment,
passive millimeter-wave imaging systems,
radar receivers, communication
receivers, and systems for detecting
hidden weapons. The main advantage
afforded by these MMIC LNAs, relative
to prior MMIC LNAs, is that their coverage
of the 120-to-180-GHz frequency band makes them suitable for reuse in
a wider variety of applications without
need to redesign them. Each of these
MMIC amplifiers includes InP transistors
and coplanar waveguide circuitry
on a 50-μm-thick chip (see Figure 1).
Coplanar waveguide transmission lines
are used for both applying DC bias and
matching of input and output impedances
of each transistor stage. Via
holes are incorporated between top
and bottom ground planes to suppress
propagation of electromagnetic
modes in the substrate.

Figure 2. The Measured Gain of an amplifier like that shown in Figure 1 was found to exceed 10 dB over most of the frequency range from 120 to 180 GHz. The discontinuity in the plot at 140 GHz is an artifact of switching, at that frequency, between two waveguide bands of the instrumentation used to measure the gain.
On the basis of computational
simulations, each of these
amplifiers was expected to
operate with a small-signal gain
of 14 dB and a noise figure of
4.3 dB. At the time of writing
this article, measurements of
noise figures had not been
reported, but on-chip measurements
had shown gains
approaching their simulated
values (see Figure 2).
This work was done by David
Pukala, Lorene Samoska, and
Alejandro Peralta of Caltech and
Brian Bayuk, Ron Grundbacher,
Patricia Oliver, Abdullah Cavus, and
Po-Hsin Liu of Northrop Grumman
Corporation for NASA’s Jet Propulsion
Laboratory. NPO-42783
This Brief includes a Technical Support Package (TSP).
Low-Noise MMIC Amplifiers for 120 to 180 GHz (reference NPO-42783) is currently available for download from the TSP library.
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This Brief includes a Technical Support Package (TSP).
Low-Noise MMIC Amplifiers for 120 to 180 GHz (reference NPO-42783) is currently available for download from the TSP library.
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