Monolithic (MMIC) and discrete transistor (MIC) low noise amplifiers are compared on the basis of performance, cost, and reliability. The need for cryogenic LNA’s for future large microwave arrays for radio astronomy is briefly discussed and data is presented on a prototype LNA for the 1 to 10 GHz range along with a very wideband LNA for the 1 to 60 GHz range. A table of MMIC LNA and mixer designs under development for the frequencies up to 210 GHz is reported and data on cryogenic amplifiers in the 85 to 115 GHz is reviewed. The current status of the topics of transconductance fluctuations and cryogenic noise modeling will be briefly summarized

Erickson, N.

Fernandez, J.E.

Gaier, T.

Weinreb, S.

Wielgus, J.

English

AMS Acta

CRYOGENIC MMIC LOW NOISE AMPLIFIERSS. Weinreb1,  T. Gaier1,  J. E. Fernandez1, N. Erickson2, and J. Wielgus21Jet Propulsion Laboratory, California Institute of Technology, sander.weinreb@jpl.nasa.gov2Department of Physics and Astronomy, U. of Massachusetts,  neal@fcrao1.phast.umass.eduABSTRACTMonolithic (MMIC) and discrete transistor (MIC) low noise amplifiers are compared on the basis of performance,cost, and reliability.  The need for cryogenic LNA’s for future large microwave arrays for  radio astronomy is brieflydiscussed  and  data is presented on a prototype LNA for  the  1 to 10 GHz range  along with a  very wideband LNA forthe 1 to 60 GHz range. A table of MMIC LNA and mixer designs under development  for the frequencies  up to 210 GHzis reported and data on cryogenic amplifiers in the 85 to 115 GHz is reviewed.   The current status of the topics oftransconductance fluctuations and cryogenic noise modeling will be briefly summarized. MMIC VS MIC COMPARISONAs a starting point it is  instructive to compare the advantages and disadvantages of monolithic microwave integratedcircuit   (MMIC) low noise amplifiers with microwave integrated circuit (MIC) amplifiers constructed with discretechip transistors and passive microstrip circuit boards.   A summary of this comparison on the basis of performance,frequency range, cost, and reliability follows.Transistor Performance  - The discrete transistors used in the MIC case are manufactured in the same manner as thetransistors built into the MMIC amplifier and to a large extent this leads to the same expected performance.  Twoexceptions can be argued.  In the MIC case,  transistors can be selected to give the lowest noise; however the MMIC'scan also be selected. To some extent the  cryogenic low noise performance is correlated between different discretetransistors or MMIC's on a  single wafer.  With of the order of 100,000 discrete transistors or 1000 MMIC's on a wafer,a larger number of cryogenic amplifiers can be built from one "golden" wafer.  However, the need for very largenumbers of  cryogenic amplifiers has not  yet  occurred and could be met by processing a large number of wafers andselecting the best.Passive Circuit Performance  -  A wider variety of passive circuit element values and quality factors are available to theMIC designer.  However, in most cases the loss in a cryogenic  passive circuit  is negligible and  a MMIC can use anexternal element such as an input inductor if it is necessary.   It is possible to make shorter connections on a MMICparticularly  the  transistor source ground and this can help bandwidth and stability.Frequency Range - The short connections possible with a MMIC become an important factor above 100 GHz.  MMICamplifiers with high gain at 215 GHz have been reported [1] but  has not been achieved with MIC amplifiers.Multistage MMIC amplifiers operating below 500 MHz have difficulty with achieving sufficiently large coupling andbypass  capacitors.  DC coupling may be feasible in some cases but this restriction does not occur with MIC amplifiersutilizing multi-plate layer, high-dielectric constant capacitors.Cost – The development cost of a MMIC varies between $50K and $500K dependant upon  the processing  cost forsmall mounts of wafer space for experimental circuits, the difficulty of the specifications, and the legacy  of similardesigns.  The experimental processing cost is minimized if several MMIC’s are developed simultaneously or if most ofthe wafer space is paid by a production run.  The production cost of a research quality wafer is of the order of $100Kand there are typically 1000 MMIC amplifiers per wafer, leading to a production cost of $100 a chip. Modulefabrication, assembly, and test make up a total cost of the order of $1000.   More labor is required to assemble and tunea MIC amplifier but this also varies widely with the difficulty of the specifications  and experience of the technicians.A  typical estimate may be $2000 for the MIC amplifier. If we take $200K as the development cost of a MMICamplifier and  $50K to develop an MIC amplifier then the MMIC is less expensive for quantities over 150.  During thenext few years it may be expected that there will be MMIC LNA's available that are known to give good cryogenicperformance and are available commercially off-the-shelf and hence can provide MMIC  LNA's with no developmentcost.Reliability -  Reliable MIC amplifiers can certainly be constructed but the larger number of interconnections dependantupon human skill makes it easier to achieve reliability with a  MMIC amplifier.WIDEBAND MICROWAVE AMPLIFIERS FOR LARGE  ANTENNA ARRAYSThere are requirements for large numbers of very low noise cryogenic LNA’s for large of antennas being designed orconsidered in the radio astronomy and space science communities as shown in Table I. The layout and measured noiseperformance of a MMIC amplifier designed for the  1 to 11 GHz range is shown in Figures 1 and 2.  This amplifier is aprototype of an amplifier with a balanced input that is required for a wideband log-periodic feed that is being designedfor the SETI array. To reduce cryocooler costs operation in the temperature range of 50 to 80K is being considered; theprototype amplifier has a noise temperature of <22K over most of the required frequency range even when operated at80K.   This noise is low but is several degrees higher than predicted on the basis of noise temperatures measured at 100GHz  with the same type of transistors [2].MMIC LNA’s for still wider frequency ranges are being developed either for use in very wideband systems or for IFamplifiers in millimeter wave or submillimeter wave receivers. MMIC amplifiers with instantaneous bandwidthcovering the 1 to 60 GHz range have been designed, fabricated at both TRW and HRL foundries, and have been testedat room temperature. The amplifier is coolable but in its present form dissipates  about 50 to 150 mW of DC power atroom temperature.  A noise temperature of the order of 50K  with power dissipation of  20 to 50 mW  is expected atcryogenic temperatures.It is important to note that both of the wideband amplifiers are designed to have low noise when driven from a 50 ohmsource but do not have a matched input (i.e S11 approaches but is less than 1). The conventional methods of achievingboth noise and input match (balanced amplifier, feedback, or isolators) become extremely feasible at bandwidthsbeyond one octave.  The system performance penalty for the lack of input match is the sensitivity of gain to antennaimpedance.MILLIMETER WAVE MMIC LNA’SA table of millimeter wave LNA’s and mixers currently being developed at JPL is shown in Table II.  Roomtemperature results for the 120LNX and  200LN1 have been previously published [1,3] and  most of the devices havenot yet been tested at cryogenic temperatures  An array of 16 MMIC receivers ( to be expanded to 32) covering the 85to 115 GHz range  has been constructed and is in operation on the 15m radio telescope of the Five College RadioObservatory of U. of Massachusetts [4,5,6] . These receivers utilize the 105LN1P  as a first stage and the 86LN1A  as asecond stage.  The noise and gain of both of the MMIC’s at a temperature of 15K are shown in Figure 3 along with aninterior view of the WR-10 waveguide module containing either device.  More details are given in the referencedpublications.  Recent measurements at JPL of the gain and phase match of a pair of cascaded amplifiers with 35 to 40dB gain  has shown amplitude and phase match of 0.2 dB rms and 5° rms from 80 to 100 GHz.TRANSCONDUCTANCE FLUCTUATIONSThe gain of all field-effect transistor (including HEMT) amplifiers randomly fluctuates as a function of time [7,8,9,].This effect degrades the sensitivity of  wide-bandwidth, slow-switched radiometers and may be a factor in AM noise ofradar systems and phase noise in oscillators.  The cause is believed to be due to carriers going into and out of  traps inthe semiconductor material. A summary of what is known is as follows:1) The transconductance fluctuation, ∆Gm/Gm, has a 1/F spectrum with values in the range of  5 to 50 parts per millionat 1Hz for a 50 um wide transistor. This spectrum must turn over at some low frequency – perhaps 1 mHz  since largegain changes are not observed over long periods (months) of time.2) The fluctuation varies as the inverse square root of the width of the transistor.3)  The fluctuation appears to become worse by a factor of  2 to 10 at cryogenic temperatures.4) The fluctuation is not strongly dependent upon the bias point.  This is the case even if the device is biased at the peakof the transconductance vs gate bias curve where it is insensitive to gate bias.5) The fluctuation is uncorrelated with drain current fluctuations. A constant drain current power supply with feedbackcontrolled gate voltage does not reduce the fluctuation.NOISE MODELINGThe Pospieszalski  noise model [10] with gate noise, Tg, equal to ambient temperature, Tamb, and drain noise, Td = 300+ 6 * Tamb, describes the measured noise of the lowest noise sample of the  105LN1P amplifier with a noise of theorder of 30K at 100 GHz. This result is with the optimum bias for each temperature.  However, the spread of cryogenicnoise temperature even from chips from the same wafer is quite large, 30K to 60K, so that the Td equation would bedifferent for different transistors. There is much less variation in room temperature noise.  MMIC amplifiers of typeWBA5, made from the same wafer, as the 105LN1P appear to have higher noise by about 10K at Tamb = 20K than ispredicted by the above Td equation. It is not known at present whether insufficient samples  (only 2) have beenmeasured or whether gate current noise is having an effect at cryogenic temperature.A recent paper which calculates Td  using Monte Carlo methods at Tamb = 300K and 15K finds that it is not verysensitive to temperature if the electric field is kept constant, i.e for constant bias, but Td is lower at lower electric field.However at cryogenic temperature the drain voltage and drain current can be adjusted to be much lower without a largereduction in gain and this accounts for the reduction of Td (the electric field is lower).  Thus a theoretical investigationof optimum transistors for low cryogenic noise should include an understanding of the transconductance behavior at lowdrain bias and optimization of Td / (Gm^2).ACKNOWLEDGMENTThe research described in this paper was carried out in part by the Jet Propulsion Laboratory, California Institute ofTechnology, under contract with the National Aeronautics and Space Administration.REFERENCES[1] S. Weinreb, T. Gaier, R. Lai, M. Barsky, Y. C. Leong, and L. Samoska, “High Gain 150-215 GHz MMIC Amplifierwith Integral Waveguide Transitions,”  IEEE MGWL, vol 9, no. 7, July, 1999, pp. 282-284.[2] S. Weinreb, “Noise  temperature estimates for a next generation very large microwave array,” IEEE 1998 MTT-SDigest[3]  S. Weinreb, P.C. Chao, and W. Copp, “Full waveguide band  90 to 140 GHz MMIC amplifier module,”  IEEE 1997MTT-S Digest, PP. 1279-1280.[4] S. Weinreb, R. Lai, N. Erickson, T. Gaier, and J. Wielgus, “W-band InP wideband MMIC LNA with 30K noisetemperature; IEEE 1999 MTT-S Digest, vol. 1, pp. 101-104[5] N. Erickson, R. Grosslein, R. Erickson, and S. Weinreb, “A Cryogenic Focal Plane Array for 85-115 GHz UsingMMIC Preamplifiers”,  IEEE 1999 MTT-S Digest, vol. 1, pp. 251-254.[6] N. Erickson, R. Grosslein, R. Erickson, and S. Weinreb, “A Cryogenic Focal Plane Array for 85-115 GHz UsingMMIC Preamplifiers”,  IEEE Trans. on Mic. Th. and Tech., vol. 47, no. 12, Dec. 1999, pp. 2212-2219.[7] N.C. Jarosik, "Measurements of the Low-Frequency-Fluctuations fo a 30-GHz High Electron Mobility TransistorCryogenic Amplifier ", IEEE Trans. on Mic. Th. and Tech., vol 44, no. 2, Feb 1996, pp. 193-197[8] E. J. Wollack and M.W. Pospieszalski, "Characteristics of broadband InP millimeter-wave amplifiers forradiometry." 1998 MTT-S Digest, Vol.II, pp. 669-672.[9] J. D. Gallego and I. L. Fernandez, "Measurements of Gain Fluctuations in GaAs and InP Cryogenic HEMTAmplfiiers," Technical Report C.A.Y. 2000-1, Centro Astonomico de Yebes, Spain.[10]  M. Pospieszalski, "Modeling of Noise Parameters of MESFET's and MODFET's and Their FrequencyDependence," 1989 IEEE MTT Trans, vol. MTT-37, pp. 1340-1350.Table 1 –Future Arrays of Cryogenic Microwave ReceiversArray Purpose Elements Frequency Range StatusSETI Search for extraterrestrialintelligence500 x 5m .5 to 11 GHz HardwaredevelopmentDSNA Space communication 4000 x 5m 8 to 40 GHz System studySKA Radio astronomy TBD – 10^6m area .5 to 20 GHz System studyTable 2 – Millimeter Wave MMIC Designs Under Development at JPLType Frequency Foundry Technology ApplicationWBA5 .5 - 20 GHz TRW,HRL 0.1um InP Cryogenic IF AmplfierWBA7 1 - 60 GHz TRW,HRL 0.1um InP Very Wideband, Low Power40LNX 35-60 GHz TRW, HRL 0.1um InP LNA for Sensor50LN1 45-65 GHz TRW 0.1um InP LNA for Atmospheric Array53MIX1 49-57 GHz UMS GaAs Diode I/Q Mixer70LNX 50-75 GHz TRW,HRL 0.1um InP LNA for RadioAstronomy86LN1A 75-120 GHz HRL 0.1um InP Airborne Imaging105LN1 65-105 GHz TRW 0.1um InP Cryogenic LNA,  Radio Astronomy120LNX 100-140 GHz TRW,HRL 0.1um InP Atmospheric Sensing120MIX1 90-140 GHz UMS GaAs Diode Balanced Mixer190LN1 180-200 GHz Sanders 0.1um InP Atmospheric Sensing200LN1 170-210 GHz TRW .08 um InP Atmospheric Sensing200MIX1 170-210 GHz UMS GaAs Diode 2nd Harmonic MixerT NSiNO tIHEMT TransmissionSingleChipLNAInP MMIC LNA Noise and Gain051015202530351 2 3 4 5 6 7 8 9 10 11 12Frequency, GHzNoise, K, or Gain, dBWBA5T SN102, Wafer 4080-040, #731Bias: 1.46V, 0V, 14 mA @ 19K1.46V, +0.6V, 25.5 mA @80KNoise @ 19KNoise @ 80KGain @ 80KOutput WR-10WaveguideDC BiasConnectoInput WR-10WaveguideProbeTransition 4-StageMMIC LNAFigure 1 - Layout of MMIC  1 to 20 GHz LNA ; chip size is 2.0 x .74 mm.Figure 2 - Module with single chip MMIC LNA and measured noise temperature of the module at  physicaltemperatures  of 19K and 80K.Figure 3 – Interior view of split-block module used to package either of the 4-stage MMIC’s with data shown in atright.. The data shows noise and gain at 20K for two InP  HEMT low noise amplifiers used in the U. of Massachusetts16-element focal plane array receiver [6].  The first stage is the 105LN1P fabricated at TRW and the second stage is an86LN1 fabricated at HRL laboratories.

Cryogenic MMIC low noise amplifiers

AMS Acta - Alm@DL - Università di Bologna

CRYOGENIC MMIC LOW NOISE AMPLIFIERS
S. Weinreb1,  T. Gaier1,  J. E. Fernandez1, N. Erickson2, and J. Wielgus2
1Jet Propulsion Laboratory, California Institute of Technology, sander.weinreb@jpl.nasa.gov
2Department of Physics and Astronomy, U. of Massachusetts,  neal@fcrao1.phast.umass.edu
ABSTRACT
Monolithic (MMIC) and discrete transistor (MIC) low noise amplifiers are compared on the basis of performance,
cost, and reliability.  The need for cryogenic LNA’s for future large microwave arrays for  radio astronomy is briefly
discussed  and  data is presented on a prototype LNA for  the  1 to 10 GHz range  along with a  very wideband LNA for
the 1 to 60 GHz range. A table of MMIC LNA and mixer designs under development  for the frequencies  up to 210 GHz
is reported and data on cryogenic amplifiers in the 85 to 115 GHz is reviewed.   The current status of the topics of
transconductance fluctuations and cryogenic noise modeling will be briefly summarized.
 MMIC VS MIC COMPARISON
As a starting point it is  instructive to compare the advantages and disadvantages of monolithic microwave integrated
circuit   (MMIC) low noise amplifiers with microwave integrated circuit (MIC) amplifiers constructed with discrete
chip transistors and passive microstrip circuit boards.   A summary of this comparison on the basis of performance,
frequency range, cost, and reliability follows.
Transistor Performance  - The discrete transistors used in the MIC case are manufactured in the same manner as the
transistors built into the MMIC amplifier and to a large extent this leads to the same expected performance.  Two
exceptions can be argued.  In the MIC case,  transistors can be selected to give the lowest noise; however the MMIC's
can also be selected. To some extent the  cryogenic low noise performance is correlated between different discrete
transistors or MMIC's on a  single wafer.  With of the order of 100,000 discrete transistors or 1000 MMIC's on a wafer,
a larger number of cryogenic amplifiers can be built from one "golden" wafer.  However, the need for very large
numbers of  cryogenic amplifiers has not  yet  occurred and could be met by processing a large number of wafers and
selecting the best.
Passive Circuit Performance  -  A wider variety of passive circuit element values and quality factors are available to the
MIC designer.  However, in most cases the loss in a cryogenic  passive circuit  is negligible and  a MMIC can use an
external element such as an input inductor if it is necessary.   It is possible to make shorter connections on a MMIC
particularly  the  transistor source ground and this can help bandwidth and stability.
Frequency Range - The short connections possible with a MMIC become an important factor above 100 GHz.  MMIC
amplifiers with high gain at 215 GHz have been reported [1] but  has not been achieved with MIC amplifiers.
Multistage MMIC amplifiers operating below 500 MHz have difficulty with achieving sufficiently large coupling and
bypass  capacitors.  DC coupling may be feasible in some cases but this restriction does not occur with MIC amplifiers
utilizing multi-plate layer, high-dielectric constant capacitors.
Cost – The development cost of a MMIC varies between $50K and $500K dependant upon  the processing  cost for
small mounts of wafer space for experimental circuits, the difficulty of the specifications, and the legacy  of similar
designs.  The experimental processing cost is minimized if several MMIC’s are developed simultaneously or if most of
the wafer space is paid by a production run.  The production cost of a research quality wafer is of the order of $100K
and there are typically 1000 MMIC amplifiers per wafer, leading to a production cost of $100 a chip. Module
fabrication, assembly, and test make up a total cost of the order of $1000.   More labor is required to assemble and tune
a MIC amplifier but this also varies widely with the difficulty of the specifications  and experience of the technicians.
A  typical estimate may be $2000 for the MIC amplifier. If we take $200K as the development cost of a MMIC
amplifier and  $50K to develop an MIC amplifier then the MMIC is less expensive for quantities over 150.  During the
next few years it may be expected that there will be MMIC LNA's available that are known to give good cryogenic
performance and are available commercially off-the-shelf and hence can provide MMIC  LNA's with no development
cost.
Reliability -  Reliable MIC amplifiers can certainly be constructed but the larger number of interconnections dependant
upon human skill makes it easier to achieve reliability with a  MMIC amplifier.
WIDEBAND MICROWAVE AMPLIFIERS FOR LARGE  ANTENNA ARRAYS
There are requirements for large numbers of very low noise cryogenic LNA’s for large of antennas being designed or
considered in the radio astronomy and space science communities as shown in Table I. The layout and measured noise
performance of a MMIC amplifier designed for the  1 to 11 GHz range is shown in Figures 1 and 2.  This amplifier is a
prototype of an amplifier with a balanced input that is required for a wideband log-periodic feed that is being designed
for the SETI array. To reduce cryocooler costs operation in the temperature range of 50 to 80K is being considered; the
prototype amplifier has a noise temperature of <22K over most of the required frequency range even when operated at
80K.   This noise is low but is several degrees higher than predicted on the basis of noise temperatures measured at 100
GHz  with the same type of transistors [2].
MMIC LNA’s for still wider frequency ranges are being developed either for use in very wideband systems or for IF
amplifiers in millimeter wave or submillimeter wave receivers. MMIC amplifiers with instantaneous bandwidth
covering the 1 to 60 GHz range have been designed, fabricated at both TRW and HRL foundries, and have been tested
at room temperature. The amplifier is coolable but in its present form dissipates  about 50 to 150 mW of DC power at
room temperature.  A noise temperature of the order of 50K  with power dissipation of  20 to 50 mW  is expected at
cryogenic temperatures.
It is important to note that both of the wideband amplifiers are designed to have low noise when driven from a 50 ohm
source but do not have a matched input (i.e S11 approaches but is less than 1). The conventional methods of achieving
both noise and input match (balanced amplifier, feedback, or isolators) become extremely feasible at bandwidths
beyond one octave.  The system performance penalty for the lack of input match is the sensitivity of gain to antenna
impedance.
MILLIMETER WAVE MMIC LNA’S
A table of millimeter wave LNA’s and mixers currently being developed at JPL is shown in Table II.  Room
temperature results for the 120LNX and  200LN1 have been previously published [1,3] and  most of the devices have
not yet been tested at cryogenic temperatures  An array of 16 MMIC receivers ( to be expanded to 32) covering the 85
to 115 GHz range  has been constructed and is in operation on the 15m radio telescope of the Five College Radio
Observatory of U. of Massachusetts [4,5,6] . These receivers utilize the 105LN1P  as a first stage and the 86LN1A  as a
second stage.  The noise and gain of both of the MMIC’s at a temperature of 15K are shown in Figure 3 along with an
interior view of the WR-10 waveguide module containing either device.  More details are given in the referenced
publications.  Recent measurements at JPL of the gain and phase match of a pair of cascaded amplifiers with 35 to 40
dB gain  has shown amplitude and phase match of 0.2 dB rms and 5° rms from 80 to 100 GHz.
TRANSCONDUCTANCE FLUCTUATIONS
The gain of all field-effect transistor (including HEMT) amplifiers randomly fluctuates as a function of time [7,8,9,].
This effect degrades the sensitivity of  wide-bandwidth, slow-switched radiometers and may be a factor in AM noise of
radar systems and phase noise in oscillators.  The cause is believed to be due to carriers going into and out of  traps in
the semiconductor material. A summary of what is known is as follows:
1) The transconductance fluctuation, ∆Gm/Gm, has a 1/F spectrum with values in the range of  5 to 50 parts per million
at 1Hz for a 50 um wide transistor. This spectrum must turn over at some low frequency – perhaps 1 mHz  since large
gain changes are not observed over long periods (months) of time.
2) The fluctuation varies as the inverse square root of the width of the transistor.
3)  The fluctuation appears to become worse by a factor of  2 to 10 at cryogenic temperatures.
4) The fluctuation is not strongly dependent upon the bias point.  This is the case even if the device is biased at the peak
of the transconductance vs gate bias curve where it is insensitive to gate bias.
5) The fluctuation is uncorrelated with drain current fluctuations. A constant drain current power supply with feedback
controlled gate voltage does not reduce the fluctuation.
NOISE MODELING
The Pospieszalski  noise model [10] with gate noise, Tg, equal to ambient temperature, Tamb, and drain noise, Td = 300
+ 6 * Tamb, describes the measured noise of the lowest noise sample of the  105LN1P amplifier with a noise of the
order of 30K at 100 GHz. This result is with the optimum bias for each temperature.  However, the spread of cryogenic
noise temperature even from chips from the same wafer is quite large, 30K to 60K, so that the Td equation would be
different for different transistors. There is much less variation in room temperature noise.  MMIC amplifiers of type
WBA5, made from the same wafer, as the 105LN1P appear to have higher noise by about 10K at Tamb = 20K than is
predicted by the above Td equation. It is not known at present whether insufficient samples  (only 2) have been
measured or whether gate current noise is having an effect at cryogenic temperature.
A recent paper which calculates Td  using Monte Carlo methods at Tamb = 300K and 15K finds that it is not very
sensitive to temperature if the electric field is kept constant, i.e for constant bias, but Td is lower at lower electric field.
However at cryogenic temperature the drain voltage and drain current can be adjusted to be much lower without a large
reduction in gain and this accounts for the reduction of Td (the electric field is lower).  Thus a theoretical investigation
of optimum transistors for low cryogenic noise should include an understanding of the transconductance behavior at low
drain bias and optimization of Td / (Gm^2).
ACKNOWLEDGMENT
The research described in this paper was carried out in part by the Jet Propulsion Laboratory, California Institute of
Technology, under contract with the National Aeronautics and Space Administration.
REFERENCES
[1] S. Weinreb, T. Gaier, R. Lai, M. Barsky, Y. C. Leong, and L. Samoska, “High Gain 150-215 GHz MMIC Amplifier
with Integral Waveguide Transitions,”  IEEE MGWL, vol 9, no. 7, July, 1999, pp. 282-284.
[2] S. Weinreb, “Noise  temperature estimates for a next generation very large microwave array,” IEEE 1998 MTT-S
Digest
[3]  S. Weinreb, P.C. Chao, and W. Copp, “Full waveguide band  90 to 140 GHz MMIC amplifier module,”  IEEE 1997
MTT-S Digest, PP. 1279-1280.
[4] S. Weinreb, R. Lai, N. Erickson, T. Gaier, and J. Wielgus, “W-band InP wideband MMIC LNA with 30K noise
temperature; IEEE 1999 MTT-S Digest, vol. 1, pp. 101-104
[5] N. Erickson, R. Grosslein, R. Erickson, and S. Weinreb, “A Cryogenic Focal Plane Array for 85-115 GHz Using
MMIC Preamplifiers”,  IEEE 1999 MTT-S Digest, vol. 1, pp. 251-254.
[6] N. Erickson, R. Grosslein, R. Erickson, and S. Weinreb, “A Cryogenic Focal Plane Array for 85-115 GHz Using
MMIC Preamplifiers”,  IEEE Trans. on Mic. Th. and Tech., vol. 47, no. 12, Dec. 1999, pp. 2212-2219.
[7] N.C. Jarosik, "Measurements of the Low-Frequency-Fluctuations fo a 30-GHz High Electron Mobility Transistor
Cryogenic Amplifier ", IEEE Trans. on Mic. Th. and Tech., vol 44, no. 2, Feb 1996, pp. 193-197
[8] E. J. Wollack and M.W. Pospieszalski, "Characteristics of broadband InP millimeter-wave amplifiers for
radiometry." 1998 MTT-S Digest, Vol.II, pp. 669-672.
[9] J. D. Gallego and I. L. Fernandez, "Measurements of Gain Fluctuations in GaAs and InP Cryogenic HEMT
Amplfiiers," Technical Report C.A.Y. 2000-1, Centro Astonomico de Yebes, Spain.
[10]  M. Pospieszalski, "Modeling of Noise Parameters of MESFET's and MODFET's and Their Frequency
Dependence," 1989 IEEE MTT Trans, vol. MTT-37, pp. 1340-1350.
Table 1 –Future Arrays of Cryogenic Microwave Receivers
Array Purpose Elements Frequency Range Status
SETI Search for extraterrestrial
intelligence
500 x 5m .5 to 11 GHz Hardware
development
DSNA Space communication 4000 x 5m 8 to 40 GHz System study
SKA Radio astronomy TBD – 10^6m area .5 to 20 GHz System study
Table 2 – Millimeter Wave MMIC Designs Under Development at JPL
Type Frequency Foundry Technology Application
WBA5 .5 - 20 GHz TRW,HRL 0.1um InP Cryogenic IF Amplfier
WBA7 1 - 60 GHz TRW,HRL 0.1um InP Very Wideband, Low Power
40LNX 35-60 GHz TRW, HRL 0.1um InP LNA for Sensor
50LN1 45-65 GHz TRW 0.1um InP LNA for Atmospheric Array
53MIX1 49-57 GHz UMS GaAs Diode I/Q Mixer
70LNX 50-75 GHz TRW,HRL 0.1um InP LNA for RadioAstronomy
86LN1A 75-120 GHz HRL 0.1um InP Airborne Imaging
105LN1 65-105 GHz TRW 0.1um InP Cryogenic LNA,  Radio Astronomy
120LNX 100-140 GHz TRW,HRL 0.1um InP Atmospheric Sensing
120MIX1 90-140 GHz UMS GaAs Diode Balanced Mixer
190LN1 180-200 GHz Sanders 0.1um InP Atmospheric Sensing
200LN1 170-210 GHz TRW .08 um InP Atmospheric Sensing
200MIX1 170-210 GHz UMS GaAs Diode 2nd Harmonic Mixer
T NSiN
O tI
HEMT Transmission
Single
Chip
LNA
InP MMIC LNA Noise and Gain
0
5
10
15
20
25
30
35
1 2 3 4 5 6 7 8 9 10 11 12
Frequency, GHz
N
oi
se
, K
, o
r G
ai
n,
 d
B
WBA5T SN102, Wafer 4080-040, #731
Bias: 1.46V, 0V, 14 mA @ 19K
1.46V, +0.6V, 25.5 mA @80K
Noise @ 19K
Noise @ 80K
Gain @ 80K
Output WR-10
Waveguide
DC Bias
Connecto
Input WR-10
Waveguide
Probe
Transition 4-Stage
MMIC LNA
Figure 1 - Layout of MMIC  1 to 20 GHz LNA ; chip size is 2.0 x .74 mm.
Figure 2 - Module with single chip MMIC LNA and measured noise temperature of the module at  physical
temperatures  of 19K and 80K.
Figure 3 – Interior view of split-block module used to package either of the 4-stage MMIC’s with data shown in at
right.. The data shows noise and gain at 20K for two InP  HEMT low noise amplifiers used in the U. of Massachusetts
16-element focal plane array receiver [6].  The first stage is the 105LN1P fabricated at TRW and the second stage is an
86LN1 fabricated at HRL laboratories.


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Cryogenic MMIC low noise amplifiers

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AMS Acta

AMS Acta - Alm@DL - Università di Bologna