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This project develops methods for very accurate measurements of thermal noise and provides support for such measurements in the communications and electronics industries and in other government agencies.


Amplifier noise-parameter measurements using two cryogenic standards, one to calibrate the radiometer and one for input to the amplifier.

Customer Needs

Noise is a crucial consideration in designing or assessing the performance of virtually any electronic device or system that involves detection or processing of a signal. This includes communications systems, such as cellular phones and home entertainment systems, as well as systems with internal signal detection and processing, such as guidance and tracking systems or electronic test equipment. The global market for microwave and millimeter wave devices in these areas is huge and will grow larger. Important trends requiring support include the utilization of higher frequencies, the growing importance of low-noise amplifiers and transistors, and the perpetual quest for faster, less expensive measurements. The two most important noise-related technical parameters requested by industry are the noise temperature of a one-port source and the noise figure of an amplifier.

Noise power is also the quantity that is measured in passive remote sensing, such as that used to measure properties of the earth's surface from satellites or airplanes. The growing importance of such measurements for climate monitoring, weather forecasting, agriculture, and other applications has highlighted the need for better calibration techniques, smaller uncertainties, and compatibility between results from different instruments.

Technical Strategy

We are working in three general areas: traditional noise-temperature measurements, characterization of amplifier and transistor noise properties, and calibration of remote-sensing radiometers. In traditional noise-temperature measurements, we offer measurement services at 30 and 60 megahertz and from 1 to 40 gigahertz for coaxial sources, and from 8.2 gigahertz to 65 gigahertz for waveguide sources. Recent improvements have reduced the time required for these measurements, thereby reducing the costs to our customers.

The second general thrust of the project is in amplifier and transistor noise-parameter measurements. The long-term goals in this area are to improve techniques for measurement of noise parameters of low-noise amplifiers and transistors, to develop measurement capability for noise parameters of amplifiers with coaxial connectors from 1 to 12 gigahertz, and to provide a mechanism for industry to access this capability, either through measurement comparisons or a measurement service.

A new thrust of the project is in improving methods for calibration and validation of microwave radiometers used for remote sensing from satellite or airplane. The central element of this effort will be the development of microwave brightness-temperature standards, comprising both standard radiometers and standard calibration targets. The standard radiometers will be used to measure customer calibration targets at NIST, and the standard calibration targets will be used in measurements at outside facilities, as well as for comparison measurements with the NIST standard radiometer.


Our goals for this coming year are to measure the noise parameters of a low-noise amplifier for an interlaboratory comparison with NPL, measure the noise parameters of a cryogenic amplifier belonging to the Terahertz Project, and measure noise parameters of ultra-large-scale integration (ULSI) devices on wafer for comparison to IBM and RFMD. We intend to study the uncertainties in onwafer measurements of noise parameters; design a temperature-controlled, shielded, anechoic chamber for standard radiometer(s); use the Physics Laboratory's infrared (IR) imaging system to study thermal gradients in a calibration target used for microwave remote sensing; and continue to provide noise-temperature measurement services.

   • Warsaw University of Technology (W. Wiatr), on-wafer noise-parameter measurements
   • IBM and RFMicroDevices (Kelvin Project), noise parameters of ULSI devices
   • National Polar-orbiting Operational Environmental Satellite System (NPOESS), ATMS Calibration and Validation Working Group
   • NOAA Environmental Technology Laboratory (A. Gasiewski and M. Klein), calibration target characterization
   • NASA Microwave Instrument Technology Branch (P. Racette, J. Piepmeier), calibration target characterization
   • Physics Laboratory (J. Rice, C. Johnson), radiometer calibration and validation and target characterization
   • Information Technology Laboratory (K. Coakley, J. Splett), nonlinear modeling of tunnel diode detectors

Standards and Technical Committee Participation:
   • Consultative Committee on Electricity and Magnetism (CCEM), Working Group on Radio Frequencies, Chairman
   • IEEE Microwave Theory and Techniques Society, Technical Committee on Microwave Low-Noise Techniques, TC-14
   • IEEE Geoscience and Remote Sensing Society Technical Committee on Instrumentation and Future Technologies
   • IEEE Geoscience and Remote Sensing Society liaison to IEEE Standards Board
   • CEOS Working Group on Calibration and Validation, Microwave Sensors Subgroup, Standard Terminology compilation (Chapters I and II)

Major Accomplishments

• Amplifier Noise-Parameter Measurements and Verification — The Noise Project completed development of a measurement capability for noise parameters of low-noise amplifiers (LNAs), including a Monte Carlo assessment of uncertainties. We also completed and successfully implemented two types of verification tests for such measurements. All tests were satisfied within the uncertainties, thereby providing support for both the measurement results and the associated uncertainty estimates.
• Variable-Termination Unit — A variable-termination unit (VTU) was designed, fabricated, and tested. The VTU will be used in noise-parameter measurements, allowing automated switching to an array of different input terminations for the amplifier, rather than the manual disconnecting and connecting that is currently used.
• Traceability for Microwave Remote-Sensing Measurements — A plan was developed for establishing traceability to NIST for microwave remote-sensing measurements. The plan includes the theory necessary to link microwave remote-sensing measurements to primary noise standards. It was documented in a NIST internal report and in a conference paper.
• Measurement of Microwave Brightness Temperature — Preliminary measurements were performed on a hot calibration target borrowed from the NOAA Environmental Technology Laboratory. A standard gain horn (SGH) was characterized by the Antenna Metrology Project and was connected to the measurement plane of the Noise Project's WR-42 waveguide radiometer to form a standard radiometer for remote sensing. This standard radiometer was then set up to view the calibration target mounted in the anechoic chamber. The target's brightness temperature was measured for different distances and compared to the nominal brightness temperature based on the sampled physical temperature. Satisfactory to good agreement was obtained, and possible areas of improvement were identified.
• Target Reflectivity — A study performed in FY 2004 on the effects of target reflectivity in the calibration of microwave remote-sensing radiometers was documented in a conference paper and a journal paper. This study found that a common approximation used in calibrating microwave radiometers leads to errors that can be quite significant.
• Detector Linearity Study — Measurements were made on tunnel diode detectors of the type typically used in microwave remote-sensing radiometers. These measurements included variations in detector temperature as well as output load impedance. Results point to improved test methods and a way to greatly reduce the cost associated with radiometer linearity tests.
• CEOS Definitions — The Web site for standard definitions was maintained ( and Chapters 1 and 2 of the compilation of standard definitions for microwave radiometry were accepted by the Committee on Earth Observation Satellites (CEOS).

Created August 11, 2009, Updated July 13, 2022