The SIRCUS facility is designed to reduce the uncertainty in irradiance and radiance responsivity calibrations to the 0.1 % level and to expand the spectral range where these uncertainty levels are achievable. The facility expands on previous work at NIST and the National Physical Laboratory (NPL) in the U.K. beginning in the mid-1980's using tunable lasers and silicon-based pyrometers traceable to cryogenic radiometers to determine the melting and freezing points of primary metal blackbodies with uncertainties approaching or exceeding those achievable using more conventional technologies.
All irradiance and radiance responsivity calibrations made in the SIRCUS facility are traceable to the U.S. standard for optical power, the Primary Optical Watt Radiometer (POWR), which is located in the SIRCUS facility. The optical power scale is transferred either directly from POWR, or a portable cryogenic radiometer that is directly traceable to POWR, to transfer detectors used in SIRCUS. The uncertainty in the detector responsivity is minimized by the short calibration chain from the primary cryogenic radiometer to the reference detector responsivity..The irradiance responsivity of the SIRCUS reference detector is derived from the power responsivity and the area of a precision aperture attached to the front of the detector. The area of this precision aperture is measured with uncertainties less than 100 ppm at the NIST Aperture Area Facility.
In many cases, instruments cannot travel to NIST for calibration. To increase the dissemination of the SIRCUS-based scale, we have developed Traveling SIRCUS. These table-top, tunable laser systems are portable and include integrating spheres and transfer standard detectors. The traveling SIRCUS units have been sent to NASA, NOAA, and USGS sites to characterize instruments in support of NIST's Environmental Remote Sensing Program.
For more information about the calibration setup and uncertainties for SIRCUS measurements, see SIRCUS facility and uncertainties.