What this opportunity is
NASA is seeking to procure Sun photometers and their components for the AERONET project, which involves monitoring aerosol properties and precipitable water. This opportunity is open to all businesses as there is no set-aside, and it is categorized under NAICS 334516. The notice is a Sources Sought, indicating that interested vendors should focus on compatibility with existing instruments and specifications outlined in the statement of work, rather than submitting formal bids at this stage.
Analysis by Mindy, grounded in the SAM.gov notice.
Description
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AERONET Sun Photometer Procurement Contract
Description of Sun Photometer and Components
STATEMENT OF WORK
March 23, 2026
TABLE OF CONTENTS
SUMMARY
1. General Description
2. Instrument Specifications
Capabilities
2A – Non Required specification items (These items are part of
the specifications but will not be ordered)
• 2-1 Sun and Sky Measurement Mode Selections
• 2-2 Automatic Selection of Geometrical Conditions
• 2-3 Optics
• 2-4 Detectors
• 2-5 Filters
2B – REQUIRED SPECIFIATION ITEMS
• 2-1 Advanced Control Box
• 2-2 Tracking Robot
• 2-3 Microprocessor
• 2-4 DCS Compatibility
• 2-5 Instrument Sensitivity
• 2-6 Power Requirements
• 2-7 Environmental Requirements
3. Description of Daily Measurement Program
• 3-1 Optical Thickness and Water
• 3-2 Langley Plot
3-3 Sky Radiance Measurement
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• 3-3.1 Almucantar
• 3-3.2 Principal Plane Measurement
• 3-3.3 Hybrid Scan Measurement
Summary
NASA owns and or manages over 600 Cimel Sun-Sky-Lunar
Scanning photometers as part of the EOS Aerosol Validation Program called
AERONET. The program is part of a larger Federated Global Network of
identical instruments designed to measure aerosol properties from land and
ocean sites. In order to ensure compatibility within the network, any
additional instruments must be identical in optical characteristics,
measurement protocol, data acquisition and field hardness.
The CE 318 T Sun photometer functions reliably in the harsh
environmental conditions (humidity, rain, insects, dust and sea spray.)
expected in our remote sites. The instrument is required to have multiple
data communication options including the data collection system (DCS) of
the international constellation of geostationary meteorological satellites,
cellular and PC/internet.
The measurement protocol requires direct solar and lunar plus diffuse
sky measurements to be automatically taken according to reprogrammed
solar zenith angles and scattering angles optimized for analysis of data to
estimated aerosol properties.
We are adding additional systems to the AERONET program. The
additional systems being procured for the AERONET program must be
identical in function and be electronically compatible with the existing
instruments.
Sun and sky-scanning spectral radiometers are used in the AERONET
program to monitor aerosol optical properties and precipitable water in near
real-time for the validation of satellite-derived retrievals of aerosol
properties and provide a uniform database for long-term characterization of
aerosol optical properties within NASA's Earth Science program. To
develop such a database, AERONET has imposed a standardization in data
measurement, data collection, data format, and data processing that is
fundamental to the objectives and success of the program. Any deviation
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from these standards will erode the quality control necessary for network
operations. The following instrument specifications are required to meet the
requirements of the AERONET network measurement program.
1. GENERAL DESCRIPTION
The radiometer system will measure both sun and lunar irradiances
and sky radiances using a combination of spectral filters and a fully-
autonomous azimuth/zenith viewing microprocessor-controlled robot. The
daily data stream will be transmitted via the internationally-standardized
Data Collection System (DCS) aboard the geostationary satellite system
GOES, METEOSAT and HIMAWARI. The radiometer must be capable of
unattended operation for up to eight weeks in any environmental conditions
and be powered by rechargeable batteries and a five watt solar panel.
Place of Performance
Radiometers to be built at the Contractor facility and sent to NASA Goddard
Space Flight Center. CIMEL Electronique,172 Rue de Charonne, 75011
Paris, FR
Period of Performance
Oct 1 2026 to Sept 30 2031
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2. INSTRUMENT SPECIFICATIONS
CAPABILITIES
The Sun and Sky radiometers must have a broad spectral range from the
UV to the short wave infrared. It shall incorporate the digital electronics
in the sensor head, and its components are compatible with earlier models
of the CE318 including the robots.
The instrument shall incorporate polarization to the standard
measurements. It will be an important instrument for new research
activities and synergism with future satellite validation activities. It shall
be fully compatible with existing system components and network
standardization.
The instrument shall be able to take the atmospheric and ocean radiances.
It shall be fully compatible with the existing network components.
The instrument shall be able to be used to extend measurement from
daylight only to day and night time measurements with lunar
observations in addition to solar observations and support validation of
all Earth viewing satellite monitoring systems. It shall be compatible
with the existing robot infrastructure.
A. NON REQUIRED SPECIFICATION ITEMS
2.1 SUN AND SKY MEASUREMENT MODE
SELECTION
The radiometer must automatically change gains from the sky
radiance measurement mode to the sun-measuring mode
without saturating the signal response. It is fundamental that a
two-detector two-collimator system be used in order to assess
the quality of data from each detector system.
2.2 AUTOMATIC SELECTION OF GEOMETRICAL
CONDITIONS
The automatic instrument is set up on an axis which is able
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through step-by-step motors to move in two directions, in the
zenith and in the azimuth planes. The step-by-step motors
piloted by the microprocessor card are able to reach any
geometrical conditions. Computations of the equation of Sun
are performed by the microprocessor and combined with a four-
quadrant detector system enables accuracy of sun
position to ±0.05°. Therefore, the specification of accuracy in
pointing to any direction is ±0.05, relative to the sun.
2.3 OPTICS
Collimator Detector Sun, 1.2 degree FOV, no optics sky,
collimator 1.2 degree FOV, lens required, …
Source: SAM.gov, as posted. Verify the current solicitation before responding.