Basically a sky - sun photometer consists of a light sensor with an amplifier. The sensor is kept in a sealed metal cylinder (or sensor head) behind a quartz window. A tube for limiting the incident light reaching the sensor is attached in front of the window. By the use of a rotating wheel we can sequentially interpose different interferential filters to select a set of wavelengths for measuring incoming radiance. A programmable robot will aim the optical head at the different required sun and sky positions. This basic instrument can be completed with other features: a diode for keeping the alignment with the sun, solar panels for autonomy, power batteries, and wet sensors to park the instrument when it rains.

There are several commercially available sky-sun photometers in the international market. The two most well known models are the Cimel Electronique CE318 (produced in France) and the Prede POM (produced in Japan). Both instruments are devoted to atmospheric aerosol characterization and they offer very similar features.


CE318 in Burjassot (Spain)
  • Manufacturer: Cimel (France)
  • Automatic sun-sky photometer.
  • Normal, polarised, or extended NIR versions.
  • Available standard channels: 340, 380, 440, 500, 670, 870, 940, 1020, 1600 nm.
  • FWHM: 2 nm (UV), 10 nm (VIS), 40nm (NIR).
  • Active sun tracking.
  • Wet sensor.
  • Temperature measurement.
  • Solar panel for autonomy in remote sites.
  • It is possible to send the data via satellite.
  • Light weight.
POM01L from Skynet
  • Manufacturer: Prede (Japan)
  • Automatic sun-sky photometer.
  • Normal or extended NIR versions.
  • Available standard channels: 315, 400, 440, 500, 675, 870, 940, 1020, 1600 nm.
  • FWHM: 2 nm (UV), 10 nm (VIS), 40nm (NIR).
  • Active sun tracking.
  • Wet sensor.
  • Temperature controlled.
  • In situ calibration procedure by default.
  • Robust and flexible.


Instruments and networks are very intricately related. These are the main differences between both network and instrument concepts:

  1. Radiance sensor: The POM model uses only one sensor and tube for both sky and sun measurements. On the contrary, the CE318 used two different sensors and tubes. New models of CE318 include now a single detector, but many of the active instruments still work with two sensors.

  2. Temperature effect: Due to sensor dependence on temperature in the NIR band, raw photometric measurements show a significant dependence on temperature. The POM model is equipped with a temperature controlled optical head. The CE318 standard model is not temperature controlled, but the measurements can still be corrected afterwards.

  3. Temporal resolution: CE318 radiometers measure with the AERONET standard schedule, broadly an almucantar scenario every 60 minutes and a direct sun measurement every 15 minutes. The POM radiometers measure an almucantar scenario every 10 or 20 minutes and a sun direct measurement every minute.


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