Optical scintillometers measure atmospheric turbulence using the phenomenon of optical scintillation. Scintillation denotes the apparent intensity fluctuations of a remote radiation source, an effect known from starlight twinkling. There is a thorough theory between the attributing refractive index fluctuations and thermal turbulence in the atmosphere. Optical scintillometers can measure a wide range of quantities used in meteorology and related sciences. Optical scintilometers are also applied in wave propagation studies.

The quantities most often measured using scintillometers are the structure function constant of refractive index C_n², the structure function constant of temperature C_T², the turbulent flux of heat, the turbulent flux of momentum, the inner scale of turbulence, the kinetic energy dissipation rate and the crosswind. Evaporation or evapotranspiration are also commonly assessed.

Optical scintillometers measure a path average between a transmitter and a receiver. They have superior characteristics over conventional point measurement devices. Because scintillometers are double-ended remote sensing systems, the measurement paths can also lead over terrain which is difficult to access by in-situ sensors. Since transmitter and receiver are remote from the measurement volume, there is no flow distortion caused by them. The path averaging does not only provide spatially representative data, it also reduces the need of averaging over time, resulting in a higher temporal resolution of the obtained statistical measurement results.

Scintillometry is still a relatively new technology which is far from being fully exploited. As an inventor and pioneer in scintillometry, Scintec supplies the most up-to-date devices which are used at the forefront of atmospheric sciences all over the world.