Home > Ozone and Radiation Observation > Observation of Infrared Radiation
All materials emit electromagnetic radiation in proportion to the fourth power of their temperature. The earth and its atmosphere emit infrared radiation with wavelengths longer than those of solar radiation because their temperature is lower than that of the sun’s surface. Most of the energy of the infrared radiation emitted from the earth and its atmosphere is concentrated in the 3 - 100 μm range.
A pyrgeometer is used to observe infrared radiation. This is a thermopile radiometer with a sensor that converts absorbed radiant energy into thermal energy using a thermocouple. It allows measurement of infrared radiation with high accuracy regardless of wavelengths.
A pyrgeometer is used for observation of infrared radiation. The instrument’s sensor is covered with a silicone dome to keep out wind and rain, and the unit is ventilated to improve measurement stability. The inner surface of the dome has an interference filter that cuts out short-wavelength radiative energy from the sun.
Pyrgeometer used for observation of downward infrared radiation
Pyrgeometer used for observation of upward infrared radiation
Infrared radiation observation data are acquired from regular one-second samplings, and their quality is checked to ensure compliance with Baseline Surface Radiation Network (BSRN) specifications. Examples of data from observation at Tsukuba are shown below.
Seasonal variations of monthly averages at Tsukuba (2021)
Long-term variations of annual average infrared radiation at Tsukuba