The infrared thermometer consists of an optical system, a photodetector, a signal amplifier, signal processing, and display output. The optical system converges the target infrared radiation energy within its field of view, and the size of the field of view is determined by the optical components of the thermometer and their position. The infrared energy is focused on the photodetector and converted into a corresponding electrical signal. The signal passes through the amplifier and the signal processing circuit, and is converted to the temperature value of the measured object after being corrected according to the algorithm of the internal treatment of the instrument and the target emissivity.
In nature, all objects with temperatures above absolute zero are constantly emitting infrared radiation energy to the surrounding space. The magnitude of the infrared radiation energy of an object and its distribution by wavelength are closely related to its surface temperature. Therefore, by measuring the infrared energy radiated by the object itself, it can accurately determine its surface temperature, which is the objective basis on which infrared radiation is measured.
A blackbody is an idealized radiator that absorbs radiant energy at all wavelengths. Without the reflection and transmission of energy, the surface has an emissivity of one. However, the actual objects existing in nature are hardly black. In order to clarify and obtain the law of infrared radiation distribution, it is necessary to choose a suitable model in theoretical research. This is the quantized oscillator model of body cavity radiation proposed by Planck. The law of Planck blackbody radiation, the blackbody spectral irradiance expressed in wavelength, is derived. This is the starting point of all infrared radiation theory, so it is called the blackbody radiation law. The amount of radiation of all actual objects depends on the wavelength of the radiation and the temperature of the object, as well as the type of material that makes up the object, the method of preparation, the thermal process, and the surface state and environmental conditions. Therefore, in order to apply the blackbody radiation law to all practical objects, it is necessary to introduce a proportionality factor, ie, emissivity, related to the material properties and surface state. This coefficient indicates how close the thermal radiation of the actual object is to the blackbody radiation, with values ​​between zero and less than one. According to the law of radiation, as long as the emissivity of the material is known, the infrared radiation characteristics of any object are known. The main factors affecting the emissivity are: material type, surface roughness, physical and chemical structure and material thickness.
When using the infrared radiation thermometer to measure the temperature of the target, first measure the amount of infrared radiation in the range of the target, and then calculate the temperature of the target by the thermometer. The monochromatic thermometer is proportional to the amount of radiation in the band; the two-color thermometer is proportional to the ratio of the amount of radiation in the two bands.
In nature, all objects with temperatures above absolute zero are constantly emitting infrared radiation energy to the surrounding space. The magnitude of the infrared radiation energy of an object and its distribution by wavelength are closely related to its surface temperature. Therefore, by measuring the infrared energy radiated by the object itself, it can accurately determine its surface temperature, which is the objective basis on which infrared radiation is measured.
A blackbody is an idealized radiator that absorbs radiant energy at all wavelengths. Without the reflection and transmission of energy, the surface has an emissivity of one. However, the actual objects existing in nature are hardly black. In order to clarify and obtain the law of infrared radiation distribution, it is necessary to choose a suitable model in theoretical research. This is the quantized oscillator model of body cavity radiation proposed by Planck. The law of Planck blackbody radiation, the blackbody spectral irradiance expressed in wavelength, is derived. This is the starting point of all infrared radiation theory, so it is called the blackbody radiation law. The amount of radiation of all actual objects depends on the wavelength of the radiation and the temperature of the object, as well as the type of material that makes up the object, the method of preparation, the thermal process, and the surface state and environmental conditions. Therefore, in order to apply the blackbody radiation law to all practical objects, it is necessary to introduce a proportionality factor, ie, emissivity, related to the material properties and surface state. This coefficient indicates how close the thermal radiation of the actual object is to the blackbody radiation, with values ​​between zero and less than one. According to the law of radiation, as long as the emissivity of the material is known, the infrared radiation characteristics of any object are known. The main factors affecting the emissivity are: material type, surface roughness, physical and chemical structure and material thickness.
When using the infrared radiation thermometer to measure the temperature of the target, first measure the amount of infrared radiation in the range of the target, and then calculate the temperature of the target by the thermometer. The monochromatic thermometer is proportional to the amount of radiation in the band; the two-color thermometer is proportional to the ratio of the amount of radiation in the two bands.
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