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  2. Infrared thermometer - Wikipedia

    en.wikipedia.org/wiki/Infrared_thermometer

    In 2020 when COVID-19 pandemic hit the world, infrared thermometers were used to measure people's temperature and deny them entry to potential transmission sites if they showed signs of fever. Public health authorities such as the FDA in United States published rules to assure accuracy and consistency among the infrared thermometers.

  3. Emissivity - Wikipedia

    en.wikipedia.org/wiki/Emissivity

    The IPCC reports an outgoing thermal radiation flux (OLR) of 239 (237–242) W m-2 and a surface thermal radiation flux (SLR) of 398 (395–400) W m-2, where the parenthesized amounts indicate the 5-95% confidence intervals as of 2015. These values indicate that the atmosphere (with clouds included) reduces Earth's overall emissivity, relative ...

  4. Brightness temperature - Wikipedia

    en.wikipedia.org/wiki/Brightness_temperature

    In pulsars the brightness temperature can reach 10 30 K. [9] For the radiation of a helium–neon laser with a power of 1 mW, a frequency spread Δf = 1 GHz, an output aperture of 1 mm 2, and a beam dispersion half-angle of 0.56 mrad, the brightness temperature would be 1.5 × 10 10 K.

  5. Thermal radiation - Wikipedia

    en.wikipedia.org/wiki/Thermal_radiation

    A kitchen oven, at a temperature about double room temperature on the absolute temperature scale (600 K vs. 300 K) radiates 16 times as much power per unit area. An object at the temperature of the filament in an incandescent light bulb —roughly 3000 K, or 10 times room temperature—radiates 10,000 times as much energy per unit area.

  6. Mean radiant temperature - Wikipedia

    en.wikipedia.org/wiki/Mean_radiant_temperature

    The operative temperature, which is a more functional measure of thermal comfort in a building, is calculated from air temperature, mean radiant temperature and air speed. [6] Maintaining a balance between the operative temperature and the mean radiant temperature can create a more comfortable space. [ 7 ]

  7. Effective temperature - Wikipedia

    en.wikipedia.org/wiki/Effective_temperature

    The effective temperature of the Sun (5778 kelvins) is the temperature a black body of the same size must have to yield the same total emissive power.. The effective temperature of a star is the temperature of a black body with the same luminosity per surface area (F Bol) as the star and is defined according to the Stefan–Boltzmann law F Bol = σT eff 4.

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  9. Effect of radiation on perceived temperature - Wikipedia

    en.wikipedia.org/wiki/Effect_of_radiation_on...

    Thermal radiation emitted by all bodies above absolute zero (-273.15 °C). [3] [4] It differs from other forms of electromagnetic radiation such as x-rays, gamma rays, microwaves that are not related to temperature. Therefore, people constantly radiate their body heat, but at different rates depending on body and surrounding temperatures.