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  2. 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.

  3. Operative temperature - Wikipedia

    en.wikipedia.org/wiki/Operative_temperature

    Operative temperature is used in heat transfer and thermal comfort analysis in transportation and buildings. [10] Most psychrometric charts used in HVAC design only show the dry bulb temperature on the x-axis(abscissa), however, it is the operative temperature which is specified on the x-axis of the psychrometric chart illustrated in ANSI/ASHRAE Standard 55 – Thermal Environmental Conditions ...

  4. ASHRAE 55 - Wikipedia

    en.wikipedia.org/wiki/ASHRAE_55

    For this model the standard provides a graph of acceptable indoor temperature limits at prevailing mean outdoor temperatures (a mean of the daily mean outdoor temperatures of the previous 7–30 days). An accompanying table lists provisions for higher operative temperatures at air speeds above 0.3 m/s (59 ft/min) and up to 1.2 m/s (240 ft/min).

  5. Black-body radiation - Wikipedia

    en.wikipedia.org/wiki/Black-body_radiation

    This temperature, calculated for the case of the planet acting as a black body by setting =, is known as the effective temperature. The actual temperature of the planet will likely be different, depending on its surface and atmospheric properties.

  6. Color temperature - Wikipedia

    en.wikipedia.org/wiki/Color_temperature

    For example, the color temperature of an A0V star is about 15000 K compared to an effective temperature of about 9500 K. [27] For most applications in astronomy (e.g., to place a star on the HR diagram or to determine the temperature of a model flux fitting an observed spectrum) the effective temperature is the quantity of interest. Various ...

  7. Brightness temperature - Wikipedia

    en.wikipedia.org/wiki/Brightness_temperature

    Brightness temperature or radiance temperature is a measure of the intensity of electromagnetic energy coming from a source. [1] In particular, it is the temperature at which a black body would have to be in order to duplicate the observed intensity of a grey body object at a frequency ν {\displaystyle \nu } . [ 2 ]

  8. NTU method - Wikipedia

    en.wikipedia.org/wiki/NTU_Method

    The other fluid would change temperature more slowly along the heat exchanger length. The method, at this point, is concerned only with the fluid undergoing the maximum temperature change. The effectiveness of the heat exchanger ( ϵ {\displaystyle \epsilon } ) , is the ratio between the actual heat transfer rate and the maximum possible heat ...

  9. Temperature - Wikipedia

    en.wikipedia.org/wiki/Temperature

    Temperature is a physical ... A more physically informative version of such a law views empirical temperature as a chart on a hotness manifold. ... D Effective ...