Flick (physics) explained

In optical engineering and telecommunications engineering, the flick is a unit of spectral radiance. One flick corresponds to a spectral radiance of 1 watt per steradian per square centimeter of surface per micrometer of span in wavelength (W·sr−1·cm−2·μm−1). This is equivalent to 1010 watts per steradian per cubic meter (W·sr−1·m−3). In practice, spectral radiance is typically measured in microflicks (10−6 flicks).[1] One microflick is equivalent to 10 kilowatts per steradian per cubic meter (kW·sr−1·m−3).[2]

History

In radio astronomy, the unit flik was coined by a group at Lockheed in Palo Alto, California as a substitute for the SI derived unit W cm−2 sr−1 μm−1, or watts divided by centimeters squared, steradians, and micrometers.[3] While originally used only at Lockheed, many in the radio astronomy field adopted its use.

Notes and References

  1. Web site: Palmer. James M.. The SI system and SI units for Radiometry and photometry. 2012-08-10. https://web.archive.org/web/20120802170633/http://www.optics.arizona.edu/palmer/opti400/suppdocs/bkappndx.pdf. 2012-08-02. dead.
  2. Web site: Rowlett. Russ. How Many? A Dictionary of Units of Measurement. 10 August 2012 . https://web.archive.org/web/20120920072819/https://www.unc.edu/~rowlett/units/dictF.html#flick . 20 September 2012 .
  3. Book: Schlessinger. Infrared Technology Fundamentals, 2nd ed. 1994. CRC Press. 9780824792596. 21.