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Flick (physics)

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<sup>−1</sup>·cm<sup>−2</sup>·μm<sup>−1</sup>). This is equivalent to 10<sup>10</sup> watts per steradian per cubic meter (W·sr<sup>−1</sup>·m<sup>−3</sup>). In practice, spectral radiance is typically measured in microflicks (10<sup>−6</sup> flicks). One microflick is equivalent to 10 kilowatts per steradian per cubic meter (kW·sr<sup>−1</sup>·m<sup>−3</sup>).

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<sup>−2</sup> sr<sup>−1</sup> μm<sup>−1</sup>, or watts divided by centimeters squared, steradians, and micrometers. While originally used only at Lockheed, many in the radio astronomy field adopted its use.

References