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>âÂÂ1</sup>÷cm<sup>âÂÂ2</sup>֟m<sup>âÂÂ1</sup>). This is equivalent to 10<sup>10</sup> watts per steradian per cubic meter (W÷sr<sup>âÂÂ1</sup>÷m<sup>âÂÂ3</sup>). In practice, spectral radiance is typically measured in microflicks (10<sup>âÂÂ6</sup> flicks). One microflick is equivalent to 10 kilowatts per steradian per cubic meter (kW÷sr<sup>âÂÂ1</sup>÷m<sup>âÂÂ3</sup>).
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>âÂÂ2</sup> sr<sup>âÂÂ1</sup> üm<sup>âÂÂ1</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.