CTA will observe the sky in the gamma-ray energy range. When this very energetic electromagnetic radiation hits the Earth's atmosphere, the photons interact with air molecules and so-called electromagnetic showers are generated. Because of their very high energies, these secondary particles can move faster than the speed of light in air, which is 0.03 percent slower than the speed of light in vacuum.
What happens then is similar to what can be observed when the speed of airplanes exceeds the speed of sound: a shock wave is generated, which produces the well-known sonic boom. For particle showers, the equivalent effect is the Cherenkov radiation, a flash of bluish light lasting for some billions of a second, too short for the human eye to detect.
However, the mirrors of CTA and the high speed cameras can observe this radiation. Even though it occurs relatively rarely, the unprecendented area covered by CTA is expected to increase the number of known sources (about 150) by a factor of 10.