An ordinary dielectric mirror is made to reflect a single frequency of light.
This ability to tighten or more tightly pack a pulse of light of different wavelengths is important, because some commonly used optical elements naturally disperse a packet of light according to wavelength, a phenomenon known as chromatic dispersion.
A chirped mirror can be designed to compensate for the chromatic dispersion created by other optical elements in a system.
So if a given chirped mirror has 60 layers, light of a specific frequency interacts only with one sixth of the whole stack.
A detailed calculation (references in the external link) shows that the reflectivity of the mirror must also be chirped, which can be done by allotting the half-wavelength unequally across the high- and low-index zones.
In Ti-sapphire lasers employing Kerr-lens modelocking, chirped mirrors are often used as the sole means to compensate group delay variations.
Considering the group velocity this is enough for the 3 m air inside the cavity, for the 3 mm of Ti:sapphire crystal three more mirrors are needed, so that a simple Z-cavity can already be compensated.
In Chirped pulse amplification these mirrors are used to correct residual variations of group delay after a grating compressor is inserted into the system.
The scarab beetle species Chrysina limbata reflects close to 97% of light across the visible wavelength range.