Vignetting is light falloff in the corners of an image. There are three types of vignetting: mechanical, optical, and natural. Mechanical Vignetting Mechanical vignetting comes from physical objects that actually block light, such as a dewshield on a telescope that is too long, or lens shade that is too small. Using a camera adapter that is physically too small can also cause vignetting, such as a DSLR in a 1.25 inch focuser. Improperly spaced telecompressors, particularly on Schmidt-Cassegrains can cause vignetting. Undersized secondary mirrors in Newtonians can also cause vignetting.
By far and away, the best way to correct this kind of vignetting is to fix the problem at the source. This kind of vignetting can produce images with literally no signal at all in the corners, so flat-field calibration frames and image processing in software have no data in the vignetted areas to work with.
Optical Vignetting Optical vignetting is caused by the complex arrangement of optical elements in a camera lens where front elements can block part of the off-axis light reaching rear elements. This type of vignetting in common in camera lenses when they are used wide open.
Natural Vignetting Natural vignetting is light falloff in the corners of the frame due to geometrical reasons and the angle at which light reaches the sensor. It can not be fixed by stopping down the lens.
Gradients Whereas vignetting is related to the optical system, gradients are usually caused by real brightness variations in the sky. They are frequently caused by light pollution. They can also be caused by natural atmospheric extinction near the horizon.
Flat-field calibration frames will not fix in-sky gradients.
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