The Order of Image Processing
The 100 Best Targets for AstrophotographyPatrick Moore's Practical Astronomy Series(2009)
摘要
The first step in processing your exposures should be the dark frame subtraction and flat-field correction. Some programs,
like CCDSoft, call this process image reduction, whereas other programs, like Maxim DL, call this image calibration. Most
image processing programs have a routine to perform this efficiently on all of your images. Make sure that the dark frames
match the temperature, the exposure time, and the bin mode of your light exposures. Also, confirm that your flat fields match
the optical system of your light exposures. See the section on “Combining Images” for suggestions on dark frame and flat-field
combining. Your calibrated images should be saved in a different folder from your raw images. This way, if your images are
not calibrated correctly, you can repeat the process on your raw images. The calibrated image should be virtually free of
the scattered hot pixels that plague the raw image. Vignetting and dust shadows should be improved substantially.
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