Advanced Image Calibration
It
is a normal run of data collection: You've acquired 600
images with your CCD camera. But there's something ominous yet to be done
before your data are really useful: quantitative image calibration. Note:
This Brief describes luminance calibration; spatial calibration is a
different topic. Luminance calibration involves correction of instrumental signatures and effects like
bias, dark current, and flat field corrections, removal of defective pixels and
artifacts, and other tasks. And add to this complexity the fact that
different data sources often require different calibration steps and
strategies, and that some data sets require master calibration frames to be
created each time. With all the details and endless variations, quantitative
image calibration once boiled down to these options: 1) Perform hours of
tedious, error-prone work, or 2) Create a script. Now, Mira breaks through this
complexity by reducing it to a matter of checkboxes, buttons, and re-usable
profiles. This feature is included in the Mira MX, Pro, and AP platforms. Of
course, you also may create a script for processing that is too specialized
or complex to be done using the Image Calibration package.