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Monochrome sensors would produce better results but they need a filter wheel and a longer post-processing procedure. Overall colour sensors are better for small telescopes and do not require a long post-processing as there is only one channel. In same cases such as during the Mars opposition in 2018 where all planetary details were obfuscated by a dust storm, imaging in the IR channel was the only way to reveal some details. Also, monochromatic sensors have the advantage to be highly sensitive in the infrared spectrum and many planets reveal the majority of their details in this spectrum interval. Monochromatic cameras need coloured filters and a filter wheel but here the atmospheric dispersion can be corrected in post processing by aligning the colour channels. Therefore this accessory could be quite complicated to use, especially in Newton telescopes. The atmospheric dispersion corrector however generates a chromatic dispersion equal and opposite to the atmospheric dispersion, nulling the effect. Colour cameras will show a red and blue rim on the opposite side of the objects and it is almost impossible to correct it during post processing. In fact, for small pixel/arc second ratios in the order of 0.25"-0.1"/pixel, the atmospheric dispersion could be relevant with objects below 65° of elevation.
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How to choose between a camera with a colour or monochrome sensor? For planetary cameras this decision is determined by the pixel scale and the elevation of the object above the horizon. So to get a sufficient number of frames, you will need a fast computer equipped with USB3.0 port and SSD drivers. For certain planets with a fast rotation such as Jupiter and Saturn, the video captured should not be longer than 30-60 seconds. For bright objects like planets, the moon and the sun, a small uncooled sensor is all you need to capture a short video of the object and then process the frames with the technique of the lucky imaging. To choose the right camera can be complicated so the two tabs below will assist you to get an easy insight of all the ZWO camera features at first glance.Īs you can see, there are two "families" of sensors: cooled cameras for deep Sky Objects (DSO) and uncooled for planetary imaging.
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Monochrome, RGB, DSO camera, planetary camera, cooled, uncooled these are only some of the different features of the ZWO cameras.