{"id":1062,"date":"2014-01-08T22:25:19","date_gmt":"2014-01-08T20:25:19","guid":{"rendered":"https:\/\/www.planetary-astronomy-and-imaging.com\/?p=1062"},"modified":"2018-10-17T09:40:56","modified_gmt":"2018-10-17T07:40:56","slug":"use-true-green-filter","status":"publish","type":"post","link":"https:\/\/www.planetary-astronomy-and-imaging.com\/en\/use-true-green-filter\/","title":{"rendered":"Use a true green filter for your images"},"content":{"rendered":"
Among the different techniques of imaging that we saw over the years, there was the use of a “synthetic” green image. Here is why it is less interesting than a true green image. This technique is quite outdated now and has never been really widely used, but this is a good opportunity to take a closer look at how color rendition is working.<\/strong><\/em><\/p>\n Many years ago, some imagers were using a purely computer-generated green frame by averaging red and blue frames. It is very simple to do: in any software, add R with B and divide by 2 the result. This produces a synthesized G frame that we’re going to call “sG” and the final color image is “RsGB”.<\/p>\n The advantage of this method was clear: by using only R and B, it was possible to get more raw frames during the same total time for those bands that are the most important. During ages were the CCD cameras were much slower than today, it could be welcomed to handle the rotation of planets.<\/p>\nA synthetic green image, why?<\/strong><\/span><\/h2>\n