Handbook for the SXVR-H694
Issue 1 March 2012
16
press a computer key. The images will be saved in FITs format with sequential names
such as ‘Img23, Img24….’ and will be found in the ‘Autosave’ directory (or a sub-
directory of Autosave, set up in the program defaults menu).
The exposure time needed for good planetary images is such that the image histogram
has a peak value at around 200 and does not extend much above 220 (Ignore the
major peak near zero, due to the dark background). If you use too short an exposure
time, the image noise level will be increased, and if too long a time is used you will
saturate the highlights and cause white patches on the image. With the recommended
focal length, Jupiter and Mars will both need an exposure time of between 0.1 and 1
seconds and Saturn will need between 0.5 and 2 seconds.
Processing a planetary image:
Planetary images have one major advantage over deep sky images, when you come to
process them – they are MUCH brighter, with a correspondingly better signal to noise
ratio. This means that aggressive sharpening filters may be used without making the
result look very noisy and so some of the effects of poor seeing can be neutralised.
A raw image
Try applying an ‘Unsharp Mask’ filter with a radius of 5 and a power of 5. This will
greatly increase the visibility of any detail on the planet, but the optimum radius and
power will have to be determined by experiment.
