Fig. 6From: Design of a Mars atmosphere simulation chamber and testing a Raman Laser Spectrometer (RLS) under conditions pertinent to Mars rover missionsTemperature-induced shift of the observed white light emission in 3rd order on the CCD at 283, 278 and 253 K. The X axis shows the column number of CCD pixels; the Y axis shows the row number of a part of the CCD pixels, vertically expanded for clarity. The pixel size is 13.5 μm squareBack to article page