VIA Technologies EPIA SN-Series Specifications Page 18

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Background
6
that best fits the implementation of a system for the acquisition of satellite images is a
CCD (although CMOS based devices are currently the best choice in order to reduce
power consumption). This stems mainly from the high sensitivity of silicon at
wavelengths of less than 1.1 μm, ideal if one is interested in capturing images in the
visible spectrum (0.4-0.7 μm) or nIR (near infrared).
Among all manufacturers taken into consideration, the selected device is a DALSA
FTF 2020M which is a squared full frame CCD with 2048x2048 pixels (12 µm side) with
100% optical fill factor and a considerably high dynamic range (which represents an
equivalent measure for the contrast the device is able to achieve). As stated by the final M
in the product code the sensor is monochrome with no reported Bayern filter in front of
the sensible area.
Figure 1: Dalsa FTF2020M sensor
Figure 2: Dalsa demoboard with FTF2020M sensor
support
Typically, in digital still cameras, multispectral capabilities are achieved by using
mechanical wheels that rotate optical filters in front of the sensor. To avoid moving parts
inside the instrument, which could compromise the success of the entire mission, a LCD
continuous tuneable filter will be placed in-between the sensor and the optics, to provide
better multispectral capabilities than the mechanical wheel. Multispectral images will be
generated overlapping single band images and creating arrays with a maximum of 10
spectral bands. The time the filter takes to switch between one wavelength to another is
typically 50 to 150 ms depending on the value of λ. AMSC will be one of the first
spaceborne instrument based on the use of a tunable filter.
CRI (Cambridge Research Inc, manufacturer of the filter) has already tested the
correct operation of the filter in vacuum conditions; it was found that the filter did not
experience mechanical damages or deformations during the test and that the optical
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