VIA Technologies EPIA SN-Series Specifications Page 16

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Background
4
Chapter 2. Background
In this Chapter a brief description of all the preparatory activities carried out during
the three years PhD course is reported, emphasizing those that led to the definition of the
subject of this work.
In Section 2.1 the AMSC project is discussed in detail; this study allowed to deepen
themes such as the development of optical systems for remote sensing purposes. Digital
sensor technologies, their electronic integration and optical layouting using CAO
(Computer Aided Optics) software are only part of the background knowledge acquired in
the course of this work. The AMSC project aimed to the development of a digital
multispectral camera equipped with an innovative tunable LCD filter ended with the need
to find a suitable platform to carry out functional tests on the prototype model, because of
the inherent difficulties in reproducing the same operational conditions.
Sections 2.2 and 2.3 describe two projects directly related to the previous one because
they are possible candidates for an image based attitude determination sensor that will be
utilized onboard the ALMASat-EO mission. STARS is a very accurate three axial
standalone attitude determination sensor that processes Earth image sequences in the
visible spectrum. STARS involves the use of an high frame rate detector which is
significantly different from that used on the AMSC and many image process algorithms
must be run in real time mode. LCCES is also an Earth sensor but working in the Thermal
Infrared spectrum. This project has much in common with both STARS and AMSC
because of the use of an image based sensing device and the development of custom
optics. This study is built around a new detector type, the uncooled microbolometer,
which allows the development of small size and low power systems without substantial
performances loss. Optics are also characterized by the use of Germanium lens which
have its own transmission window in the TIR spectrum.
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