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The optical system
To fully exploit the detector performance, a very fast custom designed
optical system would need to be designed for ALIS. Ideally this would
include a set of replaceable front-lenses, preferably mounted on a
rotating disc in front of the filter-wheel, resulting in a remotely
selectable field-of-view. As narrow-band interference filters are to
be used, a telecentric lens system is required to have nearly parallel
rays through the filters (see Section 3.5 for details).
It was realised early that the requirement of changeable field-of-view
had to be dropped due to reliability as well as budgetary constraints.
Therefore, given the station separation, a field-of-view of approximately
-
would be the best compromise (See also Figure 2.3 in
Chapter 2). Following quotations from various optical manufacturers
in the field, it was also quickly realised that the cost of
one custom designed optical system would quickly exceed the
entire project budget. Therefore a commercial telecentric optical
system, frequently used in this field, was selected.
This system consists of a replaceable front-objective (A), two
plano-convex telecentric lens-elements (B), a filter holder (C,
replaced by the IRF-designed filter-wheel Section 3.5.1), a
field-lens (D), two close-up lenses (E,F) and a camera objective(G)
(Figure 3.7).
As discussed in Section 2.1.1, the station separation baseline
was selected for a moderate field of view of about
-90.
For the first four imagers, the 45 mm front-objective resulted in a
diagonal field-of-view of about
. Experiences gained from
tomographic reconstruction using images from these four systems
resulted in a decision to slightly widen the field-of-view for the
next two imagers. Consequently these were equipped with a 35 mm
front-objective, giving a diagonal field-of-view of about
.
According to vendor specifications [Keo Consultants, 1997; Keo Consultants, 1994], the
f-number setting on the front lens, , will
determine image brightness on the CCD, as well as the
maximum ray-angle through the
filter,
, given by the following approximate
formula:
|
(3.44) |
A photograph of the six ALIS imagers appears in Figure 3.6.
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copyright Urban Brändström