Test-bed overview Sample Clauses

Test-bed overview. The FIRI instrument is designed to operate over a band spanning from 25 to 400 µm, split into 4 channels using dichroic filters (See FIRI deliverable 1.2). Clearly the short- wavelength channel is the most challenging from the point of view of optical and alignment tolerances. The layout of the test-bed is shown in Figure 2. A water-cooled mercury-arc lamp which has an equivalent blackbody-like Raleigh Jeans emission in the FIR is used as a source to mimic an astronomical object located at infinity. The source is collimated using a section of the BLAST telescope (Xxxxxxx et al. 2008, SM in the Figure 2 diagram). This is a gold plated 2m spherical mirror with a 2-m focal length. The mirror is made of 6 carbon fibre sections and one of these sections is used as collimator in the test-bed. The plate scale at the collimator focal plane is 1.64 arcmin/mm. The aperture of the source can be adjusted, up to a maximum diameter of 10mm, the diameter of the mercury arc lamp. To create a scene, such as a single slit, a double slits or three slits, aperture plates can be placed directly at the focus of the collimator, in front the mercury arc lamp. As the maximum interferometer baseline achievable is 400 mm, the maximum achievable spatial resolution is about 8.5 arcmin at 1 mm wavelength or 3 arcmin at 350μm. So a 1mm wide slit (1.72 arcmin source) will not be resolved but two slits 9mm apart will produce fringes at the detector for wavelengths ≤ 1mm. At 25μm the optical resolving power achievable will be 8 times larger – so more complex scenes are possible.
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