Future Upgrades and Conclusions Sample Clauses

Future Upgrades and Conclusions. In this section we have used optical models of the Cardiff University testbed to analyse the effects of long-wavelength operation, non-idealities such as mis-alignments aberrations and truncations and the use of a spherical collimating mirror to simulate astronomical sources. The collimating mirror is specific to laboratory testbeds but the other analyses should be useful when considering the design of long-wavelength interferometers for space in general. The spreading of beams at the longest of the testbed wavelengths gives rise to significant truncation and loss in power. When the full band is considered the effect on the recovered spectra is small, though wavelength-dependent. It should be considered in a real instrument when a detailed spectral analysis of sources in required. Aberrations, unless they are of an amplitude of about an order of magnitude smaller than the wavelength could on the other hand cause a significant reduction in fringe visibility of the testbed. Since the distances between optical components in the testbed can be either in the near- of far-field of beams, depending on which end of the band is being considered, it can be difficult to predict trends with wavelength without doing a proper analysis. The optical modelling has shown that accurate alignment of the components, in particular the roof-mirrors, is very important at the long baselines. Replacing the spherical mirror in the collimator with a parabolic on would also make it easier to recover fringes at long baselines.
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