Performance of Adaptive Optics for Large Apertures, is a set of functions and procedures written in IDL (version 5.4 at least) for calculating the performances of an AO system installed at the focus of an astronomical telescope.
Unlike most of AO simulation packages, the code is not a Monte-Carlo one. It relies on an analytic expression of the power spectrum of the corrected phase, and its relation with the AO Optical Transfer Function (OTF). The advantage over Monte-Carlo codes is the huge decrease in computation time (few minutes instead of hours). The drawback is that it is difficult if impossible to simulate the ``second order'' behavior of a real AO system (misalignments, imperfect reconstruction matrix, imperfect mirror influence functions,...).
So, the assumption that makes the analytical approach possible is that the AO system is perfect, i.e. all the components are left with their own limitations, but without any manufacturing/assembling/software errors. As a consequence, PAOLA is not a tool for studying the fine details of an AO system design. Rather, it has been developed as a toll for assessing AO performance on a given site and telescope, mainly to do science cases (but not limited to).
4 modes are available: diffraction limited, seeing limited, classical AO correction, and Ground Layer AO. The WFS is a Shack-Hartmann sensor. The deformable mirror can be conjugated to any height in the atmosphere.
As a summary, PAOLA helps the user to answer the question : if a perfect AO system is installed on a certain telescope at a certain observation site, what performances can we get on the sky ? (Strehl, FWHM, limit magnitude, 50% energy radius ...)
The input parameters are:
The toolbox is given as a "tar.gz" archive file, and includes:
Platform: IDL release 5.4 and after (no GUI)
Please write me at: email@example.com (Observatory of Leiden, Netherlands) to get a copy of the PAOLA package. PAOLA user manual can be downloaded at http://www.strw.leidenuniv.nl/~jolissaint/
|Last Modified: Dec 5, 2008|
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