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Gonsalves, R. A. (1982). Phase retrieval and diversity in adaptive optics, Opt. , Vol. 21: 829–832. Harding, K. G. & Harris, J. S. (1983). Projection moiré interferometer for vibration analysis, Appl. , Vol. 22: 856–861. Herrmann, J. (1980). Least-squares wavefront errors of minimum norm, J. Opt. Soc. , Vol. 70: 28–35. Hunt, B. R. (1979). Matrix formulation of the reconstruction of phase values from phase differences, J. Opt. Soc. , Vol. 69: 393–399. ICO Newsletter, (2009). ICO Newsletter, April 2009, Number 79.
39: 5415–5425. Walker, C. A. (2004). Handbook of moiré measurement, Institute of Physics, London. Part 2 Imaging and Laser Propagation Systems 3 Direct Imaging of Extra-Solar Planets – Homogeneous Comparison of Detected Planets and Candidates Ralph Neuhäuser and Tobias Schmidt Astrophysical Institute and University Observatory, Friedrich Schiller University Jena, Jena Germany 1. Introduction Planets orbiting stars other than the Sun are called extra-solar planets or exo-planets. Since about 1989, several hundred such objects were detected using various techniques.
36 14 Topics in Adaptive Optics Will-be-set-by-IN-TECH Fig. 12. Three virtual traces are produced between two adjacent bright and dark traces by using their intensities and locations. Algorithmically, this involves the calculation of a surface by an integration-like process. The reconstruction problem can be expressed in a matrix-algebra framework. The unknowns, a vector Φ of N phase values over a grid, must be calculated from the data, from a measurement vector S of M elements of wavefront gradients in two directions.