Introduction to Interferometry

作者: Timothy R. Bedding

DOI: 10.1007/978-3-540-69398-7_1

关键词:

摘要: This tutorial gives a general introduction to optical and infrared interferometry. The observables measured by an interferometer are fringe visibility closure phase, which can then be fitted model or used reconstruct image. In order measure fringes, the path lengths from source detector via different individual apertures must equalized. requires some form of tracking, constrains type observations that feasible has important implications for complexity size resulting

参考文章(5)
Rajaram Nityananda, Comparing Optical and Radio - Quantum Issues Symposium - International Astronomical Union. ,vol. 158, pp. 11- 18 ,(1994) , 10.1007/978-94-011-0880-5_2
F. Roddier, Interferometric imaging in optical astronomy Physics Reports. ,vol. 170, pp. 97- 166 ,(1988) , 10.1016/0370-1573(88)90045-2
Sudhakar Prasad, Implications of light amplification for astronomical imaging Journal of The Optical Society of America A-optics Image Science and Vision. ,vol. 11, pp. 2799- 2803 ,(1994) , 10.1364/JOSAA.11.002799
M. Shao, M. M. Colavita, Long-Baseline Optical and Infrared Stellar Interferometry Annual Review of Astronomy and Astrophysics. ,vol. 30, pp. 457- 498 ,(1992) , 10.1146/ANNUREV.AA.30.090192.002325
N. J. Woolf, High Resolution Imaging From the Ground Annual Review of Astronomy and Astrophysics. ,vol. 20, pp. 367- 398 ,(1982) , 10.1146/ANNUREV.AA.20.090182.002055