Isoplanatic patch
The isoplanatic patch is defined as an arbitrary area of the sky over which the path length of incoming electromagnetic waves (such as light or radio waves) only varies by a relatively small amount relative to their wavelength.[1] Typically this area is measured by angular size. Poor seeing, a larger telescope aperture, or a higher altitude for the dominant turbulent layers, will all decrease the size of a patch. Thus, the patch size decreases with increased atmospheric turbulent activity. In addition, the isoplanatic patch size is proportional to the Fried parameter and the telescope's angular resolution.[2][3][4][5][6] In order to correct for atmospheric distortion, telescopes fitted with adaptive optics use a bright light source such as a laser to identify the properties of a patch in the area of interest.
See also
[edit]References
[edit]- ↑ Thompson, A. Richard; Moran, James M.; Swenson, Jr., George W. (November 20, 2008), Interferometry and Synthesis in Radio Astronomy, Wiley, p. 640, ISBN 9783527617852.
- ↑ Tatarskiĭ, V. I.; Silverman, Richard A. (2016). Wave propagation in a turbulent medium. Dover books on physics. Mineola, New York: Dover Publications, Inc. ISBN 978-0-486-81029-4.
- ↑ Fried, D. L. (1965-11-01). "Statistics of a Geometric Representation of Wavefront Distortion". JOSA. 55 (11): 1427–1435. doi:10.1364/JOSA.55.001427.
- ↑ Noll, Robert J. (1976-03-01). "Zernike polynomials and atmospheric turbulence*". JOSA. 66 (3): 207–211. doi:10.1364/JOSA.66.000207.
- ↑ Hardy, John W. (1998). Adaptive optics for astronomical telescopes. Oxford series in optical and imaging sciences. New York: Oxford University Press. ISBN 978-0-19-509019-2.
- ↑ Roddier, F. (1981), "V The Effects of Atmospheric Turbulence in Optical Astronomy", Progress in Optics, vol. 19, Elsevier, pp. 281–376, doi:10.1016/s0079-6638(08)70204-x, ISBN 978-0-444-85444-5, retrieved 2026-04-01
Further reading
[edit]- Birney S, Gonzalez G, Oesper D "observational astronomy" second edition, Cambridge university press, 2006
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