Astronomy:Isoplanetic patch
From HandWiki
The isoplanetic 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 or a larger telescope aperture will decrease the size of a patch. Thus, the patch size varies inversely with the Fried parameter and the telescope's angular resolution. 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
References
- ↑ Thompson, A. Richard; Moran, James M.; Swenson, Jr., George W. (November 20, 2008), Interferometry and Synthesis in Radio Astronomy, Wiley, p. 640, ISBN 9783527617852, https://books.google.com/books?id=S99Z7kNBYzAC&pg=PA460.
Further reading
- Birney S, Gonzalez G, Oesper D "observational astronomy" second edition, Cambridge university press, 2006
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