استقرار الجو
Schematic diagram illustrating how optical wavefronts from a distant star may be perturbed by a turbulent layer in the atmosphere. The vertical scale of the wavefronts plotted is highly exaggerated.
استقرار الجو Astronomical seeing هوحالة ثبات الغلاف الجوي واستقراره فحينقد يكون الغلاف الغازى الجوي غير مستقر تبدوالنجوم متلألئة وتقفز الصورة حول التليسكوب ويطلق الفلكيون على هذة الحالة (الاستقرار الجوي الردئ). وحينقد يكون الغلاف الغازى الجوي ثابتا ومستقرا تكون الصورة صافية واضحة المعالم ويطلق الفلكيون على هذة الحالة (الاستقرار الجوى الجيد).
التدابير الفلكية
Simulated negative image showing what a single (point-like) star would look like through a ground-based telescope with a diameter of 2r0. Diffraction makes the image appear blurred. The atmosphere would make the blob move around very rapidly, so that in a long-exposure photograph it would appear more blurred.
Simulated negative image showing what a single (point-like) star would look like through a ground-based telescope with a diameter of 7r0, on the same angular scale as the 2r0 image above. The atmosphere makes the image break up into several blobs (speckles). The speckles move around very rapidly, so that in a long-exposure photograph the star would appear as a single blurred blob.
Simulated negative image showing what a single (point-like) star would look like through a ground-based telescope with a diameter of 20r0. The atmosphere makes the image break up into several blobs (speckles). The speckles move around very rapidly, so that in a long-exposure photograph the star would appear as a single blurred blob.
أنظر ايضا
- Transient lunar phenomenon
- Mirage
- Clear Sky Clock which include a weather forecast of astronomical seeing.
المصادر
- مؤمن, عبد الأمير (2006). قاموس دار الفهم الفلكي. بيروت، لبنان: دار الفهم للملايين.
Much of the above text is taken (with permission) from Lucky Exposures: Diffraction limited astronomical imaging through the atmosphere, by Robert Nigel Tubbs
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BUSCHER, D. F. (1995). "Interferometric seeing measurements on Mt. Wilson: power spectra and outer scales". Applied Optics. 34: 1081–1096. doi:10.1364/AO.34.001081. Unknown parameter
|coauthors=ignored (|author=suggested) (help); Unknown parameter|month=ignored (help) -
COLAVITA, M. M. (1987). "Atmospheric phase measurements with the Mark III stellar interferometer". Applied Optics. 26: 4106–4112. doi:10.1364/AO.26.004106. Unknown parameter
|coauthors=ignored (|author=suggested) (help); Unknown parameter|month=ignored (help) - FRIED, D. L. (1965). "Statistics of a Geometric Representation of Wavefront Distortion". Optical Society of America Journal. 55: 1427–1435. doi:10.1364/JOSA.55.001427.
- KOLMOGOROV, A. N. (1941). "Dissipation of energy in the locally isotropic turbulence". Comptes rendus (Doklady) de l'Académie des Sciences de l'U.R.S.S. 32: 16–18.
- KOLMOGOROV, A. N. (1941). "The local structure of turbulence in incompressible viscous fluid for very large Reynold's numbers". Comptes rendus (Doklady) de l'Académie des Sciences de l'U.R.S.S. 30: 301–305.
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NIGHTINGALE, N. S. (1991). "Interferometric seeing measurements at the La Palma Observatory". Monthly Notices of the Royal Astronomical Society. 251: 155–166. Unknown parameter
|coauthors=ignored (|author=suggested) (help); Unknown parameter|month=ignored (help) -
NOLL, R. J. (1976). "Zernike polynomials and atmospheric turbulence". Optical Society of America Journal. 66: 207–211. doi:10.1364/JOSA.66.000207. Unknown parameter
|month=ignored (help) -
O'BYRNE, J. W. (1988). "Seeing measurements using a shearing interferometer". Publications of the Astronomical Society of the Pacific. 100: 1169–1177. doi:10.1086/132285. Unknown parameter
|month=ignored (help) - TATARSKI, V. I. (1961). Wave Propagation in a Turbulent Medium. McGraw-Hill Books.
وصلات خارجية
- Seeing prediction for every location in Europe, South America and Southern Africa (use myMap Server and click on Astronomy)
- This is an example prediciton
- Seeing forecasts for North America
- Seeing forecasts for Mauna Kea, Hawaii
