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On the potential of the total phase accumulation method in object observations through earth’s atmosphere

Рубрика: 

Manuscript submitted 24.01.2020
Radiofiz. elektron. 2020, 25(3): 60-67
Full text  (PDF)

References: 

 

 

1. Timofeev, Yu.M., Vasilyev A.V., 2003. Theoretical basis of atmosphere optics. Moscow: Nauka Publ. (in Russian).
 
2. Kornienko, Yu.V., 2008. Image processing in IRE NAS of Ukraine. In: V.M.Yakovenko, ed. 2008. Radiofizika i elektronika. Kharkov: IRE NAS of Ukraine Publ. 13(spec. iss.), pp. 423-445 (in Russian).
 
3. Labeyrie, A., 1970. Attainment of diffraction limited resolution in large telescopes by Fourier analysing speckle patterns in star images. Astron. astrophys., 6(1), pp. 85-87.
 
4. Sodin, L.G., 1976. Prospects for achieving the diffraction limit of telescope resolution in a turbulent atmosphere. Sov. Astron. Lett., 2(6), pp. 220-222.
 
5. Kornienko, Yu.V., Skuratovskiy, S.I., 2011. Fourier-component phase accumulation in observation of an object through a turbulent atmosphere: I. Kinematics Phys. Celestial Bodies, 27(6), pp. 304-310 (in Russian). DOI: https://doi.org/10.3103/S0884591311060043
 
6. Kornienko, Yu.V., Skuratovskiy, S.I., 2010. About the reconstruction of the undistorted image of an object by a series of its images distorted by a medium with random inhomogeneities of the refractive index. Dopov. Nac. akad. nauk Ukr., 2, pp. 83-89 (in Russian).
 
7. Kornienko, Yu.V., Skuratovskiy, S.I., 2012. Mechanism of information degradation in observations through a randomly inhomogeneous medium. Radiophysics and radioastronomy, 17(1), pp. 39-48 (in Russian).
 
8. Kornienko, Yu.V., Skuratovskiy, S.I., 2012. Fourier-component phase accumulation in observation of an object through a turbulent atmosphere: II. Kinematics Phys. Celestial Bodies, 28(2), pp. 77-84 (in Russian). DOI: https://doi.org/10.3103/S0884591312020043
 
9. Hadamard, J., 1902. Sur les Problèmes aux Dérivées Partielles et Leur Signification Physique. Princeton Université Bulletin, 13, p. 82.