The Ground Based Imaging of Spacecraft and Inverse Problems

V.P. Aleshin

The Ground Based Imaging of Spacecraft and Inverse Problems

V.P. Aleshin¹

research article Pages: 60-67

¹ Ph. D. (Eng.), Head of Sector of OJC «RPC «PSI» (Moscow)

Keywords: inverse problems speckle interferometry adaptive optics system Stein-s method

Abstract

The analysis of experimental data revealed the following problems: for optical images with quality approaching the diffraction limit, it is necessary to optimize the instrumental component of the system and perform an additional algorithmic processing. When optimizing the instrumental components (speckle interferometry and adaptive optical system) there is a conflict between a systemic errors (accumulation times, band filters, the number of sub-apertures) and the noise component. This conflict can be resolved in the framework of statistical inverse problems

How to cite

Алешин В.П. Наземные системы получения оптических изображений космических аппаратов и обратные задачи // Электромагнитные волны и электронные системы. 2014. № 8. С. 60–67.

References

Altarac, Tallon M., Thiebaut E. and Foy R. Speckle interferometry. Data acquisition and control for the SPID instrument // IEEE Trans. Nucl. Sci. August 1998.V. 45. № 4. P. 2057−2061.
Antoine Labeyrie. Attainment of diffraction limited resolution in large telescopes by Fourier analyzing speckle patterns in star images. Astronomy and Astrophysics. 1970. V. 6. R. 85−87.
Lohmann A.W., Weigelt G., Wiritzer B. Speckle masking in astronomy - Triple correlation theory and applications // Applied Optics. 1983. V. 22. P. 4028−4037.
Lawrence T.W., Goodman D.M., Fitch J.P. Speckle imaging of satellites at the U.S. Air Force Maui Optical Station // Appl. Opt.1992. V. 31. P. 6307−6321.
Aleshin V.P., Balega YU.YU., Grishin E.A., Maksimov A.F., D'yachenko V.V., Malogolovecz E.V., Komarinskij S.L., Novgorodczev D.D., SHargorodskij V.D. Bol'sheaperturny'e teleskopy' v zadachax polucheniya izobrazhenij geostaczionarny'x kosmicheskix apparatov dlya czelej situaczionnoj oczenki kosmicheskoj obstanovki // E'lektromagnitny'e volny' i e'lektronny'e sistemy'. 2011, T. 16. № 3. S. 9−17.
Tixonov A.N., Arsenin V.YA. Metody' resheniya nekorrektny'x zadach. M.: Nauka. 1986. 286 s.
LaurentCavalier. Inverse problems in statistics: Part 1 in book «Inverse Problems and High-Dimensional Estimation» // Lecture Notes in Statistics 203. Springer-Verlag Berlin Heidelberg. 2011. P. 3−96.
He X.D., Torrance K.E, Sillion F.X, Greenberg D.P.A Comprehensive Physical Model for Light Reflection // Computer Graphics. July 1991. V. 25. № 4. P. 175−186.
Hoover B.G.andGamiz V.L. Coherence solution for bidirectional reflectance distributions of surfaces with wavelength-scale statistics // J. Opt. Soc. Am. A. 2006. V. 23. № 2. P. 314−327.
Aleshin V.P., Modelirovanie i vosstanovlenie opticheskix izobrazhenij v okolozemnoj astronomii // Sb. trudov Mezhd. Konf. «Okolozemnaya astronomiya 2013». ISSN 1729‑5459. E'kologicheskij vestnik nauchny'x czentrov CHE'S. 2013. № 4. T. 3. S. 7−12.
Stein C. Inadmissibility of the usual estimator for the mean of a multivariate normal distribution // In Proc. 3th Berkeley Sympos. Math. Statist. and Prob., V. I. Univ. California Press. Berkeley. Calif., 1956. P. 197−206.
Aleksandrov A.B., Inshin P.P. Adaptivnaya korrekcziya fazovy'x iskazhenij polya protyazhennogo istochnika izlucheniya neizvestnoj formy' // Radiotexnika i e'lektronika. 1990. № 6. S. 1225−1228.

[1] Altarac, Tallon M., Thiebaut E. and Foy R. Speckle interferometry. Data acquisition and control for the SPID instrument // IEEE Trans. Nucl. Sci. August 1998.V. 45. № 4. P. 2057−2061.

[2] Antoine Labeyrie. Attainment of diffraction limited resolution in large telescopes by Fourier analyzing speckle patterns in star images. Astronomy and Astrophysics. 1970. V. 6. R. 85−87.

[3] Lohmann A.W., Weigelt G., Wiritzer B. Speckle masking in astronomy - Triple correlation theory and applications // Applied Optics. 1983. V. 22. P. 4028−4037.

[4] Lawrence T.W., Goodman D.M., Fitch J.P. Speckle imaging of satellites at the U.S. Air Force Maui Optical Station // Appl. Opt.1992. V. 31. P. 6307−6321.

[5] Aleshin V.P., Balega YU.YU., Grishin E.A., Maksimov A.F., D'yachenko V.V., Malogolovecz E.V., Komarinskij S.L., Novgorodczev D.D., SHargorodskij V.D. Bol'sheaperturny'e teleskopy' v zadachax polucheniya izobrazhenij geostaczionarny'x kosmicheskix apparatov dlya czelej situaczionnoj oczenki kosmicheskoj obstanovki // E'lektromagnitny'e volny' i e'lektronny'e sistemy'. 2011, T. 16. № 3. S. 9−17.

[6] Tixonov A.N., Arsenin V.YA. Metody' resheniya nekorrektny'x zadach. M.: Nauka. 1986. 286 s.

[7] LaurentCavalier. Inverse problems in statistics: Part 1 in book «Inverse Problems and High-Dimensional Estimation» // Lecture Notes in Statistics 203. Springer-Verlag Berlin Heidelberg. 2011. P. 3−96.

[8] He X.D., Torrance K.E, Sillion F.X, Greenberg D.P.A Comprehensive Physical Model for Light Reflection // Computer Graphics. July 1991. V. 25. № 4. P. 175−186.

[9] Hoover B.G.andGamiz V.L. Coherence solution for bidirectional reflectance distributions of surfaces with wavelength-scale statistics // J. Opt. Soc. Am. A. 2006. V. 23. № 2. P. 314−327.

[10] Aleshin V.P., Modelirovanie i vosstanovlenie opticheskix izobrazhenij v okolozemnoj astronomii // Sb. trudov Mezhd. Konf. «Okolozemnaya astronomiya 2013». ISSN 1729‑5459. E'kologicheskij vestnik nauchny'x czentrov CHE'S. 2013. № 4. T. 3. S. 7−12.

[11] Stein C. Inadmissibility of the usual estimator for the mean of a multivariate normal distribution // In Proc. 3th Berkeley Sympos. Math. Statist. and Prob., V. I. Univ. California Press. Berkeley. Calif., 1956. P. 197−206.

[12] Aleksandrov A.B., Inshin P.P. Adaptivnaya korrekcziya fazovy'x iskazhenij polya protyazhennogo istochnika izlucheniya neizvestnoj formy' // Radiotexnika i e'lektronika. 1990. № 6. S. 1225−1228.

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