Skip to main content
Log in

On the possibility of obtaining strip distributions of radio brightness by the minimal phase method

  • Published:
Astrophysics Aims and scope

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Literature Cited

  1. C. van Schooneveld (ed.), Image Formation from Coherence Functions in Astronomy (Proc. IAU Colloquium No. 49 on the Formation of Images from Spatial Coherence Functions, Groningen, 1978), Astrophys. and Space Sci. Libr., Vol. 76, Dordrecht (1979).

  2. A. A., Gal'chenko, I. F. Malov, L. F. Mogil'nitskaya, and V. A. Frolov, Kratk. Soobshch. Fiz.,2, 8 24 (1982); 9, 23 (1982);3 11 (1984).

    Google Scholar 

  3. I. G. Kosarev, I. F. Malov, and V. A. Frolov, Preprint No. 90 [in Russian], P. N. Lebedev Physics Institute, Moscow (1980); Kratk. Soobshch. Fiz., No. 7, 15 (1982).

  4. E. E. Fomalont, Astrophys. J. Suppl. Ser.,138, 15, 203 (1968).

    Google Scholar 

  5. J. A. Hogbom and I. Carlsson, Astron. Astrophys.,34, 341 (1974).

    Google Scholar 

  6. S. F. Burch, Mon. Not. R. Astron. Soc.,181, 599 (1977).

    Google Scholar 

  7. G. K. Meley and G. C. Perola, Astron. Astrophys.,45, 223 (1975).

    Google Scholar 

  8. Yu. A. Evsikov and V. V. Chapurskii, Transformation of Random Processes in Electronic Devices [in Russian], Vysshaya Shkola, Moscow (1977).

    Google Scholar 

  9. Yu. M. Bruck and L. G. Sodin, Opt. Commun.,30, 304 (1979).

    Google Scholar 

  10. R. H. T. Bates, Optik,61, 247 (1982).

    Google Scholar 

Download references

Authors

Additional information

P. N. Lebedev Physics Institute, USSR Academy of Sciences. Translated from Astrofizika, Vol. 26, No. 2, pp. 351–361, March–April, 1987.

Rights and permissions

Reprints and permissions

About this article

Cite this article

Malov, I.F., Frolov, V.A. On the possibility of obtaining strip distributions of radio brightness by the minimal phase method. Astrophysics 26, 213–220 (1987). https://doi.org/10.1007/BF01005561

Download citation

  • Received:

  • Accepted:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF01005561

Keywords

Navigation