Skip to main content
Log in

Interstellar scintillations and nanoarcsecond resolution in radio astronomy

  • Published:
Astronomy Reports Aims and scope Submit manuscript

Abstract

Interstellar turbulent plasma can be considered to be a radio astronomy antenna—an interstellar diffraction grating, with an aperture size roughly equal to the scattering-disk radius, R sc = z eff θ sc ≈ 1 AU (where z eff is the effective distance and θ sc the scattering angle). The angular resolution of this interstellar diffraction grating is of the order of ϕ dif = 1/(k R sc ). A single ground-based radio telescope can be used as a receiver for the interstellar diffraction grating. The grating’s parameters can be obtained only from observations on a system of interferometers with an angular resolution comparable to the scattering angle θ sc . The range of baselines necessary to determine the parameters of the grating is close that of the Earth-space RadioAstron interferometer.

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.

Similar content being viewed by others

References

  1. L. T. Little and A. Hewish, Mon. Not. R. Astron. Soc. 134, 221 (1966).

    ADS  Google Scholar 

  2. M.H. Cohen, E.J. Gunderman, H.E. Hardebeck, and L.E. Sharp, Astrophys. J. 147, 449 (1967).

    Article  ADS  Google Scholar 

  3. A. Wolsczan and J.M. Cordes, Astrophys. J. 320, L35 (1987).

    Article  ADS  Google Scholar 

  4. T. V. Smirnova and V. I. Shishov, Pis’ma Astron. Zh. 15, 443 (1989) [Sov. Astron. Lett. 15, 191 (1989)].

    ADS  Google Scholar 

  5. T. V. Smirnova, V. I. Shishov, and V. M. Malofeev, Astrophys. J. 462, 289 (1996).

    Article  ADS  Google Scholar 

  6. C. Gwinn, M. J. Ojeda, M. C. Britton, et al., Astrophys. J. 483, L53 (1997).

    Article  ADS  Google Scholar 

  7. J.M. Cordes, arXiv: astro-ph/0007231 (2000).

  8. A. M. Prokhorov, F. V. Bunkin, K. S. Gochelashvili, and V. I. Shishov, Usp. Fiz. Nauk 114, 415 (1974) [Sov. Phys. Usp. 17, 826 (1974)].

    Google Scholar 

  9. V. I. Shishov and T. V. Smirnova, Astron. Zh. 79, 810 (2002) [Astron. Rep. 46, 731 (2002)].

    Google Scholar 

  10. V. I. Shishov, T. V. Smirnova, W. Sieber, et al., Astron. Astrophys. 404, 557 (2003).

    Google Scholar 

  11. T.V. Smirnova, V.I. Shishov, W. Sieber, et al., Astron. Astrophys. 455, 195 (2006).

    Article  ADS  Google Scholar 

  12. T. V. Smirnova, C. R. Gwinn, and V. I. Shishov, Astron. Astrophys. 453, 601 (2006).

    Article  ADS  Google Scholar 

  13. T.V. Smirnova and V. I. Shishov, Astron. Zh. 85, 818 (2008) [Astron. Rep. 52, 736 (2008)].

    Google Scholar 

  14. V. E. Ostashev and V. I. Shishov, Izv. Vyssh. Uchebn. Zaved., Radiofiz. 20, 833 (1977).

    Google Scholar 

  15. T. V. Smirnova, V. I. Shishov, and D. R. Stinebring, Astron. Zh. 75, 866 (1998) [Astron. Rep. 42, 766 (1998)].

    Google Scholar 

  16. N. D. R. Bhat, Y. Gupta, and A. P. Rao, Astrophys. J. 500, 262 (1998).

    Article  ADS  Google Scholar 

  17. N. S. Kardashev, Experim. Astron. 7, 329 (1997).

    Article  ADS  Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Additional information

Original Russian Text © V.I. Shishov, 2010, published in Astronomicheskiĭ Zhurnal, 2010, Vol. 87, No. 8, pp. 789–794.

Rights and permissions

Reprints and permissions

About this article

Cite this article

Shishov, V.I. Interstellar scintillations and nanoarcsecond resolution in radio astronomy. Astron. Rep. 54, 724–729 (2010). https://doi.org/10.1134/S1063772910080056

Download citation

  • Received:

  • Accepted:

  • Published:

  • Issue Date:

  • DOI: https://doi.org/10.1134/S1063772910080056

Keywords

Navigation