Abstract
It is suggested that the development of the SKA will drastically change the face of radio astronomy in the 21st Century. A FAST-style SKA would admit observations of low contrast features, and would be the best design for studying the `dark ages' of the Universe (x≫ 1) where sub-arcmin total power instruments can usefully be employed. To date there have been no proposals for post-SKA, billion square-metra instruments; we speculate that mobile communication systems can be used. In the very distant future, SKA multi-beam systems could be used to collect signals reflected by Solar system bodies such as the asteroid belt.
Similar content being viewed by others
References
Esepkina, N., Korolkov, D. and Parijskij, Y.: 1973, Radio Telescopes and Radiometers, Nauka 368, Moscow.
Khaikin, S., Kaidanovsky, N., Esepkina, N., Korolkov, D., Parijskij, Y., Stotsky, S., Shakhbazian, Y., and Shivris, O.: 1967, Izvestia GAO N182, 235.
Parijskij, Y.: 1969, Ph.D Thesis, Leningrad
Parijskij, Y.: 1991, Frontiers of VLBI, Universal Academy Press, pp. 221–223.
Parijskij, Y. and Stotskij, A.: 1972, Izvestia GAO 188, 195.
Parijskij, Y. and Tsiboulev, P.: 2000, Astron. Astroph. Tr. 19, 287.
Pinchuk, G., Majorova, E. and Berlisev, I.: 1995, ASP Conf. Series 75, 163.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Parijskij, Y., Chernenkov, V. On post-SKA radio astronomy. Astrophysics and Space Science 278, 199–204 (2001). https://doi.org/10.1023/A:1013119115034
Issue Date:
DOI: https://doi.org/10.1023/A:1013119115034