Skip to main content
Log in

New estimate of the altitude of local sources of the slowly varying component of solar radio emission at the 3.2 cm wavelength

  • Published:
Radiophysics and Quantum Electronics 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. V. N. Iskhanova, Izv. GAO, No. 164, 62 (1960).

    Google Scholar 

  2. V. N. Iskhanova, Izv. GAO, No. 162, 29 (1958).

    Google Scholar 

  3. V. V. Vitkevich, Transactions of the Fifth Conference on Problems of Cosmogony [in Russian], Izd. AN SSSR, Moscow (1956), p. 149.

    Google Scholar 

  4. G. Swarup and T. Kakinuma, Astrophys. J.,136, 975 (1962).

    Google Scholar 

  5. G. Swarup et al., Astrophys. J.,137, No. 4, 1251 (1963).

    Google Scholar 

  6. A. P. Molchanov, N. L. Kaidanovskii, and N. G. Peterova, Solnechnye Dannye, No. 3, 68 (1971).

    Google Scholar 

  7. D. V. Korol'kov, N. S. Soboleva, and G. B. Gel'freikh, Izv. GAO, No. 164, 81 (1960).

    Google Scholar 

  8. S. É. Khaikin, N. L. Kaidanovskii, N. A. Esepkina, and O. N. Shivris, Izv. GAO, No. 164, 3 (1960).

    Google Scholar 

  9. G. B. Gel'freikh, Sh. B. Akhmedov, V. N. Borovik, V. Ya. Gol'nev, A. N. Korzhavin, V. G. Nagnibeda, and N. G. Peterova, Izv. GAO, No. 185, 167 (1970).

    Google Scholar 

  10. G. P. Koiper (editor), Solar System Series, Vol. 1: The Sun, University of Chicago Press (1953).

Download references

Authors

Additional information

Leningrad Branch of the Special Astrophysical Observatory, Academy of Sciences of the USSR. Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Radiofizika, Vol. 16, No. 5, pp. 731–736, May, 1973.

Rights and permissions

Reprints and permissions

About this article

Cite this article

Borovik, V.N., Gel'freikh, G.B. & Lubyshev, B.I. New estimate of the altitude of local sources of the slowly varying component of solar radio emission at the 3.2 cm wavelength. Radiophys Quantum Electron 16, 558–562 (1973). https://doi.org/10.1007/BF01033490

Download citation

  • Received:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF01033490

Keywords

Navigation