Skip to main content
Log in

Influence of temperature distribution in the chromosphere on the spectrum of the S-component of solar radio emission

  • Brief Communications and Letters to the Editor
  • 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. G. B. Gel'freikh et al., Izv. GAO, No. 185, 167 (1970).

    Google Scholar 

  2. V. V. Zheleznyakov, Radio emission from the Sun and Planets [in Russian], Izd. Nauka, Moscow (1964).

    Google Scholar 

  3. E. Ya. Zlotnik, Astron. Zh.,45, No. 2, 3 (1968).

    Google Scholar 

  4. N. G. Peterova and Sh. B. Akhmedov, Astron. Zh.,50, No. 6 (1973).

  5. M. N. Fasakhova and O. I. Yudin, Astron. Zh. (in press).

  6. S. A. Kaplan and V. N. Tsytovich, Plasma Astrophysics [in Russian], Izd. Nauka, Moscow (1972).

    Google Scholar 

  7. D. A. Kuznetsov, in: Research on Magnetism, Aeronomy, and Physics of the Sun, No. 7 [in Russian], Izd. Nauka, Moscow (1970), p. 208.

    Google Scholar 

  8. I. F. Belov et al., Izv. VUZ. Radiofiz.,16, No. 5, 723 (1973).

    Google Scholar 

Download references

Authors

Additional information

Scientific Research Institute for Radiophysics. Translated from Izvestiya Vysshikh Uchebnykh Zavedenii. Radiofizika, Vol. 17, No. 8, pp. 1240–1242, August, 1974.

Rights and permissions

Reprints and permissions

About this article

Cite this article

Fasakhova, M.N., Yudin, O.I. Influence of temperature distribution in the chromosphere on the spectrum of the S-component of solar radio emission. Radiophys Quantum Electron 17, 944–945 (1974). https://doi.org/10.1007/BF01037096

Download citation

  • Received:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF01037096

Keywords

Navigation