Hostname: page-component-586b7cd67f-tf8b9 Total loading time: 0 Render date: 2024-11-26T17:44:31.486Z Has data issue: false hasContentIssue false
  • English
  • Français

58. Results of observations of the scattering of radio waves by the electronic inhomogeneities of the solar corona

Published online by Cambridge University Press:  14 August 2015

V. V. Vitkevitch
V. V. Vitkevitch*
Affiliation:
Crimean Station, Physical Institute of the Academy of Sciences, Moscow, U.S.S.R.

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

A new method for the investigation of the solar corona, suggested by us (Vitkevitch, 1951) [1], consists of observing the radio source identified with the Crab nebula (NGC 1952; α = 05h 31m 40s, δ = 22° 10′) when it is covered by the solar corona. This occurs every year on 14–15 June.

Type
Part IV: The Quiet Sun
Information
Symposium - International Astronomical Union , Volume 4: Radio Astronomy , 1957 , pp. 313 - 317
Copyright
Copyright © Cambridge University Press 1957 

References

References

1. Vitkevitch, V. V. Dokl. Akad. Nauk U.S.S.R. 77, 585, no. 4, 1951.Google Scholar
2. Vitkevitch, V. V. Dokl. Akad. Nauk U.S.S.R. 101, 429, no. 3, 1955.Google Scholar
3. Hewish, A. Proc. Roy. Soc. A , 228, 238, 1955.Google Scholar
4. Chandrasekhar, S. M.N. R.A.S. 112, no. 5, 1952.CrossRefGoogle Scholar
5. Machin, K. E. Nature , 167, 889–91, 1951.Google Scholar

Reference

1. Hewish, A. Proc. Roy. Soc. A , 228, 238, 1955.Google Scholar