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Measuring the polarization of solar radio emission due to the total magnetic field of the sun

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References

  1. K. de Jager, Structure and Dynamics of the Solar Atmosphere [Russian translation], IL, Moscow, 1962.

    Google Scholar 

  2. W. N. Ghristiansen, D. E. Yabsley, and B. Y. Mills, Austral. J. Sci. Res., A-2, 506, 1949.

    Google Scholar 

  3. N. L. Kaidanovskii, E. G. Mirzabekyan, and S. E. Khaikin, Proc. of the Fifth Conference on Problems of Cosmogony [in Russian], Izd. AN SSSR, Moscow, 1956.

    Google Scholar 

  4. I. F. Belov, Geomagnetizm i aeronomiya, 6, 1106, 1964.

    Google Scholar 

  5. V. V. Zheleznyakov, Astron, zh., 5, 829, 1963.

    Google Scholar 

  6. S. F. Smerd, Austral. J. Sci. Res., A-2, 265, 1950.

    Google Scholar 

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Izvestiya VUZ. Radiofizika, Vol. 8, No. 2, pp. 400–401, 1965

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Belov, I.F. Measuring the polarization of solar radio emission due to the total magnetic field of the sun. Soviet Radiophysics 8, 286–287 (1965). https://doi.org/10.1007/BF01038621

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