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Fine structure of a solar active region at 3.7 and 11.1 cm wavelengths

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Reference

  • Hobbs, R. W., Jordan, S. D., and Webster, W. J., Jr.: 1973, Nature Phys. Sci 24, 48.

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Author notes

  1. T. Velusamy

    Present address: Tata Institute of Fundamental Research, Bombay, India

Authors and Affiliations

  1. Astronomy Program, University of Maryland, Md., U.S.A.

    M. R. Kundu, R. H. Becker & T. Velusamy

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  1. M. R. Kundu
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  2. R. H. Becker
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  3. T. Velusamy
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Kundu, M.R., Becker, R.H. & Velusamy, T. Fine structure of a solar active region at 3.7 and 11.1 cm wavelengths. Sol Phys 34, 185–188 (1974). https://doi.org/10.1007/BF00149610

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  • DOI: https://doi.org/10.1007/BF00149610

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