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First results from the Clark Lake Multifrequency Radioheliograph

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Abstract

We give a brief description of the Clark Lake Multifrequency Radioheliograph which is presently used for solar research in the frequency range 20–125 MHz. We present two-dimensional images of the Sun's corona at several frequencies within this range, obtained with time resolution as good as 1.28 s. The shape of the Sun's outer corona as observed at meter-decameter wavelengths appears to change in time periods as short as a few seconds.

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References

  • Erickson, W. C. and Fisher, J. R.: 1974, Radio Science 9, 387.

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  • Erickson, W. C., Gergely, T. E., Kundu, M. R., and Mahoney, M. J.: 1977, Solar Phys. 54, 57.

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  • Fisher, J. R.: 1972, Ph.D. Thesis. University of Maryland.

  • von Arx, B., Caflish, M., and Erickson, W. C.: 1978, Internal Report, AP78-027, University of Maryland.

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Authors and Affiliations

  1. Astronomy Program, Clark Lake Radio Observatory, University of Maryland, 20742, College Park, MD, U.S.A.

    M. R. Kundu, W. C. Erickson, T. E. Gergely, M. J. Mahoney & P. J. Turner

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  1. M. R. Kundu
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  2. W. C. Erickson
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  3. T. E. Gergely
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  4. M. J. Mahoney
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  5. P. J. Turner
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Kundu, M.R., Erickson, W.C., Gergely, T.E. et al. First results from the Clark Lake Multifrequency Radioheliograph. Sol Phys 83, 385–389 (1983). https://doi.org/10.1007/BF00148288

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  • DOI: https://doi.org/10.1007/BF00148288

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