Abstract
Solar decameter bursts of Type IIIb are observed with a multichannel radiometer at wavelengths around 12m. The time and frequency resolutions were 10 ms and 100 kHz. Observations on the time structure of these bursts are presented. A theoretical model which accounts for various aspects of these bursts is proposed.
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References
de la Noë, J.: 1974, Solar Phys. 37, 225.
de la Noë, J. and Boischot, A.: 1972, Astron. Astrophys. 20, 55.
Harris, E. G.: 1969, in A. Simon and W. B. Thompson (eds.), Advances in Plasma Physics, Vol. III, Interscience Publishers.
Krishan, V.: 1978, Astrophys. Space Sci. 57, 191.
Krishan, V.: 1979, to appear in Plasma Phys.
Krishan, V., Sinha, K. P., and Krishan, S.: 1978, Astrophys. Space Sci. 53, 13.
Lang, K. R.: 1974, Astrophysical Formulae, Springer-Verlag, p. 286.
McCulloch, P. M. and Ellis G. R. A.: 1977, Radio Phys. (USSR) 20, No. 9, 1.
Sastry, Ch. V.: 1969, Solar Phys. 10, 429.
Sastry, Ch. V.: 1971, Astrophys. Letters 8, 115.
Sastry, Ch. V.: 1972, Astrophys. Letters 11, 47.
Sastry, Ch. V.: 1973, Solar Phys. 28, 197.
Smith, R. A. and de la Noë, J.: 1976, Astrophys. J. 207, 605.
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Krishan, V., Subramanian, K.R. & Sastry, C.V. Observations and interpretation of solar decameter type IIIb radio bursts. Sol Phys 66, 347–355 (1980). https://doi.org/10.1007/BF00150590
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DOI: https://doi.org/10.1007/BF00150590