Abstract
Four 15.8 mm solar bursts are discussed and the results are compared with data on recorded proton events, in relation to the prediction of such events from radio observations.
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References
Croom, D. L. and Powell, R. J.: 1969, Nature 221, 945.
Castelli, J. P. and Aarons, J.: 1969, ‘Radio Burst Spectra and the Short Term prediction of Solar Proton Events’, Proceedings XV Electromagnetic Wave Propagation Meeting of AGARD, C.P. No. 49, 1970.
ESSA: 1968, Solar Geophysical Data Nos. 291, 292, Essa Research Laboratories, Boulder, Colo., U.S.A.
Tokyo Astronomical Observatory: 1968, Monthly Solar Radio Emission Bulletin October–November 1968, Mitaka, Tokyo, Japan.
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Currently on leave of absence as 1969–70 NRC-OAR Senior Post-Doctoral Research Associate, AFCRL, Hanscom Field, Bedford, Mass. 01730.
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Croom, D.L., Powell, R.J. Solar activity at λ = 15.8 mm (19 GHz) during the period 27 October–4 November 1968 and its relation to proton events. Sol Phys 14, 221–225 (1970). https://doi.org/10.1007/BF00240182
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DOI: https://doi.org/10.1007/BF00240182