Abstract
The relationship between the proton intensity in the interplanetary space and radio bursts of type II for 78 proton events for the period of 1989–2005 is studied based on the data of the Radio Solar Telescope Network. Two families of events have been revealed in plots describing the dependence of the intensity of protons with different energies and the rate of the frequency drift of meter-decameter radio bursts. This suggests the generation of shock waves both in the region of flare energy release and at the fronts of coronal mass ejection.
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Original Russian Text © E.A. Isaeva, Yu.T. Tsap, 2011, published in Izvestiya Krymskoi Astrofizicheskoi Observatorii, 2011, Vol. 107, pp. 118–125.
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Isaeva, E.A., Tsap, Y.T. The origin of solar energetic particles and type II meter radio bursts. Bull.Crim. Astrophys. Observ. 107, 78–83 (2011). https://doi.org/10.3103/S0190271711010074
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DOI: https://doi.org/10.3103/S0190271711010074