Abstract
Peak fluxes of flare-associated 8–12 Å X-ray bursts occur at or near the time of the maximum energy content of the soft X-ray source volume. The amplitudes of flare-associated bursts may thus be used as a measure of the energy deposited in the source volume by non-thermal electrons and other processes. In the mean, the soft X-ray burst amplitude is apparently independent of the occurrence of a type III event. This is interpreted to indicate that electrons accelerated by the type III process do not directly participate in establishing the soft X-ray source volume.
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Teske, R.G., Thomas, R.J. Solar soft X-rays and solar activity. Sol Phys 24, 434–443 (1972). https://doi.org/10.1007/BF00153386
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DOI: https://doi.org/10.1007/BF00153386