The power-law energy spectra of non-thermal electrons for each 1.024 second
have been drawn together during the flare. For some flares, it is discover
ed that the energy spectra taken at different times present a roughly fixed
crossing point, at which point the flux of non-thermal electrons keeps the
same during the flare. The possible significance of this phenomenon is dis
cussed. We conjecture that there may be a flux saturation at the low-energy
cutoff in the process of electron acceleration.