Many-site multichannel simultaneous observations of the flare star EV Lac r
evealed high-frequency brightness oscillations superimposed on the mean fla
re light curve. Oscillations occur at the earliest stage of a flare and are
visible during the high state. Coherent oscillations of 26 and 13 sec were
seen during three flare events. The pulsed fractions were 2.5% in the B ba
nd and 10-15% in the U band. This oscillatory phenomenon can be used to imp
rove our understanding of the flare process.