EVIDENCE FOR STOCHASTIC ELECTRON ACCELERATION IN THE CM2 COMPONENT OF 1988 JUNE FLARES

Secondary peak which is referred as cm2 component of microwave bursts occurred about 30-60 min later after the impulsive microwave emission (cml). Though some works have been done for cm2, the nature of cm2 component remains unclear. In this paper we present two cm2 bursts which may be explained by stochastic electron acceleration in the turbulent plasma in the closed magnetic loop.