Particle acceleration is intrinsic to the primary energy release in th
e impulsive phase of solar flares, and we cannot understand flares wit
hout understanding acceleration. New observations in soft and hard X-r
ays, gamma-rays and coherent radio emissions are presented, suggesting
flare fragmentation in time and space. X-ray and radio measurements e
xhibit at least five different time scales in flares. In addition, sam
e new observations of delayed acceleration signatures are also present
ed. The theory of acceleration by parallel electric fields is used to
model the spectral shape and evolution of hard X-rays. The possibility
of the appearance of double layers is further investigated.