The flux of high energy cosmic rays coming from the decay of vortons i
s estimated. If the abundance of loops corresponding to a superconduct
ivity scale coincident with that of the string formation is corrected
to be compatible with the critical density of universe, it is found th
at the emission of one carrier per vorton may produce a flux of one co
smic ray event per km(2) of detector and per year. (C) 1998 Elsevier S
cience B.V.