The use of the World Neutron Monitor Network to detect high-energy sol
ar neutrons is discussed in detail. It is shown that the existing netw
ork can be used for the routine detection of intense sporadic solar-ne
utron events whenever they occur. A technique is suggested involving t
he weighted summation of responses of separate monitors to solar neutr
ons. It is demonstrated that the use of this method improves the signi
ficance of solar-neutron event detection. Different results of the sim
ulation of the neutron-monitor sensitivity to solar neutrons have been
tested with respect to their application for practical use. It is sho
wn that the total number of neutrons with energy above 300 MeV injecte
d from the Sun during a solar flare can be estimated directly from the
time-integrated neutron-monitor response to solar neutrons without an
y model assumptions. The estimation technique has been developed.