Ground-based extensive air shower arrays can observe Gamma Ray Bursts in th
e 1 GeV-1 TeV energy range using the "single particle" technique. The sensi
tivity to detect a GRB as a function of the burst parameters and the detect
or characteristics are discussed. The rate of possible observations is eval
uated, making reasonable assumptions on the high energy emission, the absor
ption of gamma-rays in the intergalactic space, the distribution of the sou
rces in the universe and the bursts luminosity function. We show that a lar
ge area detector located at high mountain altitude has good prospects for p
ositive detections, providing useful information on the high energy compone
nt of GRBs. (C) 2000 Elsevier Science B.V. All rights reserved.