Cosmic rays physics is currently studied with rather sophisticated detector
s operating in a variety of either experimental conditions or atmospheric d
epths in the world. In this paper we present the main properties of the obs
erved features of high-energy nuclear interaction phenomena of cosmic rays,
with particular emphasis on some experimental observations made by the emu
lsion chamber technique at Chacaltaya Laboratory (Bolivia, 5230 m a.s.l.).
A discussion on the past and present achievements as well as the future pro
spects of high altitude mountain laboratories for cosmic ray physics is pre
sented.