  The general aim of this work is to obtain the lateral distribution of
atmospheric Cherenkov light in extensive air showers produced by different
primary particles precisely by. protons, Helium, Iron, Oxygen, Carbon,
Nitrogen, Calcium, Silicon and gamma quanta in wide energy range at high
mountain observation level of Chacaltaya cosmic ray station. The simulations
are divided generally in two energy ranges 10GeV-10 TeV and 10 TeV-10 PeV. One
large detector has been used for simulations, the aim being to reduce the
statistical fluctuations of the obtained characteristics. The shape of the
obtained lateral distributions of Cherenkov light in extensive air showers is
discussed and the scientific potential for solution of different problems as
well.
