  Atmospheric Cherenkov technique is an established methodology to study TeV
energy gamma rays. Here we carry out systematic monte carlo simulation studies
of the timing information of Cherenkov photons. Extensive studies have already
been carried out in this regard. Most of these are carried out at higher
energies with the aim of studying the elemental composition of cosmic rays.
However not much attention is paid to the species dependent signatures at TeV
energies. In this work, functional fits have been carried out to the spherical
Cherenkov shower fronts and the radii of curvature have been found to be equal
to the height of shower maximum irrespective of the species or the observation
level. Functional fits have also been carried out to describe the pulse shapes
at various core distances in terms of well known probability density
distribution functions (PDF). Two types of PDF's have been tried viz. gamma
function and lognormal function. The variation of the pulse shape parameters as
a function of primary energy, observation height and incident angles have been
studied. The possibility of deriving the pulse shape parameters like the rise &
decay times, full width at half maximum from the easily measurable quantities
like the mean and RMS variation of photon arrival times offers a very important
new technique which can be easily applied in an observation.
