  A preliminary flux estimate of various cosmic-ray constituents based on the
atmospheric Cerenkov light flux of extensive air showers using fractal and
wavelet analysis approach is proposed. Using a Monte-Carlo simulated database
of Cerenkov images recorded by the TACTIC telescope, we show that one of the
wavelet parameters (wavelet dimension B6) provides ? 90% segregation of the
simulated events in terms of the primary mass. We use these results to get a
preliminary estimate of primary flux for various cosmic-ray primaries above 5
TeV energy. The simulation based flux estimates of the primary mass as recorded
by the TACTIC telescope are in good agreement with the experimentally
determined values.
