Аннотация:Tunka-133 EAS Cherenkov light array
constructing now in Tunka Valley (Siberia) will
provide registration of pulse waveform with 5 ns
step from every of 133 detectors. To use such unique
abundant information the new method of EAS core
position and depth of maximum (Xmax) reconstruction,
based on the measurement of Full Width at
Half Maximum (FWHM) of Cherenkov light pulses
has been developed. The method is based on the
CORSIKA simulation and takes into account all the
real apparatus characteristics.
Using of a new width-distance function (WDF) will
allow to reconstruct the EAS core position not only
inside the array, but also at a certain distance beyond
the array geometrical border. This can increase
substantially the effective area for EAS registration
in the energy range more than 1017 eV .