Abstract
Measurements of the RMS fluctuation of the depth of shower maximum sigma (Xm) as a function of energy are reported from 1.5*1017 to 1019 eV. The results are based on a study of the risetimes of pulses recorded from four 34 m2 water-Cerenkov detectors in 2691 showers having zenith angle less than 40 degrees . The energy dependence of sigma (Xm) is determined and found to be in reasonable agreement with what is expected for a constant mass composition and an energy-dependent nucleon-air cross section.

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