Subcore observations and high psub(t)

The observations of subcores with the Leeds 35m2 spark chamber array have shown a much lower frequency of subcores than observed at Kiel and at Tokyo with detectors also well suited to observe detailed shower structure. However, overlying material was quite different and the resulting transition effects are difficult to correct for. One seems forced to compare results for subcores occuring only under relatively thin roof material. The discrepancy is thereby nearly removed. As a further test, the Leeds array has recently been run with simulated roof beams above the array. A spin-off from this run is the verification of the ability of our detectors to show ''subcores'' of all sizes and the ability of our scanners to find them. When we calculate psub(t) for our subcores in the traditional manner, no values > 5 GeV/c result. Further, in another paper, we present simulation results showing that there is poor correlation between psub(t) calculated in the usual manner on an event by event basis. The conclusion is that a meaningful utilization of the data requires a comparison of frequency of observable subcore parameters derived from simulations that include QCD nuclear physics to the observed frequencies