Computer Science
Scientific paper
Aug 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....7..199l&link_type=abstract
In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 7 p 199-202 (SEE N85-35968 24-93)
Computer Science
Cerenkov Radiation, Cosmic Ray Showers, Depth Measurement, Distance Measuring Equipment, Pulse Amplitude, Pulsed Radiation, Cerenkov Counters, Computerized Simulation, Photomultiplier Tubes, Radiation Measurement
Scientific paper
The agreement between measured distances to maximum for approx. 49 simultaneous Cerenkov pulse profiles from different sites is + or - approx. 0.1 km near 4.5 km and + or - 0.5 km near 7 km. Uncertainty in depths of maximum are approx. + or - 10 g sq and + or - 30 g cm/2 respectively. Usually the Hillas-Patterson simulation is able to fit both pulse shapes satisfactorily using a single N(x) profile.
Liebing D. F.
Patterson John R.
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