RUNNR 1 PRMPAR 14 particle type ERANGE 100 1000 energy range EVTNR 1 number of first shower event NSHOW 10 number of showers to generate ESLOPE -2.73 slope of primary energy spectrum THETAP 0. 0. range of zenith angle (degree) PHIP 90. 90. range of azimuth angle (degree) VIEWCONE 0. 5. DIRECT results/ data directory managed by daemon SEED 1 3 0 seed values managed by daemon SEED 6 3 0 seed values managed by daemon SEED 1 3 0 seed values managed by daemon OBSLEV 2200.E2 observation level (in cm) ELMFLG F F em. interaction flags (NKG,EGS) RADNKG 200.E2 outer radius for NKG lat.dens.determ. MAGNET 29.5 23.0 magnetic field at LaPalma VENUS T 0 use venus for high energy hadrons VENSIG T use VENUS hadronic cross sections ECUTS 0.3 0.3 0.02 0.02 e.cuts: had, mu, elec y fot MUADDI F additional info for muons MUMULT T muon multiple scattering angle LONGI T 10. T F longit.distr. & step size & fit MAXPRT 0 max. number of printed events ECTMAP 1.E4 cut on gamma factor for printout STEPFC 0.1 mult. scattering step length fact. DEBUG F 6 F 1000000 debug flag and log.unit for out CWAVLG 290. 600. Cherenkov wavelength band CSCAT 1 0. 40000. scatter Cherenkov events CERSIZ 1. bunch size Cherenkov photons CERFIL T Cherenkov output to extra file CERTEL 1 0. 0. 0. 0. 0. 20000. 17000. Location and size of each CT DATBAS T write .dbase file USER dorota user atmosphere 6 T EXIT terminates input