| 1 | RUNNR 1
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| 2 | PRMPAR 14 particle type
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| 3 | ERANGE 100 1000 energy range
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| 4 | EVTNR 1 number of first shower event
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| 5 | NSHOW 10 number of showers to generate
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| 6 | ESLOPE -2.73 slope of primary energy spectrum
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| 7 | THETAP 0. 0. range of zenith angle (degree)
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| 8 | PHIP 90. 90. range of azimuth angle (degree)
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| 9 | VIEWCONE 0. 5.
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| 10 | DIRECT results/ data directory managed by daemon
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| 11 | SEED 1 3 0 seed values managed by daemon
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| 12 | SEED 6 3 0 seed values managed by daemon
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| 13 | SEED 1 3 0 seed values managed by daemon
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| 14 | OBSLEV 2200.E2 observation level (in cm)
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| 15 | ELMFLG F F em. interaction flags (NKG,EGS)
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| 16 | RADNKG 200.E2 outer radius for NKG lat.dens.determ.
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| 17 | MAGNET 29.5 23.0 magnetic field at LaPalma
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| 18 | VENUS T 0 use venus for high energy hadrons
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| 19 | VENSIG T use VENUS hadronic cross sections
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| 20 | ECUTS 0.3 0.3 0.02 0.02 e.cuts: had, mu, elec y fot
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| 21 | MUADDI F additional info for muons
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| 22 | MUMULT T muon multiple scattering angle
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| 23 | LONGI T 10. T F longit.distr. & step size & fit
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| 24 | MAXPRT 0 max. number of printed events
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| 25 | ECTMAP 1.E4 cut on gamma factor for printout
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| 26 | STEPFC 0.1 mult. scattering step length fact.
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| 27 | DEBUG F 6 F 1000000 debug flag and log.unit for out
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| 28 | CWAVLG 290. 600. Cherenkov wavelength band
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| 29 | CSCAT 1 0. 40000. scatter Cherenkov events
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| 30 | CERSIZ 1. bunch size Cherenkov photons
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| 31 | CERFIL T Cherenkov output to extra file
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| 32 | CERTEL 1
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| 33 | 0. 0. 0. 0. 0. 20000. 17000. Location and size of each CT
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| 34 | DATBAS T write .dbase file
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| 35 | USER dorota user
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| 36 | atmosphere 6 T
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| 37 | EXIT terminates input
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| 38 |
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| 39 |
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