AAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAA OOO OOO OOOO OOOO OO O O O O O O O O O O O OO O O O O O O O O O O OO O O O O O O O O O OOOO OO OO O O O O O OOOO O OO O O OOOOOOO O O O O O O O O OO O O O O OOO OOO O O OOOO OO O O O O COSMIC RAY SIMULATION FOR KASCADE A PROGRAM TO SIMULATE EXTENSIVE AIR SHOWERS IN ATMOSPHERE BASED ON A PROGRAM OF P.K.F. GRIEDER, UNIVERSITY BERN, SWITZERLAND QGSJET-II MODEL ACCORDING TO S.S. OSTAPCHENKO, IEKP, KARLSRUHE AND MSU, MOSCOW, RUSSIA HDPM MODEL ACCORDING TO J.N. CAPDEVIELLE, COLLEGE DE FRANCE, PARIS, FRANCE FLUKA MODEL FROM A. FASSO (CERN), A. FERRARI, J. RANFT (SIEGEN), AND P. SALA, INFN MILAN, MILAN, ITALY, AND CERN, GENEVA, SWITZERLAND EGS4 ACCORDING TO W.R. NELSON, H. HIRAYAMA, D.W.O. ROGERS, SLAC, STANFORD, USA NKG FORMULAS FOR FAST SIMULATION OF EL.MAG. PARTICLES REFERENCES: D. HECK, J.KNAPP, J.N. CAPDEVIELLE, G. SCHATZ, T. THOUW, REPORT FZKA 6019 (1998) SEE ALSO WEB PAGE https://www.ikp.kit.edu/corsika/ KARLSRUHE INSTITUTE OF TECHNOLOGY (KIT) INSTITUT FUER KERNPHYSIK POSTFACH 3640 D-76021 KARLSRUHE GERMANY IN CASE OF PROBLEMS CONTACT: Dr. Tanguy Pierog e-mail: tanguy.pierog@kit.edu FAX: (49) 721-608-24075 PHONE: (49) 721-608-28134 OR : Dr. Dieter Heck e-mail: dieter.heck@partner.kit.edu FAX: (49) 721-608-24075 PHONE: (49) 721-608-23777 AND SEND YOUR LIST-FILE BY E-MAIL NUMBER OF VERSION : 7.6400 DATE OF VERSION : DECEMBER 21, 2017 VERSION GENERATED FOR UNIX OR COMPATIBLE SYSTEMS ^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^ (RECL IS DEFINED IN BYTES) WITH TIMERC DATE ROUTINE ZENITH ANGLE DEPENDENCE FOR FLAT DETECTOR ARRAY ========== USERS RUN DIRECTIVES FOR THIS SIMULATION =========================== DATA CARDS FOR RUN STEERING ARE EXPECTED FROM STANDARD INPUT RUNNR 2 run number EVTNR 1 number of first shower event NSHOW 10 number of showers to generate PRMPAR 14 particle type of prim. particle ESLOPE -2.7 slope of primary energy spectrum ERANGE 1.E4 1.E4 energy range of primary particle THETAP 20. 20. range of zenith angle (degree) PHIP -180. 180. range of azimuth angle (degree) SEED 1 0 0 seed for 1. random number sequence SEED 2 0 0 seed for 2. random number sequence OBSLEV 110.E2 observation level (in cm) FIXCHI 0. starting altitude (g/cm**2) MAGNET 20.0 42.8 magnetic field centr. Europe HADFLG 0 0 0 0 0 2 flags hadr.interact.&fragmentation ECUTS 0.3 0.3 0.003 0.003 energy cuts for particles MUADDI T additional info for muons MUMULT T muon multiple scattering angle ELMFLG T T em. interaction flags (NKG,EGS) STEPFC 1.0 mult. scattering step length fact. RADNKG 200.E2 outer radius for NKG lat.dens.distr. LONGI T 10. T T longit.distr. & step size & fit & out ECTMAP 1.E4 cut on gamma factor for printout MAXPRT 1 max. number of printed events DIRECT ./ output directory USER you user DEBUG F 6 F 1000000 debug flag and log.unit for out MUADDI T EXIT terminates input END OF DATACARD INPUT ========== START OF RUN ======================================================= PRESENT TIME : 13.04.2018 12:36:43 UTC RANDOM NUMBER GENERATOR AT BEGIN OF RUN : SEQUENCE = 1 SEED = 1 CALLS = 0 BILLIONS = 0 SEQUENCE = 2 SEED = 2 CALLS = 0 BILLIONS = 0 PARTICLE OUTPUT TO FILE: ./DAT000002 LONGITUDINAL OUTPUT TO FILE: ./DAT000002.long ========== INTERACTION MODELS ================================================= QGSJET TREATS HIGH ENERGY HADRONIC INTERACTIONS QGSJET CROSS-SECTIONS ARE TAKEN ==================================================== | | | QUARK GLUON STRING JET -II MODEL | | | | HADRONIC INTERACTION MONTE CARLO | | BY | | S. OSTAPCHENKO | | | | e-mail: sergei@tf.phys.ntnu.no | | | | Version II-04 | | | | Publication to be cited when using this program: | | S.Ostapchenko, PRD 83 (2011) 014018 | | | | last modification: 09.04.2013 | | | | Any modification has to be approved by the author| ==================================================== qgaini: cross sections readout from the file: qgsdat-II-04 done qgaini: nuclear cross sections readout from the file sectnu-II-04 NUCLEUS PROJECTILES FRAGMENT REALISTICALLY IN THE FIRST INTERACTION FRAGMENTATION WITH EVAPORATION (PT AFTER JACEE) FLUKA TREATS LOW ENERGY HADRONIC INTERACTIONS