Sergio J. Sciutto
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c
c Routine directly callable from C/C++ (it could be necessary to
c append an underscore, "_", to its name depending on the C/C++
c compiler used).
c
c
subroutine croinputdata0(intdata, realdata, shprimcode, shprimwt)
c
c Copying into arrays input data parameters from an already read
c compressed file header.
c
c Written by: S. J. Sciutto, La Plata 1997, 1998;
c Fermilab 1999;
c La Plata 1999, 2000, 2003, 2018.
c
c
c Arguments:
c =========
c
c intdata......... (output, integer, array(*)) Integer data array.
c The calling program must provide enough space
c for it. The following list describes the
c different data items:
c ( 1) Number of different primary particles.
c ( 2) Number of special particles defined.
c ( 3-4) Reserved for future use.
c ( 5) Primary energy distribution: 0 fixed
c energy; 1 varying energy.
c ( 6) Zenith angle distribution: 0 fixed angle;
c 1 cos distribution; 2 sin cos distribution.
c ( 7) Azimuth angle distribution: 0 (10) fixed
c angle (geographic azimuth); 1 (11) varying
c angle (geographic azimuths).
c ( 8) Number of observing levels.
c ( 9) Atmospheric model label.
c (10) Thinning switch: 0 disabled, 1 enabled.
c (11-14) Reserved for future use.
c (15) First shower number.
c realdata........ (output, double precision, array(*)) Real data
c array. The calling program must provide enough
c space for it. The following list describes the
c different data items:
c ( 1) Minimum primary energy (GeV).
c ( 2) Maximum primary energy (GeV).
c ( 3) Gamma of energy distribution.
c ( 4) Minimum zenith angle (deg).
c ( 5) Maximum zenith angle (deg).
c ( 6) Minimum azimuth angle (deg).
c ( 7) Maximum azimuth angle (deg).
c ( 8) Thinning energy parameter.
c ( 9) Injection altitude (m).
c (10) Injection depth (g/cm2).
c (11) Ground altitude (m).
c (12) Ground depth (g/cm2).
c (13-14) Reserved for future use.
c (15) Altitude of first observing level (m).
c (16) Depth of first observing level (g/cm2).
c (17) Altitude of last observing level (m).
c (18) Depth of last observing level (g/cm2).
c (19) Distance between consecutive observing
c levels in g/cm2.
c (20) Site latitude (deg).
c (21) Site longitude (deg).
c (22) Geomagnetic field strength (nT).
c (23) Local geomagnetic inclination (deg).
c (24) Local geomagnetic declination (deg).
c (25) Amplitude of relative fluctuation of B.
c (26) Event date.
c (27-29) Reserved for future use.
c (30) Minimum lateral distance used for ground
c particle histograms (m).
c (31) Maximum lateral distance used for ground
c particle histograms (m).
c (32) Minimum energy used for histograms (GeV).
c (33) Maximum energy used for histograms (GeV).
c (34-35) Reserved for future use.
c (36) Minimum radial distance parameter for the
c current compressed file (m).
c (37) Maximum radial distance parameter for the
c current compressed file (m).
c shprimcode...... (output, integer, array(*)) For i from 1 to
c intdata(1), shprimcode(i) gives the
c corresponding primary particle code. The
c coding system used is the one defined when
c starting the cio system.
c shprimwt........ (output, double precision, array(*)) For i from
c 1 to intdata(1), shprimwt(i) gives the
c corresponding primary particle weight. This
c weight is 1 in the single primary case.
c
c
c<--->
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