CORSIKA add-on package IACT/ATMO:
Version 1.63 (November 2020)
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Description of telescope position, array offets and shower parameters. More...
Data Fields | |
double | altitude |
Nominal altitude angle of telescope system [deg]. More... | |
double | aweight [MAX_ARRAY] |
Area weight for non-uniformly distributed core offsets. More... | |
double | azimuth |
Nominal azimuth angle of telescope system [deg]. More... | |
int | event |
int | max_tel |
Maximum number of telescopes acceptable (MAX_TEL) | |
struct mc_run | mc_run |
int | narray |
Number of arrays with random shifts per shower. | |
int | ntel |
Number of telescopes simulated per array. | |
double | obs_height |
Height of observation level [cm]. | |
struct mc_options | options |
File names etc. More... | |
double | refpos [3] |
Reference position with respect to obs. More... | |
double | rtel [MAX_TEL] |
Radius of spheres enclosing telescopes [cm]. | |
int | run |
struct simulated_shower_parameters | shower_sim |
double | source_altitude |
Altitude of assumed source. More... | |
double | source_azimuth |
Azimuth of assumed source. More... | |
double | toff |
Time offset from first interaction to the moment. More... | |
int | with_aweight |
Is 1 if input data came with weights. | |
double | xoff [MAX_ARRAY] |
X offsets of the randomly shifted arrays [cm]. | |
double | xtel [MAX_TEL] |
X positions of telescopes ([cm] -> north) | |
double | yoff [MAX_ARRAY] |
Y offsets of the randomly shifted arrays [cm]. | |
double | ytel [MAX_TEL] |
Y positions of telescopes ([cm] -> west) | |
double | ztel [MAX_TEL] |
Z positions of telescopes ([cm] -> up) | |
double telescope_array::altitude |
double telescope_array::aweight[MAX_ARRAY] |
(may be 0 when older data with uniform offsets are read). [cm^2]
double telescope_array::azimuth |
struct mc_options telescope_array::options |
double telescope_array::refpos[3] |
level [cm]
double telescope_array::source_altitude |
double telescope_array::source_azimuth |
double telescope_array::toff |
when the extrapolated primary flying with the vacuum speed of light would be at the observation level.