Output from the program is a CAT-file (hyp.out) and the original HYPOCENTER print file (print.out) with more detailed information. The hyp.out file can be plotted directly using EPIMAP or MAP. In addition, there is also the HYPO71 style summary file, hypsum.out. NOTE: In print.out and hypsum.out, year is only given with 2 digits. Magnitude in hypsum.out and print.out are only coda magnitude and will be different from same magnitude in hyp.out if a magnitude correction has been used.
When HYP is executed from EEV, the print.out file has no station listing. In all other cases, there is a station listing.
Some explanation is given below, for details see HYP manual
The output in print.out first shows the content of the TEST parameters in the STATION0.HYP file. After that comes some routine output from the starting location algorithm. Then follows the output from the iterations, which should be self-explanatory. The location is then given on one line containing origin time, latitude longitude (deg min), depth, number of phases, the number of degrees of freedom in the spatial solution (maximum 3), rms damping and errors, error estimates, resolution matrix. Last are the station lines with the following abbreviations:
stn : Station dist : Distance in km azm : Azimuth at the source ain : Angle of incidence at the source phs : Phase specified by user calcphs: Phase used by program w : Input weight hrmn : Hour minute t-sec: Arrival time sec t-obs: Observed travel time t-cal: Calculated travel time res : Residual wt : Weight usedi by program, normalized to 1.0 di : importance of phase in % : network and locaiton, no header
An example of output on screen is given below
date hrmn sec lat long depth no m rms damp erln erlt erdp 16 1 1 029 9.85 6749.40N 20 21.0E 15.0 8 3 0.53 0.000 54.9 42.6118.6 stn dist azm ain w phas calcphs hrmn tsec t-obs t-cal res wt di KIF 137 7.6 55.1 0 P PN4 029 29.9 20.05 21.06 -1.01 1.00 16 KIF 137 7.6 BAZ 169.2 188.0 -18.82 0.20 9 KIF 137 7.6 55.1 0 S SN4 029 46.4 36.55 36.64 -0.09 1.00 29 HEF 152 63.2 55.1 0 P PN4 029 32.5 22.61 22.93 -0.32 1.00 12 KTK1 178 40.5 55.1 0 P PN4 029 36.2 26.36 26.07 0.29 1.00 4 STEI 215 275.5 55.1 0 P PN4 029 40.3 30.50 30.66 -0.16 1.00 10 FAUS 221 259.5 55.1 0 P PN4 029 40.9 31.09 31.38 -0.30 1.00 16 ARA0 283 45.3 55.1 0 P PN4 029 50.6 40.75 39.16 1.59 1.00 4 KTK1 HZ hdist: 178.6 amp: 2.5 T: 0.2 ml = 0.9 ARA0 HZ hdist: 283.4 amp: 2.2 T: 0.8 ml = 1.2 2016 1 1 0029 9.9 L 67.823 20.349 15.0 RRR 6 0.5 1.0LRRR OLD: 1 1 0029 8.6 L 67.854 20.249 0.0 BER 6 0.6 1.0LBER In case of Nordic2 format, it would be date hrmn sec lat long depth no m rms damp erln erlt erdp 16 1 1 029 9.60 6747.52N 20 25.9E 15.0 8 3 0.59 0.000 45.2 20.4 95.9 stn dist azm ain w phas calcphs hrmn tsec t-obs t-cal res wt di KIF 140 6.1 55.1 0 P PN4 029 29.9 20.30 21.44 -1.14 1.00 29 FI00 KIF 140 6.1 BAZ-P 169.2 186.4 -17.22 0.20 5 FI00 KIF 140 6.1 55.1 0 S SN4 029 46.4 36.80 37.30 -0.50 1.00 26 FI00 HEF 151 61.5 55.1 0 P PN4 029 32.5 22.86 22.74 0.11 1.00 9 FI00 KTK1 178 39.0 55.1 0 P PN4 029 36.2 26.61 26.13 0.48 1.00 4 NS00 STEI 219 276.4 55.1 0 P PN4 029 40.3 30.75 31.13 -0.39 1.00 10 NS00 FAUS 224 260.6 55.1 0 P PN4 029 40.9 31.34 31.73 -0.40 1.00 12 NS00 ARA0 283 44.3 55.1 0 P PN4 029 50.6 41.00 39.16 1.84 1.00 5 NO00 KTK1 HZ hdist: 178.6 amp: 2.5 T: 0.2 ml = 0.9 ARA0 HZ hdist: 283.4 amp: 2.2 T: 0.8 ml = 1.2 2016 1 1 0029 9.6 L 67.792 20.432 15.0 RRR 6 0.6 1.0LRRR OLD: 1 1 029 8.6 L 67.854 20.249 0.00 BER 6 .60 1.0LBER
BAZ means there is a back azimut for station KIF. For the Nordic2 format, it is shown that the BAZ is on the P. In addion, KIF has NTLO shown at the end of the line. At the end of listin is shown the original data (OLD) and the new hypocenter so it is easy to compare the effect of changing someting. In the print.out file there are details of the difference between the two hypocenters.
A station weight wt=-1 means that the phase travel time could not be calculated. The output phases can be e.g. PN2, where 2 means that the phase calculated has been refracted in layer 2 and PN5 refracted in layer 5. The input phase is then just P and a local model is used.
To get a statistics of which phases the program has used, run the program HYP_COUNT_PHASES. It uses the print.out file to count all types of local phases like PG, PN2 etc. For an example see, section "Inversion of travel time..."
Any change in the input phase ID is signified by an asterisk (*) before the phase ID.
If amplitudes are available, Ml, Mb. Mw or Ms will be calculated, and all stations calculating Ml, Mb, Mw or MS will additionally be displayed at the end of the interactive printout.
If the origin time of the located event occur on the day before the time in the header line, the time in the header line is changed to the previous day and all phase arrivals are changed accordingly. This means that some hour values will be more than 23 since phase arrival times refer to the main header.
Seismic moments etc: After locating an event, HYP will check if there is spectral information (Moment etc, see MULPLT) available in the S-file and average values will be calculated and written into the output file.