1 0.000000 0.000000 100.000000 SP001 2 0.000000 2.000000 101.000000 SP002 3 0.000000 4.000000 102.000000 SP003 4 0.000000 6.000000 103.000000 SP004 5 2.000000 2.000000 100.000000 VP001 6 3.000000 2.000000 100.000000 VP002 7 4.000000 2.000000 100.000000 VP003 8 5.000000 2.000000 100.000000 VP004 9 6.000000 2.000000 100.000000 VP005 10 7.000000 2.000000 100.000000 VP006 11 8.000000 2.000000 100.000000 VP007 12 9.000000 2.000000 100.000000 VP008 13 10.000000 2.000000 100.000000 VP009 14 11.000000 2.000000 100.000000 VP010 15 12.000000 2.000000 100.000000 VP011 16 13.000000 2.000000 100.000000 VP012 17 2.000000 8.000000 125.000000 VP050 18 3.000000 8.000000 125.000000 VP051 19 4.000000 8.000000 125.000000 VP052 20 5.000000 8.000000 125.000000 VP053 21 6.000000 8.000000 125.000000 VP054 22 7.000000 8.000000 125.000000 VP055 23 8.000000 8.000000 125.000000 VP056 24 9.000000 8.000000 125.000000 VP057 25 10.000000 8.000000 125.000000 VP058 26 11.000000 8.000000 125.000000 VP059 27 12.000000 8.000000 125.000000 VP060 28 13.000000 8.000000 125.000000 VP061The *.nez file contains the (N,E,Z) coordinates and must include the SP and VP labels that match the shots.txt and phones.txt files. If the SEG2 data files were converted to BSEGY format with EGG2SEG 3.1.6 we might have files 1001.seg through 1004.seg in our directory. We would then run setgeom with the following command:
setgeom shots.txt phones.txt samp0000.nez
where it is assumed that the *.nez file is as shown here. The output BSEGY files would be setg1001.seg through setg1004.seg. The header dump using BDUMP 4.0.1 of file setg1001.seg would look like this:
----------------------------------------------------------------------------------- Length = 1000 samples | Shot Elevation = 100.0 Sample Interval = 0.00050 sec. | Shot Depth = 0.0 Delay Time = 0 msec. | Up Hole Time = 0 msec Low Cut Filter = 8 Hz. | Shot X-COORD = 0.00 High Cut Filter = 500 Hz. | Shot Y-COORD = 0.00 Line ID: 001^@ | Shot Date (year.moday) = 1994.1117 Shot Orientation: | Shot Time (hr:min) = 11:46 Azimuth= 0 Deg. Vertical=180 Deg.| Charge Size (grams)= 0 ----------------------------------------------------------------------------------- TRACE|SHOT| STATION | OFFSET| RECEIVER |VERT|1STBRK|K-GAIN|AZI|VER| # |REC.|SHOT REC| | ELEV. X-COORD Y-COORD|FOLD|(SEC.)| (dB) | | | -----|----|---------|-------|----------------------------|--|------|------|---|---| 1 | 1| 001 001| 2.83| 100.00 2.00 2.00| 1|0.0000| 0 | 0|180| 2 | 1| 001 002| 3.61| 100.00 2.00 3.00| 1|0.0000| 0 | 0|180| 3 | 1| 001 003| 4.47| 100.00 2.00 4.00| 1|0.0000| 20 | 0|180| 4 | 1| 001 004| 5.39| 100.00 2.00 5.00| 1|0.0000| 20 | 0|180| 5 | 1| 001 005| 6.32| 100.00 2.00 6.00| 1|0.0000| 20 | 0|180| 6 | 1| 001 006| 7.28| 100.00 2.00 7.00| 1|0.0000| 40 | 0|180| 7 | 1| 001 007| 8.25| 100.00 2.00 8.00| 1|0.0000| 40 | 0|180| 8 | 1| 001 008| 9.22| 100.00 2.00 9.00| 1|0.0000| 40 | 0|180| 9 | 1| 001 009| 10.20| 100.00 2.00 10.00| 1|0.0000| 40 | 0|180| 10 | 1| 001 010| 11.18| 100.00 2.00 11.00| 1|0.0000| 40 | 0|180| 11 | 1| 001 011| 12.17| 100.00 2.00 12.00| 1|0.0000| 40 | 0|180| 12 | 1| 001 012| 13.15| 100.00 2.00 13.00| 1|0.0000| 40 | 0|180| 13 | 1| 001 050| 26.36| 125.00 8.00 2.00| 1|0.0000| 40 | 0|180| 14 | 1| 001 051| 26.46| 125.00 8.00 3.00| 1|0.0000| 40 | 0|180| 15 | 1| 001 052| 26.59| 125.00 8.00 4.00| 1|0.0000| 40 | 0|180| 16 | 1| 001 053| 26.76| 125.00 8.00 5.00| 1|0.0000| 40 | 0|180| 17 | 1| 001 054| 26.96| 125.00 8.00 6.00| 1|0.0000| 40 | 0|180| 18 | 1| 001 055| 27.20| 125.00 8.00 7.00| 1|0.0000| 40 | 0|180| 19 | 1| 001 056| 27.48| 125.00 8.00 8.00| 1|0.0000| 40 | 0|180| 20 | 1| 001 057| 27.78| 125.00 8.00 9.00| 1|0.0000| 40 | 0|180| 21 | 1| 001 058| 28.12| 125.00 8.00 10.00| 1|0.0000| 40 | 0|180| 22 | 1| 001 059| 28.50| 125.00 8.00 11.00| 1|0.0000| 40 | 0|180| 23 | 1| 001 060| 28.90| 125.00 8.00 12.00| 1|0.0000| 40 | 0|180| 24 | 1| 001 061| 29.33| 125.00 8.00 13.00| 1|0.0000| 40 | 0|180|Note that the line ID has a binary zero. We would fix that by dumping the headers with BHED 10.1.4, then editing that zero out, replacing it with perhaps a space or some other valid ASCII character. This would be followed by an upload of the edited header file into the *.seg data by a second run of BHED. Some renaming would be required. The flow would look like this:
bhed setg1001.seg 01.hed 1 (edit the file 01.hed, say with VI) bhed setg1001.seg 01.hed 0 mv bhedsetg.seg 1001.segThe final result would be over writing 1001.seg with the corrected header version.