wphase:documentation
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wphase:documentation [2021/10/22 18:30] wphase [Extracting data from a gzipped tar archive] |
wphase:documentation [2021/10/22 18:42] wphase [RUNA scripts] |
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| ==== RUNA scripts ==== | ==== RUNA scripts ==== | ||
| - | Data extraction, screening and inversion described above can be performed by running one of the RUNA3*csh scripts (usually in bin). These scripts perform data extraction/screening and calculate a moment tensor solution after median data screening and after rejecting traces associated with large misfit using the threshold 5.0 3.0 0.9 (i.e. -th, see 2. in the "Inversion" section above): | + | Data screening and inversion can all be done at once using the RUNA3_lite.csh script: |
| + | <code> | ||
| + | ${WPHASE_HOME}/bin/RUNA3_lite.csh | ||
| + | </code> | ||
| + | This script can be used after data extraction in "DATA_org" using either "tgz2DATA_org.py" or "extract.csh" to extract data from a tgz archive or a SEED volume, respectively (see above). Once the "DATA_org" directory is populated, the "RUNA3_lite.csh" script will perform data screening and calculate a moment tensor solution after median data screening and after rejecting traces associated with large misfit using the threshold 5.0 3.0 0.9 (i.e. -th, see 2. in the "Inversion" section above). | ||
| + | |||
| + | If data is extracted directly from SEED volume(s), data extraction/screening and inversion can be done directly by running: | ||
| <code> | <code> | ||
| ${WPHASE_HOME}/bin/RUNA3.csh | ${WPHASE_HOME}/bin/RUNA3.csh | ||
| </code> | </code> | ||
| - | will perform median and rms misfit screening for Z, N, E, 1 and 2 channels, | + | To do the inversion on "Z" components only (i.e., not using the horizontals), use: |
| <code> | <code> | ||
| ${WPHASE_HOME}/bin/RUNA3_only_Z.csh | ${WPHASE_HOME}/bin/RUNA3_only_Z.csh | ||
| </code> | </code> | ||
| - | will perform median and rms misfit screening for Z channels only. | ||
| These two scripts don’t perform the “ratio screening” (i.e. 3. in the "Inversion" section above). To run the same routines with an additional screening based on the rms amplitude ratio (observed/predicted and predicted/observed), the following script can be used: | These two scripts don’t perform the “ratio screening” (i.e. 3. in the "Inversion" section above). To run the same routines with an additional screening based on the rms amplitude ratio (observed/predicted and predicted/observed), the following script can be used: | ||
| Line 165: | Line 170: | ||
| </code> | </code> | ||
| will perform median, rms misfit and rms ratio for channels Z, N, E, 1, 2 channels, | will perform median, rms misfit and rms ratio for channels Z, N, E, 1, 2 channels, | ||
| + | Warning: RUNAr.csh is not yet fully tested. | ||
| - | Remark: RUNAr.csh is not yet fully tested. | ||
| - | |||
| - | |||
| - | Several optional parameters can be used when running RUNA3*csh scripts. These parameters will apply to the wpinversion program. They are described when running wpinversion -h. | ||
| - | e.g.: RUNA3.csh -wz 1.0 -wn 0.3 -we 0.5 will give a weights of 1.0, 0.3 and 0.5 for Z, N, E components respectively. | ||
| - | |||
| - | To perform data screening and inversion only, using previously extracted SAC data, it is possible to use: | ||
| - | <code> | ||
| - | ${WPHASE_HOME}/bin/RUNA3_lite.csh | ||
| - | </code> | ||
| - | that is designed for Z, N ,Z ,1, 2 channels | ||
| ----- | ----- | ||
wphase/documentation.txt · Last modified: 2022/01/10 07:39 by wphase
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