Paraxial micro earthquake: a natural effective multi-purpose check shot for downhole earthquake monitoring
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| Format: | Preprint |
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2024
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| _version_ | 1866909319696482304 |
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| author | He, Ruiqing Paulsson, Bjorn |
| author_facet | He, Ruiqing Paulsson, Bjorn |
| contents | Downhole earthquake monitoring, without the effects from the overburden, can record better seismic data than monitoring on surface. However, in order to reasonably use the downhole vector seismic data, a constant challenge is how to accurately orient the downhole radial-component seismometers. A common practice is to use offset check shots on or near the surface. However, in areas with complex geologies, this routine may result in significant orientation errors. A ParAxial Micro Earthquake (PAME) is a micro earthquake at a close distance to the seismometers and near the extended path of the borehole's trajectory. It is rarely recorded during downhole earthquake monitoring unless designed for. If it is recorded, it can be a real treasure not only for P-wave and S-wave velocities' profiling, but for the downhole seismometers' orientation. As an example, during April to May in 2005, Paulsson installed an 80-level 3-component VSP (Vertical Seismic Profiling) array in the SAFOD (San Andreas Fault Observatory at Depth) main hole at Parkfield, California, and continuously recorded seismic data for about 13 days. Large charge offset check shots at 13 different locations near the surface were detonated in order to orient the downhole geophones; the orientation results were unsatisfactory but went unnoticed or unsolved. Besides this, a small charge "zero-offset" check shot was detonated near the wellhead in order to get the P-wave and S-wave velocity profiles, but only the P-wave velocity profiling was successful. Fortunately, we recorded a few PAMEs, through which we not only obtained better P-wave and S-wave velocity profiles, but satisfactorily oriented the downhole geophones. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2409_12442 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Paraxial micro earthquake: a natural effective multi-purpose check shot for downhole earthquake monitoring He, Ruiqing Paulsson, Bjorn Geophysics Downhole earthquake monitoring, without the effects from the overburden, can record better seismic data than monitoring on surface. However, in order to reasonably use the downhole vector seismic data, a constant challenge is how to accurately orient the downhole radial-component seismometers. A common practice is to use offset check shots on or near the surface. However, in areas with complex geologies, this routine may result in significant orientation errors. A ParAxial Micro Earthquake (PAME) is a micro earthquake at a close distance to the seismometers and near the extended path of the borehole's trajectory. It is rarely recorded during downhole earthquake monitoring unless designed for. If it is recorded, it can be a real treasure not only for P-wave and S-wave velocities' profiling, but for the downhole seismometers' orientation. As an example, during April to May in 2005, Paulsson installed an 80-level 3-component VSP (Vertical Seismic Profiling) array in the SAFOD (San Andreas Fault Observatory at Depth) main hole at Parkfield, California, and continuously recorded seismic data for about 13 days. Large charge offset check shots at 13 different locations near the surface were detonated in order to orient the downhole geophones; the orientation results were unsatisfactory but went unnoticed or unsolved. Besides this, a small charge "zero-offset" check shot was detonated near the wellhead in order to get the P-wave and S-wave velocity profiles, but only the P-wave velocity profiling was successful. Fortunately, we recorded a few PAMEs, through which we not only obtained better P-wave and S-wave velocity profiles, but satisfactorily oriented the downhole geophones. |
| title | Paraxial micro earthquake: a natural effective multi-purpose check shot for downhole earthquake monitoring |
| topic | Geophysics |
| url | https://arxiv.org/abs/2409.12442 |