| Name | python-seispy JSON |
| Version |
1.3.7
JSON |
| download |
| home_page | None |
| Summary | None |
| upload_time | 2024-05-06 16:09:18 |
| maintainer | None |
| docs_url | None |
| author | Mijian Xu |
| requires_python | None |
| license | GPLv3 |
| keywords |
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| VCS |
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| bugtrack_url |
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| requirements |
No requirements were recorded.
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No Travis.
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| coveralls test coverage |
No coveralls.
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# <img src="https://user-images.githubusercontent.com/7437523/128596331-dc5c5e40-93e1-4d9e-b92d-9c53fe51145a.png" width="500"/>
[]()
[]()
[]()
[]()
[](https://doi.org/10.1785/0220220288)
[](https://github.com/xumi1993/seispy/actions/workflows/test.yml)
[](https://codecov.io/gh/xumi1993/seispy)
[](https://github.com/xumi1993/seispy/actions/workflows/python-publish.yml)
[](https://github.com/xumi1993/seispy/actions/workflows/doc_build.yml)
<a href="https://dev.azure.com/conda-forge/feedstock-builds/_build/latest?definitionId=13623&branchName=master">
<img src="https://dev.azure.com/conda-forge/feedstock-builds/_apis/build/status/seispy-feedstock?branchName=master">
</a>
[](https://anaconda.org/conda-forge/seispy)
[](https://anaconda.org/conda-forge/seispy)
[](https://anaconda.org/conda-forge/seispy)
[](https://pypi.org/project/python-seispy/)
[](https://pypi.org/project/python-seispy/)
[]()
[]()
Seispy is a Python module for processing seismological data and calculating Receiver Functions. The advanced functions are available to improve the Obspy.
## Acknowledgements
For the use of the Seispy package, please cite as:
- Xu, M. & He, J. (2023). Seispy: Python Module for Batch Calculation and Postprocessing of Receiver Functions. Seismological Research Letters, 94 (2A): 935–943. [](https://doi.org/10.1785/0220220288)
For 3D time-difference correction, please also consider citing:
- Xu, M., Huang, H., Huang, Z., Wang, P., Wang, L., Xu, M., ... & Yuan, X. (2018). Insight into the subducted Indian slab and origin of the Tengchong volcano in SE Tibet from receiver function analysis. Earth and Planetary Science Letters, 482, 567-579. [
](https://doi.org/10.1785/0220220288)
- Xu, M., Huang, Z., Wang, L., Xu, M., Mi, N., & Yu, D. (2020). Lateral variation of the mantle transition zone beneath the Tibetan plateau: Insight into thermal processes during Indian–Asian collision. Physics of the Earth and Planetary Interiors, 301, 106452. [](https://doi.org/10.1016/j.pepi.2020.106452)
For 2D and 3D CCP stacking, please also consider citing:
- Xu, M., Huang, Z., Wang, L., Xu, M., Zhang, Y., Mi, N., ... & Yuan, X. (2020). Sharp lateral Moho variations across the SE Tibetan margin and their implications for plateau growth. Journal of Geophysical Research: Solid Earth, 125(5), e2019JB018117. [](https://doi.org/10.1029/2019JB018117)
## Installation
See [Seispy documentation](https://seispy.xumijian.me/installation.html) in detail.
## Libraries
- `seispy.distaz`: Calculate distance and azimuth credited by the [lithospheric seismology program at USC](http://www.seis.sc.edu/software/distaz/), but `numpy.ndarray` operations are supported.
- `seispy.geo`: Tiny codes of geophysics.
- `seispy.decon`: Functions of deconvolution transferred from [iwbailey/processRFmatlab](https://github.com/iwbailey/processRFmatlab) including
- Iterative time domain deconvolution method (Ligorría and Ammon 1999 BSSA).
- Water level frequency domain deconvolution method (CJ. Ammon 1991 BSSA)
- `seispy.rf`: Procedure for RF calculation. The functions of `match_eq`, `search_eq` invoked `obspy.core.UTCDateTime` and `obspy.clients` from the [Obspy](https://docs.obspy.org/).
- `seispy.eq`: RF processing for each event, which invoked `obspy.io.sac`, `obspy.signal`, `obspy.taup` and `obspy.core.Stream` from the [Obspy](https://docs.obspy.org/).
- `seispy.hk`: H-k stacking for single station (Zhu and Kanamori 2000 JGR).
- `seispy.rfani`: A joint method for crustal anisotropic calculation (Liu and Niu 2011 GJI).
- `seispy.slantstack`: Slant stacking for single station (Tauzin et al., 2008)
- `seispy.rfcorrect`: Subsequent process of RFs including moveout correction and time to depth conversion (1D and 3D) (see [Xu et al., 2018 EPSL](https://www.sciencedirect.com/science/article/pii/S0012821X17306921?via%3Dihub))
- `seispy.ccpprofile`: CCP stacking along a profile.
- `seispy.ccp3d`: 3-D CCP stacking with extracting depth D410 and D660.
[lithospheric seismology program at USC]: http://www.seis.sc.edu/software/distaz/
[scikits-bootstrap]: https://github.com/cgevans/scikits-bootstrap
[iwbailey/processRFmatlab]: https://github.com/iwbailey/processRFmatlab
[Obspy]: https://docs.obspy.org/
[Xu et al., 2018 EPSL]: https://www.sciencedirect.com/science/article/pii/S0012821X17306921?via%3Dihub
## Commands
### Receiver Functions
* `prf`: Calculate PRFs for a station.
* `pickrf`: Pick PRFs with virtual quality control after the calculation.
* `plotrt`: Plot PRFs with R and T components order by back-azimuth.
* `plotr`: Plot PRFs with R component order by back-azimuth.
* `hk`: H-Kappa stacking for estimating Moho depth and crustal Vp/Vs.
* `rf2depth`: Convert PRFs to depth axis.
* `ccp_profile`: Stack PRFs along a profile with a CCP stacking method.
* `ccp3d`: Stack PRFs with spaced bins.
* `rfani`: Estimating crustal anisotropy with a joint method.
* `rfharmo`: Harmonic decomposition to extract constant component of RF and plot dip/anisotropic components.
* `pickdepth`: Pick depth of stacked PRFs following `ccp3d`
### Others
* `veltxt2mod`: Create 3D velocity model with `numpy.lib.npyio.NpzFile` format from a ASCII table file.
* `downlod_catalog`: Download catalogs from FDSN web-service.
* `gen_rayp_lib`: Generate a rap-parameter library with depth of source and epicentral distance.
* `setpar`: Set up the values in configure files.
Raw data
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The advanced functions are available to improve the Obspy.\n\n## Acknowledgements\n\nFor the use of the Seispy package, please cite as:\n\n- Xu, M. & He, J. (2023). Seispy: Python Module for Batch Calculation and Postprocessing of Receiver Functions. Seismological Research Letters, 94 (2A): 935\u2013943. [](https://doi.org/10.1785/0220220288)\n\nFor 3D time-difference correction, please also consider citing:\n\n- Xu, M., Huang, H., Huang, Z., Wang, P., Wang, L., Xu, M., ... & Yuan, X. (2018). Insight into the subducted Indian slab and origin of the Tengchong volcano in SE Tibet from receiver function analysis. Earth and Planetary Science Letters, 482, 567-579. [\n](https://doi.org/10.1785/0220220288)\n\n- Xu, M., Huang, Z., Wang, L., Xu, M., Mi, N., & Yu, D. (2020). Lateral variation of the mantle transition zone beneath the Tibetan plateau: Insight into thermal processes during Indian\u2013Asian collision. Physics of the Earth and Planetary Interiors, 301, 106452. [](https://doi.org/10.1016/j.pepi.2020.106452)\n\nFor 2D and 3D CCP stacking, please also consider citing:\n\n- Xu, M., Huang, Z., Wang, L., Xu, M., Zhang, Y., Mi, N., ... & Yuan, X. (2020). Sharp lateral Moho variations across the SE Tibetan margin and their implications for plateau growth. Journal of Geophysical Research: Solid Earth, 125(5), e2019JB018117. [](https://doi.org/10.1029/2019JB018117)\n\n## Installation\n\nSee [Seispy documentation](https://seispy.xumijian.me/installation.html) in detail.\n \n## Libraries\n- `seispy.distaz`: Calculate distance and azimuth credited by the [lithospheric seismology program at USC](http://www.seis.sc.edu/software/distaz/), but `numpy.ndarray` operations are supported.\n- `seispy.geo`: Tiny codes of geophysics.\n- `seispy.decon`: Functions of deconvolution transferred from [iwbailey/processRFmatlab](https://github.com/iwbailey/processRFmatlab) including\n - Iterative time domain deconvolution method (Ligorr\u00eda and Ammon 1999 BSSA). \n - Water level frequency domain deconvolution method (CJ. Ammon 1991 BSSA)\n- `seispy.rf`: Procedure for RF calculation. The functions of `match_eq`, `search_eq` invoked `obspy.core.UTCDateTime` and `obspy.clients` from the [Obspy](https://docs.obspy.org/).\n- `seispy.eq`: RF processing for each event, which invoked `obspy.io.sac`, `obspy.signal`, `obspy.taup` and `obspy.core.Stream` from the [Obspy](https://docs.obspy.org/).\n- `seispy.hk`: H-k stacking for single station (Zhu and Kanamori 2000 JGR).\n- `seispy.rfani`: A joint method for crustal anisotropic calculation (Liu and Niu 2011 GJI).\n- `seispy.slantstack`: Slant stacking for single station (Tauzin et al., 2008)\n- `seispy.rfcorrect`: Subsequent process of RFs including moveout correction and time to depth conversion (1D and 3D) (see [Xu et al., 2018 EPSL](https://www.sciencedirect.com/science/article/pii/S0012821X17306921?via%3Dihub))\n- `seispy.ccpprofile`: CCP stacking along a profile.\n- `seispy.ccp3d`: 3-D CCP stacking with extracting depth D410 and D660.\n\n [lithospheric seismology program at USC]: http://www.seis.sc.edu/software/distaz/\n [scikits-bootstrap]: https://github.com/cgevans/scikits-bootstrap\n [iwbailey/processRFmatlab]: https://github.com/iwbailey/processRFmatlab\n [Obspy]: https://docs.obspy.org/\n [Xu et al., 2018 EPSL]: https://www.sciencedirect.com/science/article/pii/S0012821X17306921?via%3Dihub\n\n\n## Commands\n### Receiver Functions\n * `prf`: Calculate PRFs for a station.\n * `pickrf`: Pick PRFs with virtual quality control after the calculation.\n * `plotrt`: Plot PRFs with R and T components order by back-azimuth.\n * `plotr`: Plot PRFs with R component order by back-azimuth.\n * `hk`: H-Kappa stacking for estimating Moho depth and crustal Vp/Vs.\n * `rf2depth`: Convert PRFs to depth axis.\n * `ccp_profile`: Stack PRFs along a profile with a CCP stacking method.\n * `ccp3d`: Stack PRFs with spaced bins.\n * `rfani`: Estimating crustal anisotropy with a joint method.\n * `rfharmo`: Harmonic decomposition to extract constant component of RF and plot dip/anisotropic components.\n * `pickdepth`: Pick depth of stacked PRFs following `ccp3d`\n\n### Others\n * `veltxt2mod`: Create 3D velocity model with `numpy.lib.npyio.NpzFile` format from a ASCII table file.\n * `downlod_catalog`: Download catalogs from FDSN web-service.\n * `gen_rayp_lib`: Generate a rap-parameter library with depth of source and epicentral distance.\n * `setpar`: Set up the values in configure files.\n\n",
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