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CVM-H
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The SCEC Community Velocity Model - Harvard (CVM-H) is a velocity model of crust and upper mantle structure in southern California developed by the SCEC community for use in fault systems analysis, strong ground motion prediction, and earthquake hazards assessment.
Perspective view of the northern part of CVM-H v15.1.0, showing an enlarged transect across the Los Angeles basin. An enlarged view of the shallow velocity structure in the basin shows the Geotechnical Layer (GTL), as described in the text. B) Cross sections showing Vp across the USR. LA is Los Angeles basin; SB is Santa Barbara basin; IB is Inner Borderland; ST is Salton Trough basin (Shaw et al., 2015)
Contents
Overview
Current Release
2.1
Known Issues
Dependencies
Documentation
Downloads
Supporting Materials
Help
Software License
Release History
10
Collaborators
11
CVM Evaluation
12
Alternative SCEC CVM's
13
Known Issue Description
14
Development version
15
Related Entries
16
See Also
17
References
Overview
The latest version of the SCEC Community Velocity Model (CVM-H 15.1.0) includes basin structures embedded in the 3D waveform inversion model of Tape et al. (2009), and an explicit representation of the Moho (after Yan and Clayton, 2007; Chulick and Mooney, 2002), and an optional arbitrary-precision Vs30-derived geotechnical layer for the top 350m (Ely et al 2011).
The SCEC CVM-H velocity model describes seismic P- and S-wave velocities and densities, and is comprised of basin structures embedded in tomographic and teleseismic crust and upper mantle models. This latest release of the CVM-H (15.1.0) represents the integration of various model components, including fully 3D waveform tomographic results. We recommend use of the most recent version of CVM-H, in most cases.
Improvements in version 15.1.0 include revisions to the basement surface that include the localization and displacements of faults in the Santa Maria Basin. This affects the boundary between the sediment and basement
velocity parameterizations.
Previous improvements that appeared in version 11.9, and also appear in 15.1.0, include a newly compiled Moho surface, opening up the offshore Santa Maria basin to the western model margin, a detailed representation of the San Bernardino basin, a much smoother transition between low resolution area and high resolution area at its southern border in the Los Angeles region and removal of various small near surface artifacts. The new Moho surface was compiled by Tape et al. from a large number of data sources, including global data sets, receiver functions and local studies. In replacing this surface care was taken that the depth interval around the Moho level both in the mantle and in the crustal portions of the model which were affected by this change, were assigned the correct domain, and consequently assigned velocities extrapolated from the underlying mantle model or from the crustal background model. In the offshore Santa Maria basin we extended the definition of the basement surface using reflection seismic data (McIntosh et al., 1991) to the very western margin of the model and to the north in order to remove an abrupt transition from the basin to background. We smoothly extrapolated sediment velocities from the onshore model into this new basinal area. Another basin, the relatively small San Bernardino basin, is now represented in the model. The basement surface is based on gravity data (Anderson, 2000) and seismic reflection data (Stephenson et al., 2004). To the west the basin is connected by a thin veneer of sediments to the Los Angeles basin whereas to the ESE the basin is represented as tapering out as is the case in other such basin representation. The ESE is the deepest part of the basin, and the data do not preclude a continuation of the basin in this direction. The Vp velocity structure in the basin is defined by stacking velocities (Stephenson et al., 2004) and a 1D velocity profile (Graves, 2004). Vs is derived from Vp using Brocher (2004). Finally, we removed a discontinuity in the velocity structure between the southern margin of the high resolution model in the Los Angeles area and the surrounding low resolution model. We modified the high resolution area by introducing a smooth N-S gradient in the delta between the low and high resolution models in a region at its southern margin.
The CVM-H 15.1.0 consists of basin structures defined using high-quality industry seismic reflection profiles and tens of thousands of direct velocity measurements from boreholes (Plesch et al., 2009; Süss and Shaw, 2003). The basin structures are also compatible with the locations and displacements of major faults represented in the
SCEC Community Fault Model (CFM)
(Plesch et al., 2007). These basin structures were used to develop travel time tomographic models of the crust (after Hauksson, 2000) extending to a depth of 35 km, and upper mantle teleseismic and surface wave models extending to a depth of 300 km (Prindle and Tanimoto, 2006). These various model components were integrated and used to perform a series of 3D adjoint tomographic inversions that highlight areas of the model that were responsible for mismatches between observed and synthetic waveforms (Tape et al, 2009). Sixteen tomographic iterations, requiring 6800 wavefield simulations, yielded perturbations to the starting model that have been incorporated in the latest model release. CVM-H 15.1.0 also incorporates a new Moho surface (Yan and Clayton, 2007) and an upgraded geotechnical layer (GTL) based on a Vs30 map (Ely 2010), the Vp-density scaling relationship, and the code that delivers the model.
Current Release
SCEC CVM-H version 15.1.0 was released on Wednesday 11 February 2015.
Version 15.1.0 includes revisions to the basement surface that include the localization and displacements of faults in the on-shore Santa Maria Basin. This affects the boundary between the sediment and basement velocity parameterizations.
Version 11.9.1 represents an improvement on 11.9.0 and it is recommended that all users upgrade to this new version. Specifically, the latest iteration includes the following changes to the high resolution (HR) data set:
replaced about ten, seemingly random cells which were shallow in the basin and had a water tag with sediment and GTL tags (GTL tags are obsolete and can be considered equivalent to sediment tag)
vp63: replaced water velocity in retagged cells with average from surrounding cells
vs65: replaced all sediment tagged cells with values based on Vp using Brocher (2005). This resulted mostly in no change but fixed some cells (about 8) which were close to the southern edge and had no-data or negative values
Known Issues
CVM-H 15.1.0:
None at this time.
Dependencies
The following software is required to build and run CVM-H.
UNIX operating system (tested on Linux and SunOS, untested on Solaris and MacOS)
GNU make
tar for opening the compressed files
GNU C compiler for building the executable program.
Optionally GTS (GNU Triangulated Surface Library) for cvmdist
Optionally GMT (Generic Mapping Tools) to generate plots from vx_slice
Documentation
User Guide Wiki (includes installation instructions):
CVM-H User Guide
Downloads
To install and use the CVM-H, you need to download and build the CVM-H software distribution. There are detailed installation instructions on the
CVM-H User Guide
. The main steps involved in installing CVM-H include:
The software can be installed in an account on a Linux computer with at least 600MB of disk storage and GNU C compiler and GNU compliant make.
From the Linux computer, start a web browser and point to this download page. Alternatively, you can retrieve the files with SFTP or other retrieval software.
Download the two CVM-H files (CVM-H source, CVM-H md5sum) into a directory and run the md5sum program to confirm you have an undamaged version of the distribution files.
Uncompress the distribution (tar.gz) files into a local directory on your computer.
Configure the installer by running the ./configure script.
Build the executables by running the top level makefile ('make').
Confirm the code is built correctly by running the unit/acceptance tests ('make check').
Install the executables ('make install').
Use CVM-H for research purposes.
Please note that, depending on your version of Linux or OS X, some additional steps may be required. If you run into the following error:
configure: error: cannot find install-sh, install.sh, or shtool in ./aux-config "."/./aux-config
Then please follow these steps:
Install automake. On Ubuntu this is sudo apt install automake. On Linux systems with Yum, the command is yum install automake.
Run aclocal
Run automake --force-missing --add-missing
Run autoconf
Run ./configure --prefix=/path/to/install/cvmh
Run make, make check, and make install
Platform
File
Mirror
Notes
Linux
SCEC CVM-H 15.1.1 Source (532 MB tar (tar.gz) file)
cvmh-15.1.1.tar.gz
Latest official release
Linux
SCEC CVM-H 15.1.1 md5 (small text file)
cvmh-15.1.1.tar.gz.md5
Latest official release
Supporting Materials
These posters and presentations may contain information about earlier versions of CVM-H. This information may be useful to some users.
Overview of CVM-H 11.2 (1Mb powerpoint file)
Overview of CVM-H 11.1 (1Mb powerpoint file)
Andreas Plesch Overview of CVM-H (2008) (7.4Mb powerpoint file)
CVM-H Poster SCEC Annual Meeting (2008) (1.8Mb pdf file)
Overview of SCEC Unified Structure Representation (USR) Developments (4.2Mb powerpoint file)
Help
For assistance with the SCEC CVM-H, you may:
Browse and submit new tickets at
CVM-H Trac
Email software (at) scec.org with specific questions
Subscribe to email list cvm-h-all (at) intensity.usc.edu to receive announcements about new version of the software.
Software License
CVM-H software distributions are released under an Apache 2.0 open-source license as described here
CVM-H License
Release History
The CVM-H releases contain cumulative improvements to the geological models and software interfaces. We recommend using the most recent version of the software, in most cases.
CVM-H 15.1.0 - February 2015
Added revisions to the basement surface that include the localization and displacements of faults in the Santa Maria Basin. This affects the boundary between the sediment and basement velocity parameterizations.
CVM-H 11.9.1 - December 2012
tag: replaced about ten, seemingly random cells which were shallow in the basin and had a water tag with sediment and GTL tags (GTL tags are obsolete and can be considered equivalent to sediment tag).
vp63: replaced water velocity in retagged cells with average from surrounding cells
vs65: replaced all sediment tagged cells with values based on Vp using Brocher (2005). This resulted mostly in no change but fixed some cells (about 8) which were close to the southern edge and had no-data or negative values.
CVM-H 11.9.0 - September 2011
This release included the Santa Maria and San Bernardino basins, and changes to the Moho.
CVM-H 11.2.0 - February 2011
This is the prior release, and the first release of CVM-H that includes the Vs30-based geotechnical layer, the Hadley-Kanamori 1D background model, and the vx_lite depth-based query user interface. This version also introduces a date-based version numbering scheme (Year.Month.Revision).
CVM-H 11.2.0 contains a small code error. Only exceptionally advanced users, users that write their own C language software to query CVM-H through the vx_api interface, might encounter this bug. For nearly all standard usages, the code works as designed. Details about this known issue are described at the end of this entry. A workaround for this bug is available and is described in the users manual. This issue will be fixed in the next release. See a description below, and the the online user guide
CVM-H User Guide
for an example that employs the work-around.
CVM-H 6.3capi - November 2010
This is an interim version of CVM-H for use in testing and evaluation. This version includes an initial version of the vx_lite interface but does not provide the Vs30-based geotechnical layer. This version is distributed for completeness and we do not recommended its use by researchers.
CVM-H 6.3 - September 2010
This version CVM-H, released by the Harvard Structural Geology Group, removes all
CVM-S
geotechnical information and restores the original CVM-H material properties to all regions of the model.
CVM-H 6.2 - January 2010
This version of CVM-H includes modifications to top 300m material properties based on geotechnical information extracted from
CVM-S
as an interim approach to providing near surface geotechnical information into CVM-H material properties database.
CVM-H 6.0 - September 2009
This version of CVM-H incorporates tomographic inversion results from Carl Tape et al.
CVM-H 5.5 - September 2008
This is the last version of CVM-H prior to integration of tomographic inversion results.
The
CVM-H User Guide
contains a comprehensive version history for CVM-H that is more complete than this summary including scientific references for each version.
Please Note: These distributions are "old" version of CVM-H. We strongly recommend you use the latest version of CVM-H posted above. These versions are only distributed to support projects that used them in the past.
Platform
File
Mirror
Notes
Linux
SCEC CVM-H 11.9.1 Source (550 Mb tar (tar.gz) file)
cvmh-11.9.1.tar.gz
Prior release
Linux
SCEC CVM-H 11.9.1 md5 (small text file)
cvmh-11.9.1.md5
Prior release
Linux
SCEC CVM-H 11.9.0 Source (529 Mb tar (tgz) file)
cvmh-11.9.0.tar.gz
cvmh-11.9.0.tar.gz
Prior release
Linux
SCEC CVM-H 11.9.0 md5 (small text file)
cvmh-11.9.0.tar.gz.md5
cvmh-11.9.0.tar.gz.md5
Prior release
Linux
SCEC CVM-H 11.2.0 Source (529 Mb tar (tgz) file)
cvmh_11.2.0.tgz
cvmh_11.2.0.tgz
Prior release
Linux
SCEC CVM-H 11.2.0 md5 (small text file)
cvmh_11.2.0.tgz.md5
cvmh_11.2.0.tgz.md5
Prior release
Collaborators
Harvard Structural Geology and Earth Resources Group Home Page
San Diego State University Dept of Geological Sciences
Po Chen Tomography
Geoff Ely Geotechnical Layer Implementation
Carl Tape Tomography
USGS CVM Web Site
USGS Pasadena
SCEC
SCEC/CME Project
CVM Evaluation
We have introduced
CVM Evaluation
tests as part of the CVM-H release process. In our
CVM Evaluation
system, we evaluate CVM's using earthquake wave propagation simulations. For each CVM, we build a velocity mesh for use in a 1Hz wave propagation simulation. We then run a wave propagation simulation using the CVM mesh under evaluation, and we run goodness-of-fit measures that compare the simulation result against observation data (seismograms). The SCEC
CVM Evaluation
system is designed to compare simulation results for alternative CVM models.
Alternative SCEC CVM's
As a part of the CVM-H release procedure, we are posting the software versions used to make the velocity meshes in our CVM evaluations. We are posting these version of the software so users can get most recent, and best available, versions of SCEC CVM codes.
For the CVM-H 11.9.0 release, our CVM evaluation system was used to evaluate it in comparison with CVM-H 11.2.0.
CVM-H 15.1.0 - This is the current CVM-H. This version of CVM-H is posted in the download section of this web page.
CVM-H 11.9.0 - This is the previous CVM-H.
CVM-H 11.2.0 - This is an older CVM-H and we tested it using a newly implemented Vs30-based geotechnical layer. This version of CVM-H is posted in the download section of this web page. CVM-H 11.2 is based on CVM-H 6.3 with the following differences (1) Arbitrary precision and optional Vs30-based geotechnical layer added, (2) a 1D Hadley-Kanamori background model added to extend model region, and (3) New query interface supports query by depth in addition to query by elevation.
For the CVM-H 11.2.0 release, our CVM evaluation system was used to evaluate three different CVM's for southern California, the current release and two alternative, or earlier, SCEC CVM's.
CVM-H 11.2 - This is the prior CVM-H and we tested it using a newly implemented Vs30-based geotechnical layer. This version of CVM-H is posted in the download section of this web page. CVM-H 11.2 is based on CVM-H 6.3 with the following differences (1) Arbitrary precision and optional Vs30-based geotechnical layer added, (2) a 1D Hadley-Kanamori background model added to extend model region, and (3) New query interface supports query by depth in addition to query by elevation.
CVM-H v6.3capi
(CVM-H v63 model w/ vx_lite and C API, w/o any GTL):
This is the previous version of CVM-H. The material properties in this CVM-H 6.3 version are equivalent to the material properties in CVM-H 11.2, except for the geotechnical layer. In CVM-H 11.2, the geotechnical layer is optional, and without GTL, CVM-H 11.2 should produce material properties equivalent to this CVM-H 6.3 version. We believe CVM-H 6.3 version we are distributing is equivalent to the CVM-H 6.3 released through the Harvard Structural Geology Web site. We are posting this distribution because it contains software we developed to implement query by depth. All capabilities in CFM-H 6.3 have been implemented in CVM-H 11.2 and we recommend all users use CVM-H 11.2 or later.
CVM-S
v4.1 (CVM-4 with Ely/Graves/Small mods):
This version of CVM-S4 includes fixes to all known software bugs in the 2005 distribution released through the SCEC data center, with additional modifications by Ely/Graves/Small to support querying with binary input files, and inclusion of an MPI query utility for large point sets, as well as a static library that allows the model to be queried programmatically. This is, to our knowledge, the best available version of CVM-S4.
CVM-S
4-gely (CVM-4 with Geoff Ely bug fixes):
This version of CVM-S4 includes fixes known bugs, such as un-initialized variables, in the original CVM-S distribution distributed through the SCEC Data Center. This is the version of CVM-S used in the CVM-H 11.2.0
CVM_Evaluation
. If you want to work with
CVM-S
, we recommend you use version
CVM-S
v4.1, posted above, as it contains additional changes and capabilities not in this version.
These distributions are available for download from the table below:
Please Note: These distributions are "old" version of CVM-S. We strongly recommend you use the latest version of CVM-S posted on the
CVM-S
page. These versions are only distributed to support projects that used them in the past.
File
Mirror
CVM-S v4.1
CVM-S v4.1 Source Code File (6.5 Mb tar (tgz) file)
cvms_v41.tgz
cvms_v41.tgz
CVM-S v4.1 Source Code md5sum File (small text file)
cvms_v41.tgz.md5
cvms_v41.tgz.md5
CVM-S 4-gely
CVM-S 4-gely Source Code File (6.5 Mb tar (tgz) file)
cvm4_gely_20101209.tar
cvm4_gely_20101209.tar
CVM-S 4-gely Source Code md5sum (small text file)
cvm4_gely_20101209.tar.md5
cvm4_gely_20101209.tar.md5
Known Issue Description
CVM-H 11.2.0 is known to contain a small code error. Only advanced users might encounter this bug. For nearly all standard usages, the code works as designed.
The vx_api library has a bug in query by depth mode. The structure member vx_entry_t.coord[2] (z value) gets altered during a vx_getcoord() call from depth to elevation when querying below the GTL. This value should not be changed during the call. The work-around for this issue is to make a copy of the depth value before the call to vx_getcoord() if you wish to use that depth later. The vx_lite command line tool does not exhibit this bug. This issue will be fixed in the next release. See the online user guide
CVM-H User Guide
for an example that employs the work-around.
Development version
If you're interested in working with the latest development version of the platform, you can check it out from:
svn co
Details about working with the development version are provided in the User Guide.
Related Entries
Harvard Structural Geology and Earth Resources Web Page
Harvard Community Velocity Model
Goodness of Fit
CVM-S
CVM-H v6.3capi
CVM Toolkit
CVM Evaluation
Community Velocity Model
CVM-H User Guide
CVM Toolkit
UCVM
Geotechnical Layer
See Also
SCEC Software Downloads
SCEC Wiki Main
SCEC Home Page
References
Shaw, John H., Plesch, Andreas, Tape, Carl, Suess, M. Peter, Jordan, Thomas H., Ely, Geoffrey, Hauksson, Egill, Tromp, Jeroen, Tanimoto, Toshiro, Graves, Robert, Olsen, Kim, Nicholson, Craig, Maechling, Philip J., Rivero, Carlos, Lovely, Peter, Brankman, Charles M., Munster, Jason (2015)
Unified Structural Representation of the southern California crust and upper mantle, Earth and Planetary Science Letters, V. 415, Num. 0, p.1-15,
Suess, M. P., and J. H. Shaw, 2003:
P-wave seismic velocity structure derived from sonic logs and industry reflection data in the Los Angeles basin, California, Journal of Geophysical Research, 108/B3.
Plesch, A., C. Tape, J. H. Shaw, and members of the USR working group, 2009, CVM-H 6.0:
Inversion integration, the San Joaquin Valley and other advances in the community velocity model, in 2009 Southern California Earthquake Center Annual Meeting, Proceedings and Abstracts, vol. 19, pp. 260–261.
Tape, C., Q. Liu, A. Maggi, and J. Tromp, 2009:
Adjoint tomography of the southern California crust, Science, v. 325, p. 988-992.
Ely, G., 2010:
Vs30 Derived GTL
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This page was last edited on 5 November 2019, at 17:44.
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