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4 results for “Seismic tomography model”

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zenodo44/100

Gravity modeling of the Alpine lithosphere affected by magmatism based on seismic tomography

<p>The Southern Alpine regions have been affected by several magmatic and volcanic events between the Paleozoic and the Tertiary. This activity has undoubtedly had an important effect on the density distribution and structural setting at lithosphere scale. Combining the information from gravity field and a high-resolution seismic tomography has been carried out a new 3D lithosphere density model of the Alpine region.</p>

opencc-by-4.0Jun 2020View details →
zenodo44/100

DETOX seismic tomography models

<p>-----------------------<br> DETOX tomography models<br> -----------------------</p> <p>This folder contains three tomography models, DETOX-P1, DETOX-P2 and DETOX-P3, in the following formats:&nbsp;</p> <p>- NetCDF (dirname: grid_nc4)<br> - VTK (dirname: vtk)<br> - xyz-value (dirname: txt_tetrahedron)<br> - JPEG for GPLATES, only high-velocities (dirname: GPLATES)</p> <p>The directories are organized as follow:<br> &nbsp;<br> DETOX-P1<br> ├── GPLATES<br> ├── grid_nc4<br> ├── txt_tetrahedron<br> └── vtk<br> DETOX-P2<br> ├── GPLATES<br> ├── grid_nc4<br> ├── txt_tetrahedron<br> └── vtk<br> DETOX-P3<br> ├── GPLATES<br> ├── grid_nc4<br> ├── txt_tetrahedron<br> └── vtk</p> <p>---------------------</p> <p>Citation:</p> <p>* Kasra Hosseini, Karin Sigloch, Maria Tsekhmistrenko, Afsaneh Zaheri, Tarje Nissen-Meyer, Heiner Igel, Global mantle structure from multifrequency tomography using P, PP and P-diffracted waves, Geophysical Journal International, Volume 220, Issue 1, January 2020, Pages 96&ndash;141, https://doi.org/10.1093/gji/ggz394</p>

opencc-by-4.0Sep 2019View details →
zenodo32/100

A new lithospheric density and magnetic susceptibility model of Iran, starting from high resolution seismic tomography

<p>The Iranian collisional belt formed through&nbsp;different geological events, some of which are still in progress, such as the convergence between Eurasian and Arabian plates,&nbsp;that led to the formation of a complex structure&nbsp;throughout the entire area. To better investigate these structures, we realize a 3D&nbsp;model of the lithosphere in Iran showing the density and the magnetic susceptibility distribution, obtained from a Bayesian joint gravity and magnetic field&nbsp;inversion, starting from a&nbsp;high-resolution seismic tomography (Kaviani et al., 2020).&nbsp;With these models we also calculate the rigidity distribution of the area. The Data Cube uploaded&nbsp;contains the density, magnetic&nbsp;susceptibility and shear modulus volumes, the Bouguer gravity field and the&nbsp;magnetic field, and the Moho, Curie depth and&nbsp;sediment base depth surfaces.</p>

opencc-by-4.0Jun 2023View details →
zenodo24/100

Dataset and 3D Vs Model for "Crustal velocity images of north-western Türkiye along the North Anatolian Fault Zone from transdimensional Bayesian ambient seismic noise tomography"

<p>Final 3D Vs model and dispersion data&nbsp;for the paper entitled&nbsp;&quot;Crustal velocity images of north-western T&uuml;rkiye along the North Anatolian Fault Zone from transdimensional Bayesian ambient seismic noise tomography&quot;.</p> <p>In the vel_files folder, there are 10 files for each depth for 1-15 km. The format of each velocity&nbsp;file is as follows:</p> <p>Column&nbsp;&nbsp;&nbsp;&nbsp; Value<br> 1&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Lattitude (&deg;)<br> 2&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Longitude&nbsp;(&deg;)<br> 3&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Vs (km/s)</p> <p>The format of the dispersion data is as follows (See <a href="https://www.eas.slu.edu/eqc/eqc_cps/TUTORIAL/EMPIRICAL_GREEN/example1.html">Computer Programs in Seismology Tutorials - do_mft</a>&nbsp;for more information on the format):</p> <p>Column&nbsp;&nbsp;&nbsp;&nbsp; Value<br> 1&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Type of file, MFT96<br> 2&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Wave type: R for Rayleigh&nbsp;<br> 3&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Dispersion type:&nbsp; U for group velocity<br> 4&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Mode: 0 represents the fundamental mode<br> 5&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Filter period, T,&nbsp; in seconds<br> 6&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Dispersion value, either group or phase<br> 7&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Error in dispersion. This is just a place holder since there is no way to estimate an error from a single trace. The group velocity error is determined from the ratio of the filter period to travel time<br> 8&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Distance in km<br> 9&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Azimuth from the source to the receiver<br> 10&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Spectral amplitude.&nbsp;<br> 11&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Epicenter latitude&nbsp;<br> 12&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Epicenter longitude<br> 13&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Station latitude<br> 14&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Station longitude<br> 15&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; control flag<br> 16&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; control flag<br> 17&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Instantaneous period if this is preferred. This differs from the ilter period because the signal spectram is not flat.<br> 18&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Comment:&nbsp;&nbsp;&nbsp; keyword<br> 19&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Station&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;<br> 20&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Component<br> 21&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Year<br> 22&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Day of year<br> 23&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Hour<br> 24&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Minute&nbsp;&nbsp;&nbsp; - these identify the event origin time&nbsp;&nbsp;</p>

opencc-by-4.0Feb 2023View details →

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