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173 results for “Paleozoic”

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zenodo48/100

Global kinematics of tectonic plates and subduction zones since the late Paleozoic Era

<div>Global kinematics of tectonic plates and subduction zones since the late Paleozoic Era</div> <div>&nbsp;</div> <div>Alexander Young(1), Nicolas Flament(1), Kayla Maloney(2), Simon Williams(2), Kara Matthews(2), Sabin Zahirovic(2), Dietmar M&uuml;ller(2,3)</div> <div>&nbsp;</div> <div>1. The University of Wollongong, NSW 2522, Australia&nbsp;</div> <div>&nbsp;</div> <div>2. EarthByte Group, School of Geosciences, The University of Sydney, NSW 2006, Australia</div> <div>&nbsp;</div> <div>3. Sydney Informatics Hub, The University of Sydney, NSW 2006, Australia&nbsp;</div> <div>&nbsp;</div> <div>Contact: ajy321@uowmail.edu.au</div> <div>&nbsp;</div> <div>&nbsp;</div> <div>Supplementary Material</div> <div>&nbsp;</div> <div>We provide the digital plate model files (including rotations and geometries). These files allow for the visualisation and/or manipulation of the late Paleozoic to present-day (410-0 Ma) global plate motion model presented in this study.&nbsp;</div> <div>&nbsp;</div> <div>#########################################</div> <div>The digital plate model files are compatible with the open-source GPlates plate reconstruction software (<a href="https://www.gplates.org" target="_blank" rel="noopener">www.gplates.org</a>):</div> <div>&nbsp;</div> <div>(1) Rotations - Global rotation model that contains the reconstruction poles that describe the motions of the continents and oceans.</div> <div>- <strong>Global_250-0Ma_Young_et_al.rot</strong> (455 KB)</div> <div>-<strong> Global_410-250Ma_Young_et_al.rot</strong> (154 KB)</div> <div>&nbsp;</div> <div>(2) Plate polygons and boundary geometries - Topologically closed plate polygons are constructed from the intersection of ridges, transforms, subduction zones and other plate boundary geometries. These 'resolved topologies' are defined at 1 Myr intervals (410-0 Ma). The plate boundary geometries and plate polygons have been assigned plate reconstruction IDs to allow them to be reconstructed using the supplied rotation file.</div> <div>- <strong>Global_Mesozoic-Cenozoic_plate_bounds_Young_etal.gpml</strong> (36.5 MB)</div> <div>- <strong>Global_Paleozoic_plate_bounds_Young_etal.gpml</strong> (6.7 MB)</div> <div>- <strong>TopologyBuildingBlocks_Young_etal.gpml</strong> (2 MB) - this file is identical to M&uuml;ller et al. (2016)</div> <div>&nbsp;</div> <div>(3) Coastlines - Geometries of the present-day coastlines.</div> <div>- <strong>Global_coastlines_Young_et_al_low_res.shp</strong> (1.2 MB&nbsp; including auxiliary files, datum-WGS 1984)</div> <div>&nbsp;</div> <div>(4) Static polygons (optional) - Includes ocean isochron and terrane polygon geometries.</div> <div>- <strong>GlobalPresentDay_SPP_Young_etal.shp</strong> (1.4 MB inc. auxillary files, datum-WGS 1984)</div> <div>&nbsp;</div> <div>(5) Continental polygons (optional) - Includes continental terrane polygon geometries and excludes oceanic lithosphere.</div> <div>- <strong>PresentDay_ContPolygons_Young_etal.shp</strong> (451 KB inc. auxillary files, datum-WGS 1984)</div> <div>&nbsp;</div> <div>GPlates:&nbsp;</div> <div>To view the model, load all files in GPlates (either drag and drop files onto the globe OR from the navigation bar at the top of the screen click File -&gt; Open Feature Collection and select files). Both rotation files (1) and each of the three plate geometry files (2) need to be loaded for the model to work properly. It is recommended that coastlines (3) are loaded to see how the continents move, however only one coastline file is necessary (.gpml or .shp). The static polygons (4) and continental polygons (5) are optional.&nbsp;</div> <div>&nbsp;</div> <div>The two rotation files need to be 'connected' in order for the model to run continuously from 410 to 0 Ma. In the GPlates 'Layers' window (opened from the main navigation bar, click 'Window' -&gt; 'Show Layers') the rotation files will be highlighted yellow, yet only one will have a yellow tick next to it to signify it is being used. Click the small black triangle to the left the ticked rotation file. Under 'Inputs' -&gt; 'Reconstruction features' click 'Add new connection' and then select the other rotation file from the list of files that will appear. This will ensure that both rotation files are active.&nbsp;</div> <div>&nbsp;</div> <div>Finally, it is recommended to experiment with geometry visibility in order to make the globe less cluttered. For instance, from the navigation bar click View -&gt; Geometry Visibility and untick 'Show Line Geometries'. Alternatively, files can be toggled on and off using the tick boxes in the Layers window. For more information about using GPlates, a set of user tutorials can be accessed from the GPlates website - http://www.gplates.org/docs.html.</div> <div>&nbsp;</div> <div>&nbsp;</div> <div>#########################################</div> <div>MODEL REFERENCING:</div> <div>When using our model, in addition to citing this publication, please consider citing the studies of Domeier and Torsvik (2014), Matthews et al. (2016) and M&uuml;ller et al. (2016) which served as the basis for this model in the late Paleozoic and Mesozoic-Cenozoic, respectively, and citing any other study that describes refinements to the plate reconstructions in your region of interest as appropriate.&nbsp;</div> <div>&nbsp;</div> <div>- Domeier, M., &amp; Torsvik, T. H. (2014). Plate tectonics in the late Paleozoic. Geoscience Frontiers, 5(3), 303-350. DOI:&nbsp;<a href="https://doi.org/10.1016/j.gsf.2014.01.002" target="_blank" rel="noopener">10.1016/j.gsf.2014.01.002</a></div> <div>- M&uuml;ller, R. D., Seton, M., Zahirovic, S., Williams, S. E., Matthews, K. J., Wright, N. M., Shephard, G. E., Maloney, K., Barnett-Moore, N., Hosseinpour, M., Bower, D. J., &amp; Cannon, J. (2016). Ocean Basin Evolution and Global-Scale Plate Reorganization Events Since Pangea Breakup. Annual Review of Earth and Planetary Sciences, 44(1). DOI: <a href="https://doi.org/10.1146/annurev-earth-060115-012211" target="_blank" rel="noopener">10.1146/annurev-earth-060115-012211</a></div> <div>-Matthews, K. J., Maloney, K. T., Zahirovic, S., Williams, S. E., Seton, M., &amp; Mueller, R. D. (2016). Global plate boundary evolution and kinematics since the late Paleozoic. Global and Planetary Change, 146, 226-250.</div> <div>DOI: <a href="https://doi.org/10.1016/j.gloplacha.2016.10.002" target="_blank" rel="noopener">10.1016/j.gloplacha.2016.10.002</a></div>

opencc-by-4.0Jun 2018View details →
zenodo48/100

Global plate boundary evolution and kinematics since the late Paleozoic

<h3>Global plate boundary evolution and kinematics since the late Paleozoic&nbsp;</h3> <p>Kara J. Matthews*^, Kayla T. Maloney*, Sabin Zahirovic*, Simon E. Williams*, Maria Seton*, R. Dietmar M&uuml;ller*</p> <p>* EarthByte Group, School of Geosciences, The University of Sydney, Sydney, NSW 2006, Australia<br>^ Present address: Department of Earth Sciences, University of Oxford, South Parks Road, Oxford OX1 3AN, UK</p> <p>Contact: karajmatthews@gmail.com</p> <p>CORRECTION applied for the Pacific plate prior to 83 Ma based on Torsvik et al. (2019)</p> <h3><br>Supplementary Material</h3> <p>We provide a digital plate model files (including rotations and geometries) with this publication. These files allow for the visualisation and/or manipulation of the late Paleozoic to present-day (410-0 Ma) global plate motion model presented in this study.&nbsp;</p> <p>#########################################<br>The digital plate model files are compatible with the open-source GPlates plate reconstruction software (<a href="https://www.gplates.org" target="_blank" rel="noopener">www.gplates.org</a>):</p> <p>(1) Rotations - Global rotation model that contains the reconstruction poles that describe the motions of the continents and oceans.<br>- <strong>Global_EB_250-0Ma_GK07_Matthews_etal.rot</strong> (455 KB)<br>- <strong>Global_EB_410-250Ma_GK07_Matthews_etal.rot</strong> (115 KB) - in the comments 'POLE_RECALCULATED' means that we recalculated that finite pole of rotation such that the moving plate moves relative to a neighbouring plate rather than directly to the absolute reference frame (see Section 2.2.1 of the main text for more details). This process should have a minimal effect on the absolute motion of the plate.</p> <p>(2) Plate polygons and boundary geometries - Topologically closed plate polygons are constructed from the intersection of ridges, transforms, subduction zones and other plate boundary geometries. These 'resolved topologies' are valid at 1 Myr intervals (410-0 Ma). The plate boundary geometries and plate polygons have been assigned plate reconstruction IDs to allow them to be reconstructed using the supplied rotation file.<br>- <strong>Global_Mesozoic-Cenozoic_plate_bounds_Matthews_etal.gpml</strong> (36 MB)<br>- <strong>Global_Paleozoic_plate_bounds_Matthews_etal.gpml</strong> (8.7 MB)<br>- <strong>TopologyBuildingBlocks_Matthews_etal.gpml</strong> (2 MB) - this file has not been modified from M&uuml;ller et al. (2016)</p> <p>(3) Coastlines - Geometries of the present-day coastlines.<br>- <strong>Global_coastlines_low_res_Matthews_etal.gpml</strong> (25.4 MB)<br>- <strong>Global_coastlines_low_res_Matthews_etal.shp</strong> (2.9 MB &nbsp;inc. auxillary files, datum-WGS 1984)<br>NOTE: From 410 to 320-310 Ma Kazakhstania is represented as one or two ('Internal' and 'External' Kazakhstania - Domeier and Torsvik, 2014) ovate polygons. Kazakhstania is highly deformed following a long and complicated history, and so for simplicity we avoid using their present-day outlines in the earlier part of the model.</p> <p>(4) Static polygons (optional) - Includes ocean isochron and terrane polygon geometries.<br>- <strong>Global_EarthByte_GPlates_PresentDay_StaticPlatePolygons_Matthews_etal.shp</strong> (2.7 MB inc. auxillary files, datum-WGS 1984)</p> <p>(5) Continenal polygons (optional) - Includes continental terrane polygon geometries and excludes oceanic lithosphere.<br>- <strong>Global_EarthByte_GPlates_PresentDay_ContinentalPolygons_Matthews_etal.shp</strong> (804 KB inc. auxillary files, datum-WGS 1984)</p> <p>GPLATES:&nbsp;<br>To view the model load all files in GPlates (either drag and drop files onto the globe OR from the navigation bar at the top of the screen click File -&gt; Open Feature Collection and select files). Both rotation files (1) and each of the three plate geometry files (2) need to be loaded for the model to work properly. It is recommended that coastlines (3) are loaded to see how the continents move, however only one coastline file is necessary (.gpml or .shp). The static polygons (4) and continental polygons (5) are optional.&nbsp;</p> <p>The two rotation files need to be 'connected' in order for the model to run continuously from 410 to 0 Ma. In the GPlates 'Layers' window (opened from the main navigation bar, click 'Window' -&gt; 'Show Layers') the rotation files will be highlighted yellow, yet only one will have a yellow tick next to it to signify it is being used. Click the small black triangle to the left the ticked rotation file. Under 'Inputs' -&gt; 'Reconstruction features' click 'Add new connection' and then select the other rotation file from the list of files that will appear. This will ensure that both rotation files are active.&nbsp;</p> <p>Finally, it is recommended to experiment with geometry visibility in order to make the globe less cluttered. For instance, from the navigation bar click View -&gt; Geometry Visibility and untick 'Show Line Geometries'. Alternatively, files can be toggled on and off using the tick boxes in the Layers window. For more information about using GPlates, a set of user tutorials can be accessed from the GPlates website - http://www.gplates.org/docs.html.</p> <p><br>#########################################<br>We also provide a list of the plate reconstruction IDs used in the model:</p> <p>Plate IDs - A list of all the plate IDs used in the rotation and geometry files and their corresponding plate names.<br>-&nbsp;<strong>EarthByte_Plate_ID_Table_Matthews_etal.txt</strong> (33 KB)</p> <p>#########################################<br>MODEL REFERENCING:<br>When using our model, in addition to citing this publication:</p> <p>Matthews, K.J., Maloney, K.T., Zahirovic, S., Williams, S.E., Seton, M. and M&uuml;ller, R.D., 2016, Global plate boundary evolution and kinematics since the late Paleozoic, Global and Planetary Change, in press, accepted 3 October 2016.</p> <p>please also consider citing the studies of Domeier and Torsvik (2014) and M&uuml;ller et al. (2016) which served as the basis for this model in the late Paleozoic and Mesozoic-Cenozoic, respectively, and cite any other study that describes refinements to the plate reconstructions in your region of interest. See Section 2 and Section 3 of the main text for more information on how the present model was constructed.</p> <p>- Domeier, M., &amp; Torsvik, T. H. (2014). Plate tectonics in the late Paleozoic. Geoscience Frontiers, 5(3), 303-350. DOI:<a href="https://doi.org/10.1016/j.gsf.2014.01.002" target="_blank" rel="noopener">10.1016/j.gsf.2014.01.002</a><br>- M&uuml;ller, R. D., Seton, M., Zahirovic, S., Williams, S. E., Matthews, K. J., Wright, N. M., Shephard, G. E., Maloney, K., Barnett-Moore, N., Hosseinpour, M., Bower, D. J., &amp; Cannon, J. (2016). Ocean Basin Evolution and Global-Scale Plate Reorganization Events Since Pangea Breakup. Annual Review of Earth and Planetary Sciences, 44(1). DOI:<a href="https://doi.org/10.1146/annurev-earth-060115-012211" target="_blank" rel="noopener">10.1146/annurev-earth-060115-012211</a></p> <p>Note: We have recently fixed some issues in this model, namely the motion of the Pacific plate (following Torsvik et al., 2019), and some MOR topologies in the Arctic. The fixes are in the model files included in this folder, but the old (published) version of the model is included in a sub-folder called "_OLD_MODEL_DO_NOT_USE".&nbsp;</p> <p>Torsvik, T. H., B. Steinberger, G. E. Shephard, P. V. Doubrovine, C. Gaina, M. Domeier, C. P. Conrad, and W. W. Sager (2019), Pacific‐Panthalassic reconstructions: Overview, errata and the way forward, Geochemistry, Geophysics, Geosystems, 20(7), 3659-3689.</p> <p>&nbsp;</p>

opencc-by-4.0Oct 2016View details →
zenodo40/100

Fig. 64 in The Braincase In Paleozoic Symmoriiform And Cladoselachian Sharks

Fig. 64. ''Cobelodus''. Left side of head, with a reconstruction of main musculature associated with the jaws. No scale.

opencc-by-4.0Oct 2007View details →
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Fig. 63 in The Braincase In Paleozoic Symmoriiform And Cladoselachian Sharks

Fig. 63. ''Cobelodus''. Left side of head skeleton, with a reconstruction of the jaws and hyoid arch. No scale.

opencc-by-4.0Oct 2007View details →
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Fig. 62 in The Braincase In Paleozoic Symmoriiform And Cladoselachian Sharks

Fig. 62. Two early osteichthyan neurocrania in lateral view, showing positions of landmark features associated with the embryonic polar cartilage and antotic pila in modern gnathostomes. A, The primitive actinopterygian Ligulalepis sp., left side (after Basden and Young, 2001); B, The primitive sarcopterygian Achoania jarviki, right side of ethmosphenoid region (after Zhu et al., 2001; position of oculomotor foramen inferred from Psarolepis romeri, after Yu, 1998). Scale bars 5 5 mm.

opencc-by-4.0Oct 2007View details →
zenodo40/100

Fig. 60 in The Braincase In Paleozoic Symmoriiform And Cladoselachian Sharks

Fig. 60. Cladoselache sp., CMNH 5611, Cleveland Shale, Berea, Ohio. Ventral view of braincase lacking postorbital processes. Scale bar 5 10 mm.

opencc-by-4.0Oct 2007View details →
zenodo40/100

Fig. 59. Cladoselache kepleri, CMNH 6233 in The Braincase In Paleozoic Symmoriiform And Cladoselachian Sharks

Fig. 59. Cladoselache kepleri, CMNH 6233, Cleveland Shale, Berea, Ohio. Ventral view of braincase partly overlain by palatoquadrate. Scale bar 5 10 mm.

opencc-by-4.0Oct 2007View details →
zenodo40/100

Fig. 58. Cladoselache kepleri, CMNH 5769 in The Braincase In Paleozoic Symmoriiform And Cladoselachian Sharks

Fig. 58. Cladoselache kepleri, CMNH 5769, Cleveland Shale (late Devonian), Berea, Ohio. Ventral view of braincase. Scale bar 5 10 mm.

opencc-by-4.0Oct 2007View details →
zenodo40/100

Fig. 47 in The Braincase In Paleozoic Symmoriiform And Cladoselachian Sharks

Fig. 47. Cobelodus aculeatus FMNH PF 7345. Silicone peel of braincase dorsal surface, anterior to top

opencc-by-4.0Oct 2007View details →
zenodo40/100

Fig. 51 in The Braincase In Paleozoic Symmoriiform And Cladoselachian Sharks

Fig. 51. Outline dorsal views of the braincase in three specimens that have been referred to Stethacanthus, all from the Bear Gulch Limestone (Chesterian, late Pennsylvanian). A, Specimen referred to S. altonensis, MV 2830 (from Lund, 1974: fig. 3); B, specimen referred to S. cf. S. altonensis (from Lund, 1985: fig. 4); C, specimen referred to S. cf. S. productus (from Lund, 1985: fig. 1). Anterior to top. The original illustrations have been adjusted to approximately the same scale (scale bar 5 10 mm). See text for details.

opencc-by-4.0Oct 2007View details →
zenodo40/100

Fig. 55 in The Braincase In Paleozoic Symmoriiform And Cladoselachian Sharks

Fig. 55. Falcatus falcatus MV 4793, part and counterpart, Bear Gulch Limestone. Head in lateral view

opencc-by-4.0Oct 2007View details →
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Fig. 39 in The Braincase In Paleozoic Symmoriiform And Cladoselachian Sharks

Fig. 39. Cobelodus aculeatus FMNH PF 7347. Enlarged image of braincase, positive print from an original X-ray by R. Zangerl. Scale bar 5 10 mm.

opencc-by-4.0Oct 2007View details →
zenodo40/100

Fig. 42 in The Braincase In Paleozoic Symmoriiform And Cladoselachian Sharks

Fig. 42. ''Cobelodus'' contour-based surface rendering, ventral view with clipping plane introduced to remove parts of the basicranium, exposing the canal for the palatine ramus and the glossopharyngeal canal. Collapse of the basicranium below these structures (dashed white lines) creates paired ridges and depressions in compression fossils (see fig. 37).

opencc-by-4.0Oct 2007View details →
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Fig. 38. A in The Braincase In Paleozoic Symmoriiform And Cladoselachian Sharks

Fig. 38. A new silicone cranial endocast of Cobelodus aculeatus FMNH PF 3090. A, lateral view, right side; B, anterior view; C, dorsal view; D, ventral view; E, posterior view.

opencc-by-4.0Oct 2007View details →
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Fig. 32 in The Braincase In Paleozoic Symmoriiform And Cladoselachian Sharks

Fig. 32. Lateral view of the endocast in ''Cobelodus'' (A) and Cladodoides (B), showing different angular relationships of the plane containing the external semicircular canal (heavy line) to the endocast long axis (thinner line). Not to scale.

opencc-by-4.0Oct 2007View details →
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Fig. 43 in The Braincase In Paleozoic Symmoriiform And Cladoselachian Sharks

Fig. 43. ''Cobelodus'' CT scan, three-slice mode (digital reslicing of original transverse CT scan slices), showing orthographic views of the glossopharyngeal canal and surrounding cartilage. A, transverse slice; B, sagittal slice; C, horizontal slice. White lines correspond to x-y-z axes. Compare horizontal slice with figs. 37 and 38.

opencc-by-4.0Oct 2007View details →
zenodo40/100

Fig. 30 in The Braincase In Paleozoic Symmoriiform And Cladoselachian Sharks

Fig. 30. FMNH PF 13242 (''Cobelodus''). Endocast of otico-occipital and labyrinth regions, oblique orthographic views. A, postero-dorsolateral view; B, anterolateral view.

opencc-by-4.0Oct 2007View details →
zenodo40/100

Fig. 28 in The Braincase In Paleozoic Symmoriiform And Cladoselachian Sharks

Fig. 28. FMNH PF 13242 (''Cobelodus''). Cranial endocast, anterior views. A, entire endocast; B, endocast with anterior half removed.

opencc-by-4.0Oct 2007View details →
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Fig. 24 in The Braincase In Paleozoic Symmoriiform And Cladoselachian Sharks

Fig. 24. FMNH PF 13242 (''Cobelodus''). Contour-based surface reconstruction of cranial endocast generated from CT-scan slices. Right side, with semicircular canals and ampullae.

opencc-by-4.0Oct 2007View details →
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Fig. 23 in The Braincase In Paleozoic Symmoriiform And Cladoselachian Sharks

Fig. 23. Spino-occipital nerve canals in Cladodoides wildungensis for comparison with previous figure. A–D, CT scan slices through successive canals. Canal 1 is represented only by a slight embayment in the reconstruction and is poorly resolved in sectional views. A, canal 2 (does not widen or divide; CT scan slice 246); B, canal 3 (divides into dorsal and ventral branches; slice 260); C, canal 4 (widens externally but does not divide; slice 272); D, canal 5 (does not widen or divide; slice 287); E, medial view of digital reconstruction, showing location of spino-occipital canals.

opencc-by-4.0Oct 2007View details →

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