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hvidy / PIPE-4002-EarthByte-ModelAtlas

SIH repo for work on PIPE-4002
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Section 2 Parse Test #24

Open hvidy opened 5 months ago

hvidy commented 5 months ago

-> creator/contributor ORCID (or name)

0000-0002-6980-3392

-> slug

white_2017_pleiades

-> field of Research (FoR) Codes

510102,510109, 490304

-> license

CC-BY-4.0

-> model category

model published in study

-> associated publication DOI

https://doi.org/10.1029/2022GC010386

-> title

No response

-> description

No response

-> model authors

No response

-> scientific keywords

No response

-> funder

No response

-> include model code ?

-> model code URI/DOI

https://zenodo.org/records/5153073

-> include model output data?

-> model output URI/DOI

No response

-> software framework DOI/URI

No response

-> software framework source repository

No response

-> name of primary software framework (e.g. Underworld, ASPECT, Badlands, OpenFOAM)

No response

-> software framework authors

No response

-> software & algorithm keywords

No response

-> computer URI/DOI

No response

-> add landing page image and caption

No response

-> add an animation (if relevant)

No response

-> add a graphic abstract figure (if relevant)

No response

-> add a model setup figure (if relevant)

No response

-> add a description of your model setup

No response

github-actions[bot] commented 5 months ago

Thank you for submitting. Please check the output below, and fix any errors, etc.

Scientific keywords Warning: No keywords given Include model code? Error: both 'yes' and 'no' selected Model code URI/DOI 404 Client Error: NOT FOUND for url: https://zenodo.org/records/515-3073 Include model output data? Error: no selection made Model output URI/DOI Warning: No URI/DOI provided. Please check the output below to ensure its accuracy Creator/Contributor Creator/contributor is Timothy White (https://orcid.org/0000-0002-6980-3392)

Dumping dictionary during testing{'creator': {'@type': 'Person', '@id': 'https://orcid.org/0000-0002-6980-3392', 'givenName': 'Timothy', 'familyName': 'White', 'affiliation': [{'@type': 'Organization', 'name': 'University of Sydney'}]}, 'slug': 'white_2017_pleiades', 'for_codes': [{'@id': '#FoR_510102', '@type': 'DefinedTerm', 'name': 'Astronomical instrumentation'}, {'@id': '#FoR_510109', '@type': 'DefinedTerm', 'name': 'Stellar astronomy and planetary systems'}, {'@id': '#FoR_490304', '@type': 'DefinedTerm', 'name': 'Optimisation '}], 'license': {'name': 'Creative Commons Attribution 4.0 International', 'url': 'https://creativecommons.org/licenses/by/4.0/legalcode'}, 'model_category': ['model published in study'], 'publication': {'@type': 'ScholarlyArticle', '@id': 'http://dx.doi.org/10.1029/2022gc010386', 'name': 'The Role of Lithospheric‐Deep Mantle Interactions on the Style and Stress Evolution of Arc‐Continent Collision', 'isPartOf': ({'@type': 'PublicationIssue', 'issueNumber': '11', 'datePublished': '2022-11', 'isPartOf': {'@type': ['PublicationVolume', 'Periodical'], 'name': ['Geochemistry, Geophysics, Geosystems'], 'issn': ['1525-2027', '1525-2027'], 'volumeNumber': '23', 'publisher': 'American Geophysical Union (AGU)'}},), 'author': [{'@type': 'Person', '@id': 'http://orcid.org/0000-0002-1521-7910', 'givenName': 'Andrés Felipe', 'familyName': 'Rodríguez Corcho', 'affiliation': [{'@type': 'Organization', 'name': 'School of Geography, Earth and Atmospheric Sciences University of Melbourne Melbourne VIC Australia'}, {'@type': 'Organization', 'name': 'School of Geosciences University of Sydney Sydney NSW Australia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0002-1270-4377', 'givenName': 'Sara', 'familyName': 'Polanco', 'affiliation': [{'@type': 'Organization', 'name': 'School of Geosciences University of Sydney Sydney NSW Australia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0002-2594-6965', 'givenName': 'Rebecca', 'familyName': 'Farrington', 'affiliation': [{'@type': 'Organization', 'name': 'School of Geography, Earth and Atmospheric Sciences University of Melbourne Melbourne VIC Australia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0003-3891-5444', 'givenName': 'Romain', 'familyName': 'Beucher', 'affiliation': [{'@type': 'Organization', 'name': 'Research School of Earth Sciences Australian National University Canberra ACT Australia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0002-3553-0787', 'givenName': 'Camilo', 'familyName': 'Montes', 'affiliation': [{'@type': 'Organization', 'name': 'Department of Physics and Geosciences Universidad del Norte Barranquilla Colombia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0003-3685-174X', 'givenName': 'Louis', 'familyName': 'Moresi', 'affiliation': [{'@type': 'Organization', 'name': 'Research School of Earth Sciences Australian National University Canberra ACT Australia'}]}], 'abstract': 'We investigate how the mechanical properties of intra‐oceanic arcs affect the collision style and associated stress‐strain evolution with buoyancy‐driven models of subduction that accurately reproduce the dynamic interaction of the lithosphere and mantle. We performed a series of simulations only varying the effective arc thickness as it controls the buoyancy of intra‐oceanic arcs. Our simulations spontaneously evolve into two contrasting styles of collision that are controlled by a 3% density contrast between the arc and the continental plate. In simulations with less buoyant arcs (15–31\xa0km; effective thickness), we observe arc‐transference to the overriding plate and slab‐anchoring and folding at the 660\xa0km transition zone that result in fluctuations in the slab dip, strain‐stress regime, surface kinematics, and viscous dissipation. After slab‐folding occurs, the gravitational potential energy is dissipated in the form of lithospheric flow causing lithospheric extension in the overriding plate. Conversely, simulations with more buoyant arcs (32–35\xa0km; effective thickness) do not lead to arc‐transference and result in slab break‐off, which causes an asymptotic trend in surface kinematics, viscous dissipation and strain‐stress regime, and lithospheric extension in the overriding plate. The results of our numerical modeling highlight the importance of slab‐anchoring and folding in the 660\xa0km transition zone on increasing the mechanical coupling of the subduction system.', 'identifier': ['10.1029/2022GC010386'], 'funder': [{'@type': 'Organization', 'name': 'University of Melbourne'}]}, 'title': 'The Role of Lithospheric‐Deep Mantle Interactions on the Style and Stress Evolution of Arc‐Continent Collision', 'description': 'We investigate how the mechanical properties of intra‐oceanic arcs affect the collision style and associated stress‐strain evolution with buoyancy‐driven models of subduction that accurately reproduce the dynamic interaction of the lithosphere and mantle. We performed a series of simulations only varying the effective arc thickness as it controls the buoyancy of intra‐oceanic arcs. Our simulations spontaneously evolve into two contrasting styles of collision that are controlled by a 3% density contrast between the arc and the continental plate. In simulations with less buoyant arcs (15–31\xa0km; effective thickness), we observe arc‐transference to the overriding plate and slab‐anchoring and folding at the 660\xa0km transition zone that result in fluctuations in the slab dip, strain‐stress regime, surface kinematics, and viscous dissipation. After slab‐folding occurs, the gravitational potential energy is dissipated in the form of lithospheric flow causing lithospheric extension in the overriding plate. Conversely, simulations with more buoyant arcs (32–35\xa0km; effective thickness) do not lead to arc‐transference and result in slab break‐off, which causes an asymptotic trend in surface kinematics, viscous dissipation and strain‐stress regime, and lithospheric extension in the overriding plate. The results of our numerical modeling highlight the importance of slab‐anchoring and folding in the 660\xa0km transition zone on increasing the mechanical coupling of the subduction system.', 'authors': [{'@type': 'Person', '@id': 'http://orcid.org/0000-0002-1521-7910', 'givenName': 'Andrés Felipe', 'familyName': 'Rodríguez Corcho', 'affiliation': [{'@type': 'Organization', 'name': 'School of Geography, Earth and Atmospheric Sciences University of Melbourne Melbourne VIC Australia'}, {'@type': 'Organization', 'name': 'School of Geosciences University of Sydney Sydney NSW Australia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0002-1270-4377', 'givenName': 'Sara', 'familyName': 'Polanco', 'affiliation': [{'@type': 'Organization', 'name': 'School of Geosciences University of Sydney Sydney NSW Australia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0002-2594-6965', 'givenName': 'Rebecca', 'familyName': 'Farrington', 'affiliation': [{'@type': 'Organization', 'name': 'School of Geography, Earth and Atmospheric Sciences University of Melbourne Melbourne VIC Australia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0003-3891-5444', 'givenName': 'Romain', 'familyName': 'Beucher', 'affiliation': [{'@type': 'Organization', 'name': 'Research School of Earth Sciences Australian National University Canberra ACT Australia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0002-3553-0787', 'givenName': 'Camilo', 'familyName': 'Montes', 'affiliation': [{'@type': 'Organization', 'name': 'Department of Physics and Geosciences Universidad del Norte Barranquilla Colombia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0003-3685-174X', 'givenName': 'Louis', 'familyName': 'Moresi', 'affiliation': [{'@type': 'Organization', 'name': 'Research School of Earth Sciences Australian National University Canberra ACT Australia'}]}], 'keywords': [], 'funder': [{'@type': 'Organization', 'name': 'University of Melbourne'}]}

github-actions[bot] commented 5 months ago

Thank you for submitting. Please check the output below, and fix any errors, etc.

Scientific keywords Warning: No keywords given Model output URI/DOI Warning: No URI/DOI provided. Please check the output below to ensure its accuracy Creator/Contributor Creator/contributor is Timothy White (https://orcid.org/0000-0002-6980-3392)

Dumping dictionary during testing{'creator': {'@type': 'Person', '@id': 'https://orcid.org/0000-0002-6980-3392', 'givenName': 'Timothy', 'familyName': 'White', 'affiliation': [{'@type': 'Organization', 'name': 'University of Sydney'}]}, 'slug': 'white_2017_pleiades', 'for_codes': [{'@id': '#FoR_510102', '@type': 'DefinedTerm', 'name': 'Astronomical instrumentation'}, {'@id': '#FoR_510109', '@type': 'DefinedTerm', 'name': 'Stellar astronomy and planetary systems'}, {'@id': '#FoR_490304', '@type': 'DefinedTerm', 'name': 'Optimisation '}], 'license': {'name': 'Creative Commons Attribution 4.0 International', 'url': 'https://creativecommons.org/licenses/by/4.0/legalcode'}, 'model_category': ['model published in study'], 'publication': {'@type': 'ScholarlyArticle', '@id': 'http://dx.doi.org/10.1029/2022gc010386', 'name': 'The Role of Lithospheric‐Deep Mantle Interactions on the Style and Stress Evolution of Arc‐Continent Collision', 'isPartOf': ({'@type': 'PublicationIssue', 'issueNumber': '11', 'datePublished': '2022-11', 'isPartOf': {'@type': ['PublicationVolume', 'Periodical'], 'name': ['Geochemistry, Geophysics, Geosystems'], 'issn': ['1525-2027', '1525-2027'], 'volumeNumber': '23', 'publisher': 'American Geophysical Union (AGU)'}},), 'author': [{'@type': 'Person', '@id': 'http://orcid.org/0000-0002-1521-7910', 'givenName': 'Andrés Felipe', 'familyName': 'Rodríguez Corcho', 'affiliation': [{'@type': 'Organization', 'name': 'School of Geography, Earth and Atmospheric Sciences University of Melbourne Melbourne VIC Australia'}, {'@type': 'Organization', 'name': 'School of Geosciences University of Sydney Sydney NSW Australia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0002-1270-4377', 'givenName': 'Sara', 'familyName': 'Polanco', 'affiliation': [{'@type': 'Organization', 'name': 'School of Geosciences University of Sydney Sydney NSW Australia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0002-2594-6965', 'givenName': 'Rebecca', 'familyName': 'Farrington', 'affiliation': [{'@type': 'Organization', 'name': 'School of Geography, Earth and Atmospheric Sciences University of Melbourne Melbourne VIC Australia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0003-3891-5444', 'givenName': 'Romain', 'familyName': 'Beucher', 'affiliation': [{'@type': 'Organization', 'name': 'Research School of Earth Sciences Australian National University Canberra ACT Australia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0002-3553-0787', 'givenName': 'Camilo', 'familyName': 'Montes', 'affiliation': [{'@type': 'Organization', 'name': 'Department of Physics and Geosciences Universidad del Norte Barranquilla Colombia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0003-3685-174X', 'givenName': 'Louis', 'familyName': 'Moresi', 'affiliation': [{'@type': 'Organization', 'name': 'Research School of Earth Sciences Australian National University Canberra ACT Australia'}]}], 'abstract': 'We investigate how the mechanical properties of intra‐oceanic arcs affect the collision style and associated stress‐strain evolution with buoyancy‐driven models of subduction that accurately reproduce the dynamic interaction of the lithosphere and mantle. We performed a series of simulations only varying the effective arc thickness as it controls the buoyancy of intra‐oceanic arcs. Our simulations spontaneously evolve into two contrasting styles of collision that are controlled by a 3% density contrast between the arc and the continental plate. In simulations with less buoyant arcs (15–31\xa0km; effective thickness), we observe arc‐transference to the overriding plate and slab‐anchoring and folding at the 660\xa0km transition zone that result in fluctuations in the slab dip, strain‐stress regime, surface kinematics, and viscous dissipation. After slab‐folding occurs, the gravitational potential energy is dissipated in the form of lithospheric flow causing lithospheric extension in the overriding plate. Conversely, simulations with more buoyant arcs (32–35\xa0km; effective thickness) do not lead to arc‐transference and result in slab break‐off, which causes an asymptotic trend in surface kinematics, viscous dissipation and strain‐stress regime, and lithospheric extension in the overriding plate. The results of our numerical modeling highlight the importance of slab‐anchoring and folding in the 660\xa0km transition zone on increasing the mechanical coupling of the subduction system.', 'identifier': ['10.1029/2022GC010386'], 'funder': [{'@type': 'Organization', 'name': 'University of Melbourne'}]}, 'title': 'The Role of Lithospheric‐Deep Mantle Interactions on the Style and Stress Evolution of Arc‐Continent Collision', 'description': 'We investigate how the mechanical properties of intra‐oceanic arcs affect the collision style and associated stress‐strain evolution with buoyancy‐driven models of subduction that accurately reproduce the dynamic interaction of the lithosphere and mantle. We performed a series of simulations only varying the effective arc thickness as it controls the buoyancy of intra‐oceanic arcs. Our simulations spontaneously evolve into two contrasting styles of collision that are controlled by a 3% density contrast between the arc and the continental plate. In simulations with less buoyant arcs (15–31\xa0km; effective thickness), we observe arc‐transference to the overriding plate and slab‐anchoring and folding at the 660\xa0km transition zone that result in fluctuations in the slab dip, strain‐stress regime, surface kinematics, and viscous dissipation. After slab‐folding occurs, the gravitational potential energy is dissipated in the form of lithospheric flow causing lithospheric extension in the overriding plate. Conversely, simulations with more buoyant arcs (32–35\xa0km; effective thickness) do not lead to arc‐transference and result in slab break‐off, which causes an asymptotic trend in surface kinematics, viscous dissipation and strain‐stress regime, and lithospheric extension in the overriding plate. The results of our numerical modeling highlight the importance of slab‐anchoring and folding in the 660\xa0km transition zone on increasing the mechanical coupling of the subduction system.', 'authors': [{'@type': 'Person', '@id': 'http://orcid.org/0000-0002-1521-7910', 'givenName': 'Andrés Felipe', 'familyName': 'Rodríguez Corcho', 'affiliation': [{'@type': 'Organization', 'name': 'School of Geography, Earth and Atmospheric Sciences University of Melbourne Melbourne VIC Australia'}, {'@type': 'Organization', 'name': 'School of Geosciences University of Sydney Sydney NSW Australia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0002-1270-4377', 'givenName': 'Sara', 'familyName': 'Polanco', 'affiliation': [{'@type': 'Organization', 'name': 'School of Geosciences University of Sydney Sydney NSW Australia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0002-2594-6965', 'givenName': 'Rebecca', 'familyName': 'Farrington', 'affiliation': [{'@type': 'Organization', 'name': 'School of Geography, Earth and Atmospheric Sciences University of Melbourne Melbourne VIC Australia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0003-3891-5444', 'givenName': 'Romain', 'familyName': 'Beucher', 'affiliation': [{'@type': 'Organization', 'name': 'Research School of Earth Sciences Australian National University Canberra ACT Australia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0002-3553-0787', 'givenName': 'Camilo', 'familyName': 'Montes', 'affiliation': [{'@type': 'Organization', 'name': 'Department of Physics and Geosciences Universidad del Norte Barranquilla Colombia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0003-3685-174X', 'givenName': 'Louis', 'familyName': 'Moresi', 'affiliation': [{'@type': 'Organization', 'name': 'Research School of Earth Sciences Australian National University Canberra ACT Australia'}]}], 'keywords': [], 'funder': [{'@type': 'Organization', 'name': 'University of Melbourne'}], 'include_model_code': False, 'model_code_uri': 'https://zenodo.org/records/5153073'}

github-actions[bot] commented 5 months ago

Thank you for submitting. Please check the output below, and fix any errors, etc.

Errors and WarningsScientific keywords

Warning: No keywords given Model output URI/DOI Warning: No URI/DOI provided.

Parsed dataPlease check the output below to ensure its accuracy

Creator/Contributor Creator/contributor is Timothy White 0000-0002-6980-3392 Model Repository Slug Model repo will be created with name white_2017_pleiades Field of Research (FoR) Codes

github-actions[bot] commented 5 months ago

Thank you for submitting. Please check the output below, and fix any errors, etc.

Errors and Warnings

Scientific keywords Warning: No keywords given Model output URI/DOI Warning: No URI/DOI provided.

Parsed data

Please check the output below to ensure its accuracy Creator/Contributor Creator/contributor is Timothy White (0000-0002-6980-3392) Model Repository Slug Model repo will be created with name white_2017_pleiades Field of Research (FoR) Codes

License Creative Commons Attribution 4.0 International Model Category

Associated Publication Found publication: The Role of Lithospheric‐Deep Mantle Interactions on the Style and Stress Evolution of Arc‐Continent Collision Title The Role of Lithospheric‐Deep Mantle Interactions on the Style and Stress Evolution of Arc‐Continent Collision Description We investigate how the mechanical properties of intra‐oceanic arcs affect the collision style and associated stress‐strain evolution with buoyancy‐driven models of subduction that accurately reproduce the dynamic interaction of the lithosphere and mantle. We performed a series of simulations only varying the effective arc thickness as it controls the buoyancy of intra‐oceanic arcs. Our simulations spontaneously evolve into two contrasting styles of collision that are controlled by a 3% density contrast between the arc and the continental plate. In simulations with less buoyant arcs (15–31 km; effective thickness), we observe arc‐transference to the overriding plate and slab‐anchoring and folding at the 660 km transition zone that result in fluctuations in the slab dip, strain‐stress regime, surface kinematics, and viscous dissipation. After slab‐folding occurs, the gravitational potential energy is dissipated in the form of lithospheric flow causing lithospheric extension in the overriding plate. Conversely, simulations with more buoyant arcs (32–35 km; effective thickness) do not lead to arc‐transference and result in slab break‐off, which causes an asymptotic trend in surface kinematics, viscous dissipation and strain‐stress regime, and lithospheric extension in the overriding plate. The results of our numerical modeling highlight the importance of slab‐anchoring and folding in the 660 km transition zone on increasing the mechanical coupling of the subduction system. Model Authors

Scientific Keywords

Funder

github-actions[bot] commented 5 months ago

Thank you for submitting. Please check the output below, and fix any errors, etc.

Errors and Warnings

Scientific keywords Warning: No keywords given Model output URI/DOI Warning: No URI/DOI provided.

Parsed data

Please check the output below to ensure its accuracy

Creator/Contributor Creator/contributor is Timothy White (0000-0002-6980-3392)

Model Repository Slug Model repo will be created with name white_2017_pleiades

Field of Research (FoR) Codes

License Creative Commons Attribution 4.0 International

Model Category

Associated Publication Found publication: The Role of Lithospheric‐Deep Mantle Interactions on the Style and Stress Evolution of Arc‐Continent Collision

Title The Role of Lithospheric‐Deep Mantle Interactions on the Style and Stress Evolution of Arc‐Continent Collision

Description We investigate how the mechanical properties of intra‐oceanic arcs affect the collision style and associated stress‐strain evolution with buoyancy‐driven models of subduction that accurately reproduce the dynamic interaction of the lithosphere and mantle. We performed a series of simulations only varying the effective arc thickness as it controls the buoyancy of intra‐oceanic arcs. Our simulations spontaneously evolve into two contrasting styles of collision that are controlled by a 3% density contrast between the arc and the continental plate. In simulations with less buoyant arcs (15–31 km; effective thickness), we observe arc‐transference to the overriding plate and slab‐anchoring and folding at the 660 km transition zone that result in fluctuations in the slab dip, strain‐stress regime, surface kinematics, and viscous dissipation. After slab‐folding occurs, the gravitational potential energy is dissipated in the form of lithospheric flow causing lithospheric extension in the overriding plate. Conversely, simulations with more buoyant arcs (32–35 km; effective thickness) do not lead to arc‐transference and result in slab break‐off, which causes an asymptotic trend in surface kinematics, viscous dissipation and strain‐stress regime, and lithospheric extension in the overriding plate. The results of our numerical modeling highlight the importance of slab‐anchoring and folding in the 660 km transition zone on increasing the mechanical coupling of the subduction system.

Model Authors

Scientific Keywords

Funder

github-actions[bot] commented 5 months ago

Thank you for submitting. Please check the output below, and fix any errors, etc.

Errors and Warnings

Scientific keywords Warning: No keywords given Model output URI/DOI Warning: No URI/DOI provided.

Parsed data

Section 1: Summary of your model

Creator/Contributor Creator/contributor is Timothy White (0000-0002-6980-3392)

Model Repository Slug Model repo will be created with name white_2017_pleiades

Field of Research (FoR) Codes

License Creative Commons Attribution 4.0 International

Model Category

Associated Publication Found publication: The Role of Lithospheric‐Deep Mantle Interactions on the Style and Stress Evolution of Arc‐Continent Collision

Title The Role of Lithospheric‐Deep Mantle Interactions on the Style and Stress Evolution of Arc‐Continent Collision

Description We investigate how the mechanical properties of intra‐oceanic arcs affect the collision style and associated stress‐strain evolution with buoyancy‐driven models of subduction that accurately reproduce the dynamic interaction of the lithosphere and mantle. We performed a series of simulations only varying the effective arc thickness as it controls the buoyancy of intra‐oceanic arcs. Our simulations spontaneously evolve into two contrasting styles of collision that are controlled by a 3% density contrast between the arc and the continental plate. In simulations with less buoyant arcs (15–31 km; effective thickness), we observe arc‐transference to the overriding plate and slab‐anchoring and folding at the 660 km transition zone that result in fluctuations in the slab dip, strain‐stress regime, surface kinematics, and viscous dissipation. After slab‐folding occurs, the gravitational potential energy is dissipated in the form of lithospheric flow causing lithospheric extension in the overriding plate. Conversely, simulations with more buoyant arcs (32–35 km; effective thickness) do not lead to arc‐transference and result in slab break‐off, which causes an asymptotic trend in surface kinematics, viscous dissipation and strain‐stress regime, and lithospheric extension in the overriding plate. The results of our numerical modeling highlight the importance of slab‐anchoring and folding in the 660 km transition zone on increasing the mechanical coupling of the subduction system.

Model Authors

Funder

Section 2: your model code, output data

Include model code? True

Model code URI/DOI https://zenodo.org/records/5153073

Include model output data? False

Section 3: software framework and compute details

Section 4: web material (for mate.science)

Dumping dictionary during testing{'creator': {'@type': 'Person', '@id': 'https://orcid.org/0000-0002-6980-3392', 'givenName': 'Timothy', 'familyName': 'White', 'affiliation': [{'@type': 'Organization', 'name': 'University of Sydney'}]}, 'slug': 'white_2017_pleiades', 'for_codes': [{'@id': '#FoR_510102', '@type': 'DefinedTerm', 'name': 'Astronomical instrumentation'}, {'@id': '#FoR_510109', '@type': 'DefinedTerm', 'name': 'Stellar astronomy and planetary systems'}, {'@id': '#FoR_490304', '@type': 'DefinedTerm', 'name': 'Optimisation '}], 'license': {'name': 'Creative Commons Attribution 4.0 International', 'url': 'https://creativecommons.org/licenses/by/4.0/legalcode'}, 'model_category': ['model published in study'], 'publication': {'@type': 'ScholarlyArticle', '@id': 'http://dx.doi.org/10.1029/2022gc010386', 'name': 'The Role of Lithospheric‐Deep Mantle Interactions on the Style and Stress Evolution of Arc‐Continent Collision', 'isPartOf': ({'@type': 'PublicationIssue', 'issueNumber': '11', 'datePublished': '2022-11', 'isPartOf': {'@type': ['PublicationVolume', 'Periodical'], 'name': ['Geochemistry, Geophysics, Geosystems'], 'issn': ['1525-2027', '1525-2027'], 'volumeNumber': '23', 'publisher': 'American Geophysical Union (AGU)'}},), 'author': [{'@type': 'Person', '@id': 'http://orcid.org/0000-0002-1521-7910', 'givenName': 'Andrés Felipe', 'familyName': 'Rodríguez Corcho', 'affiliation': [{'@type': 'Organization', 'name': 'School of Geography, Earth and Atmospheric Sciences University of Melbourne Melbourne VIC Australia'}, {'@type': 'Organization', 'name': 'School of Geosciences University of Sydney Sydney NSW Australia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0002-1270-4377', 'givenName': 'Sara', 'familyName': 'Polanco', 'affiliation': [{'@type': 'Organization', 'name': 'School of Geosciences University of Sydney Sydney NSW Australia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0002-2594-6965', 'givenName': 'Rebecca', 'familyName': 'Farrington', 'affiliation': [{'@type': 'Organization', 'name': 'School of Geography, Earth and Atmospheric Sciences University of Melbourne Melbourne VIC Australia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0003-3891-5444', 'givenName': 'Romain', 'familyName': 'Beucher', 'affiliation': [{'@type': 'Organization', 'name': 'Research School of Earth Sciences Australian National University Canberra ACT Australia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0002-3553-0787', 'givenName': 'Camilo', 'familyName': 'Montes', 'affiliation': [{'@type': 'Organization', 'name': 'Department of Physics and Geosciences Universidad del Norte Barranquilla Colombia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0003-3685-174X', 'givenName': 'Louis', 'familyName': 'Moresi', 'affiliation': [{'@type': 'Organization', 'name': 'Research School of Earth Sciences Australian National University Canberra ACT Australia'}]}], 'abstract': 'We investigate how the mechanical properties of intra‐oceanic arcs affect the collision style and associated stress‐strain evolution with buoyancy‐driven models of subduction that accurately reproduce the dynamic interaction of the lithosphere and mantle. We performed a series of simulations only varying the effective arc thickness as it controls the buoyancy of intra‐oceanic arcs. Our simulations spontaneously evolve into two contrasting styles of collision that are controlled by a 3% density contrast between the arc and the continental plate. In simulations with less buoyant arcs (15–31\xa0km; effective thickness), we observe arc‐transference to the overriding plate and slab‐anchoring and folding at the 660\xa0km transition zone that result in fluctuations in the slab dip, strain‐stress regime, surface kinematics, and viscous dissipation. After slab‐folding occurs, the gravitational potential energy is dissipated in the form of lithospheric flow causing lithospheric extension in the overriding plate. Conversely, simulations with more buoyant arcs (32–35\xa0km; effective thickness) do not lead to arc‐transference and result in slab break‐off, which causes an asymptotic trend in surface kinematics, viscous dissipation and strain‐stress regime, and lithospheric extension in the overriding plate. The results of our numerical modeling highlight the importance of slab‐anchoring and folding in the 660\xa0km transition zone on increasing the mechanical coupling of the subduction system.', 'identifier': ['10.1029/2022GC010386'], 'funder': [{'@type': 'Organization', 'name': 'University of Melbourne'}]}, 'title': 'The Role of Lithospheric‐Deep Mantle Interactions on the Style and Stress Evolution of Arc‐Continent Collision', 'description': 'We investigate how the mechanical properties of intra‐oceanic arcs affect the collision style and associated stress‐strain evolution with buoyancy‐driven models of subduction that accurately reproduce the dynamic interaction of the lithosphere and mantle. We performed a series of simulations only varying the effective arc thickness as it controls the buoyancy of intra‐oceanic arcs. Our simulations spontaneously evolve into two contrasting styles of collision that are controlled by a 3% density contrast between the arc and the continental plate. In simulations with less buoyant arcs (15–31\xa0km; effective thickness), we observe arc‐transference to the overriding plate and slab‐anchoring and folding at the 660\xa0km transition zone that result in fluctuations in the slab dip, strain‐stress regime, surface kinematics, and viscous dissipation. After slab‐folding occurs, the gravitational potential energy is dissipated in the form of lithospheric flow causing lithospheric extension in the overriding plate. Conversely, simulations with more buoyant arcs (32–35\xa0km; effective thickness) do not lead to arc‐transference and result in slab break‐off, which causes an asymptotic trend in surface kinematics, viscous dissipation and strain‐stress regime, and lithospheric extension in the overriding plate. The results of our numerical modeling highlight the importance of slab‐anchoring and folding in the 660\xa0km transition zone on increasing the mechanical coupling of the subduction system.', 'authors': [{'@type': 'Person', '@id': 'http://orcid.org/0000-0002-1521-7910', 'givenName': 'Andrés Felipe', 'familyName': 'Rodríguez Corcho', 'affiliation': [{'@type': 'Organization', 'name': 'School of Geography, Earth and Atmospheric Sciences University of Melbourne Melbourne VIC Australia'}, {'@type': 'Organization', 'name': 'School of Geosciences University of Sydney Sydney NSW Australia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0002-1270-4377', 'givenName': 'Sara', 'familyName': 'Polanco', 'affiliation': [{'@type': 'Organization', 'name': 'School of Geosciences University of Sydney Sydney NSW Australia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0002-2594-6965', 'givenName': 'Rebecca', 'familyName': 'Farrington', 'affiliation': [{'@type': 'Organization', 'name': 'School of Geography, Earth and Atmospheric Sciences University of Melbourne Melbourne VIC Australia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0003-3891-5444', 'givenName': 'Romain', 'familyName': 'Beucher', 'affiliation': [{'@type': 'Organization', 'name': 'Research School of Earth Sciences Australian National University Canberra ACT Australia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0002-3553-0787', 'givenName': 'Camilo', 'familyName': 'Montes', 'affiliation': [{'@type': 'Organization', 'name': 'Department of Physics and Geosciences Universidad del Norte Barranquilla Colombia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0003-3685-174X', 'givenName': 'Louis', 'familyName': 'Moresi', 'affiliation': [{'@type': 'Organization', 'name': 'Research School of Earth Sciences Australian National University Canberra ACT Australia'}]}], 'keywords': [], 'funder': [{'@type': 'Organization', 'name': 'University of Melbourne'}], 'include_model_code': True, 'model_code_uri': 'https://zenodo.org/records/5153073', 'include_model_output': False}

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Section 1: Summary of your model

Creator/Contributor Creator/contributor is Timothy White (0000-0002-6980-3392)

Model Repository Slug Model repo will be created with name white_2017_pleiades

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License Creative Commons Attribution 4.0 International

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Associated Publication Found publication: The Role of Lithospheric‐Deep Mantle Interactions on the Style and Stress Evolution of Arc‐Continent Collision

Title The Role of Lithospheric‐Deep Mantle Interactions on the Style and Stress Evolution of Arc‐Continent Collision

Description We investigate how the mechanical properties of intra‐oceanic arcs affect the collision style and associated stress‐strain evolution with buoyancy‐driven models of subduction that accurately reproduce the dynamic interaction of the lithosphere and mantle. We performed a series of simulations only varying the effective arc thickness as it controls the buoyancy of intra‐oceanic arcs. Our simulations spontaneously evolve into two contrasting styles of collision that are controlled by a 3% density contrast between the arc and the continental plate. In simulations with less buoyant arcs (15–31 km; effective thickness), we observe arc‐transference to the overriding plate and slab‐anchoring and folding at the 660 km transition zone that result in fluctuations in the slab dip, strain‐stress regime, surface kinematics, and viscous dissipation. After slab‐folding occurs, the gravitational potential energy is dissipated in the form of lithospheric flow causing lithospheric extension in the overriding plate. Conversely, simulations with more buoyant arcs (32–35 km; effective thickness) do not lead to arc‐transference and result in slab break‐off, which causes an asymptotic trend in surface kinematics, viscous dissipation and strain‐stress regime, and lithospheric extension in the overriding plate. The results of our numerical modeling highlight the importance of slab‐anchoring and folding in the 660 km transition zone on increasing the mechanical coupling of the subduction system.

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Include model code? True

Model code URI/DOI https://zenodo.org/records/5153073

Include model output data? False

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Dumping dictionary during testing{'creator': {'@type': 'Person', '@id': 'https://orcid.org/0000-0002-6980-3392', 'givenName': 'Timothy', 'familyName': 'White', 'affiliation': [{'@type': 'Organization', 'name': 'University of Sydney'}]}, 'slug': 'white_2017_pleiades', 'for_codes': [{'@id': '#FoR_510102', '@type': 'DefinedTerm', 'name': 'Astronomical instrumentation'}, {'@id': '#FoR_510109', '@type': 'DefinedTerm', 'name': 'Stellar astronomy and planetary systems'}, {'@id': '#FoR_490304', '@type': 'DefinedTerm', 'name': 'Optimisation '}], 'license': {'name': 'Creative Commons Attribution 4.0 International', 'url': 'https://creativecommons.org/licenses/by/4.0/legalcode'}, 'model_category': ['model published in study'], 'publication': {'@type': 'ScholarlyArticle', '@id': 'http://dx.doi.org/10.1029/2022gc010386', 'name': 'The Role of Lithospheric‐Deep Mantle Interactions on the Style and Stress Evolution of Arc‐Continent Collision', 'isPartOf': ({'@type': 'PublicationIssue', 'issueNumber': '11', 'datePublished': '2022-11', 'isPartOf': {'@type': ['PublicationVolume', 'Periodical'], 'name': ['Geochemistry, Geophysics, Geosystems'], 'issn': ['1525-2027', '1525-2027'], 'volumeNumber': '23', 'publisher': 'American Geophysical Union (AGU)'}},), 'author': [{'@type': 'Person', '@id': 'http://orcid.org/0000-0002-1521-7910', 'givenName': 'Andrés Felipe', 'familyName': 'Rodríguez Corcho', 'affiliation': [{'@type': 'Organization', 'name': 'School of Geography, Earth and Atmospheric Sciences University of Melbourne Melbourne VIC Australia'}, {'@type': 'Organization', 'name': 'School of Geosciences University of Sydney Sydney NSW Australia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0002-1270-4377', 'givenName': 'Sara', 'familyName': 'Polanco', 'affiliation': [{'@type': 'Organization', 'name': 'School of Geosciences University of Sydney Sydney NSW Australia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0002-2594-6965', 'givenName': 'Rebecca', 'familyName': 'Farrington', 'affiliation': [{'@type': 'Organization', 'name': 'School of Geography, Earth and Atmospheric Sciences University of Melbourne Melbourne VIC Australia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0003-3891-5444', 'givenName': 'Romain', 'familyName': 'Beucher', 'affiliation': [{'@type': 'Organization', 'name': 'Research School of Earth Sciences Australian National University Canberra ACT Australia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0002-3553-0787', 'givenName': 'Camilo', 'familyName': 'Montes', 'affiliation': [{'@type': 'Organization', 'name': 'Department of Physics and Geosciences Universidad del Norte Barranquilla Colombia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0003-3685-174X', 'givenName': 'Louis', 'familyName': 'Moresi', 'affiliation': [{'@type': 'Organization', 'name': 'Research School of Earth Sciences Australian National University Canberra ACT Australia'}]}], 'abstract': 'We investigate how the mechanical properties of intra‐oceanic arcs affect the collision style and associated stress‐strain evolution with buoyancy‐driven models of subduction that accurately reproduce the dynamic interaction of the lithosphere and mantle. We performed a series of simulations only varying the effective arc thickness as it controls the buoyancy of intra‐oceanic arcs. Our simulations spontaneously evolve into two contrasting styles of collision that are controlled by a 3% density contrast between the arc and the continental plate. In simulations with less buoyant arcs (15–31\xa0km; effective thickness), we observe arc‐transference to the overriding plate and slab‐anchoring and folding at the 660\xa0km transition zone that result in fluctuations in the slab dip, strain‐stress regime, surface kinematics, and viscous dissipation. After slab‐folding occurs, the gravitational potential energy is dissipated in the form of lithospheric flow causing lithospheric extension in the overriding plate. Conversely, simulations with more buoyant arcs (32–35\xa0km; effective thickness) do not lead to arc‐transference and result in slab break‐off, which causes an asymptotic trend in surface kinematics, viscous dissipation and strain‐stress regime, and lithospheric extension in the overriding plate. The results of our numerical modeling highlight the importance of slab‐anchoring and folding in the 660\xa0km transition zone on increasing the mechanical coupling of the subduction system.', 'identifier': ['10.1029/2022GC010386'], 'funder': [{'@type': 'Organization', 'name': 'University of Melbourne'}]}, 'title': 'The Role of Lithospheric‐Deep Mantle Interactions on the Style and Stress Evolution of Arc‐Continent Collision', 'description': 'We investigate how the mechanical properties of intra‐oceanic arcs affect the collision style and associated stress‐strain evolution with buoyancy‐driven models of subduction that accurately reproduce the dynamic interaction of the lithosphere and mantle. We performed a series of simulations only varying the effective arc thickness as it controls the buoyancy of intra‐oceanic arcs. Our simulations spontaneously evolve into two contrasting styles of collision that are controlled by a 3% density contrast between the arc and the continental plate. In simulations with less buoyant arcs (15–31\xa0km; effective thickness), we observe arc‐transference to the overriding plate and slab‐anchoring and folding at the 660\xa0km transition zone that result in fluctuations in the slab dip, strain‐stress regime, surface kinematics, and viscous dissipation. After slab‐folding occurs, the gravitational potential energy is dissipated in the form of lithospheric flow causing lithospheric extension in the overriding plate. Conversely, simulations with more buoyant arcs (32–35\xa0km; effective thickness) do not lead to arc‐transference and result in slab break‐off, which causes an asymptotic trend in surface kinematics, viscous dissipation and strain‐stress regime, and lithospheric extension in the overriding plate. The results of our numerical modeling highlight the importance of slab‐anchoring and folding in the 660\xa0km transition zone on increasing the mechanical coupling of the subduction system.', 'authors': [{'@type': 'Person', '@id': 'http://orcid.org/0000-0002-1521-7910', 'givenName': 'Andrés Felipe', 'familyName': 'Rodríguez Corcho', 'affiliation': [{'@type': 'Organization', 'name': 'School of Geography, Earth and Atmospheric Sciences University of Melbourne Melbourne VIC Australia'}, {'@type': 'Organization', 'name': 'School of Geosciences University of Sydney Sydney NSW Australia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0002-1270-4377', 'givenName': 'Sara', 'familyName': 'Polanco', 'affiliation': [{'@type': 'Organization', 'name': 'School of Geosciences University of Sydney Sydney NSW Australia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0002-2594-6965', 'givenName': 'Rebecca', 'familyName': 'Farrington', 'affiliation': [{'@type': 'Organization', 'name': 'School of Geography, Earth and Atmospheric Sciences University of Melbourne Melbourne VIC Australia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0003-3891-5444', 'givenName': 'Romain', 'familyName': 'Beucher', 'affiliation': [{'@type': 'Organization', 'name': 'Research School of Earth Sciences Australian National University Canberra ACT Australia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0002-3553-0787', 'givenName': 'Camilo', 'familyName': 'Montes', 'affiliation': [{'@type': 'Organization', 'name': 'Department of Physics and Geosciences Universidad del Norte Barranquilla Colombia'}]}, {'@type': 'Person', '@id': 'http://orcid.org/0000-0003-3685-174X', 'givenName': 'Louis', 'familyName': 'Moresi', 'affiliation': [{'@type': 'Organization', 'name': 'Research School of Earth Sciences Australian National University Canberra ACT Australia'}]}], 'keywords': [], 'funder': [{'@type': 'Organization', 'name': 'University of Melbourne'}], 'include_model_code': True, 'model_code_uri': 'https://zenodo.org/records/5153073', 'include_model_output': False, 'software': {'@type': 'SoftwareApplication'}}