github-actions[bot]
commented
5 months ago Thank you for submitting. Please check the output below, and fix any errors, etc.
Errors and Warnings
Include model output data?
Error: no selection made
Model output URI/DOI
Warning: No URI/DOI provided.
Software Framework DOI/URI
Error: unable to obtain metadata for DOI org/records/5153073
name 'parse_software' is not defined
Name of primary software framework
Error: no name found
Software framework authors
Error: no authors found
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
#FoR_510102: Astronomical instrumentation#FoR_510109: Stellar astronomy and planetary systems#FoR_490304: Optimisation
License Creative Commons Attribution 4.0 International
Model Category
- model published in study
- attempted reproduction of a model
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
- Andrés Felipe Rodríguez Corcho (0000-0002-1521-7910)
- Sara Polanco (0000-0002-1270-4377)
- Rebecca Farrington (0000-0002-2594-6965)
- Romain Beucher (0000-0003-3891-5444)
- Camilo Montes (0000-0002-3553-0787)
- Louis Moresi (0000-0003-3685-174X)
Scientific Keywords
- arc continent collision
- arc buoyancy
- contrasting style of collision
- lithospheric flow
Funder
- University of Melbourne
Section 2: your model code, output data
Include model code? True
Model code URI/DOI https://zenodo.org/records/5153073
Section 3: software framework and compute details
Software Repository https://github.com/underworldcode/underworld2
Software & algorithm keywords
- Python
- Finite element
Computer URI/DOI https://doi.org/10.25914/608bfd1838db2
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', 'attempted reproduction of a model'], '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': ['arc continent collision', 'arc buoyancy', 'contrasting style of collision', 'lithospheric flow'], 'funder': [{'@type': 'Organization', 'name': 'University of Melbourne'}], 'include_model_code': True, 'model_code_uri': 'https://zenodo.org/records/5153073', 'software': {'@type': 'SoftwareApplication', 'codeRepository': 'https://github.com/underworldcode/underworld2', 'keywords': ['Python', 'Finite element']}, 'computer_uri': 'https://doi.org/10.25914/608bfd1838db2'}
-> 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, attempted reproduction of a model
-> associated publication DOI
https://doi.org/10.1029/2022GC010386
-> title
No response
-> description
No response
-> model authors
No response
-> scientific keywords
arc continent collision, arc buoyancy, contrasting style of collision, lithospheric flow
-> 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
https://doi.org/10.5281/zenodo.5131909
-> software framework source repository
https://github.com/underworldcode/underworld2
-> name of primary software framework (e.g. Underworld, ASPECT, Badlands, OpenFOAM)
No response
-> software framework authors
No response
-> software & algorithm keywords
Python, Finite element
-> computer URI/DOI
https://doi.org/10.25914/608bfd1838db2
-> 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