Welcome! This is a template repository for submitting models to Model Atlas of The Earth (M@TE).
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- fork this template and rename using this convention:
creatorname_year_keyword(e.g.corcho_2022_collision)
- populate this markdown document (
Readme.md) with as much information as you can- information is recorded in Markdown Tables (Metadata fields) and additional Metadata Tags.
- submit a pull request to merge this model into the ModelAtlasofTheEarth
Note The Wiki provides more detailed information on submission. Create a Github Issue if you have problems or questions.
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Metadata fields
| Field | Value | Notes |
|---|---|---|
| Title | The Role of Lithospheric-Deep Mantle Interactions on the Style and Stress Evolution of Arc-Continent Collision | ... |
| Abstract | Continents grow by the successive accretion of material to their margins, mostly collision and accretion of intra-oceanic magmatic arcs. We investigate the effect of arc buoyancy and viscosity on the mode of collision, and the effects on the margin using a computer modeling approach. Our simulations show that upon collision, it is a small differential in density (3%) between the colliding arc and the continental margin that dictates whether subduction continues or stops after collision. In addition, our models show that arc buoyancy and viscosity drive lithospheric extension in the continental plate. Also, as the subducting slab reaches a mantle discontinuity at 660 km depth, it folds and causes strain and stress fluctuations on the margin. | |
| Keywords | Collision, subduction, accretion | |
| Field of research (FOR) code | 3706,370604 |
Metadata Tags
Note Place an X in in the boxes to select!
- published study
- commmunity benchmark
- reproduction of published model
- missing data model (needs rebuilding by community)
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Metadata fields
The following fields provide information and references for sources and processes that were used to create the dataset and an audit trail for modifications to the original data. Provide web references, DOIs, Github links, etc. on any of the components that went into the generation of the dataset. Please provide versioning wherever possible or relevant. Examples may include: software packages, programs of work, input datasets.
| Field | Value | Notes |
|---|---|---|
| software framework | UWGeodynamics | |
| software version | ||
| source code link | https://github.com/underworldcode/UWGeodynamics | |
| input datasets | None | |
| computer details | E.g., cluster name, Operating System, MPI version, number of cores | |
| additional notes | E.g., This product was generated by XX method as described by XX et al. (yyyy) . Further details and code for the method are available in the Github/code repository XX....This product is derived from dataset XX (dataset doi or link to details). The method is detailed in .... and uses inputs X (link), Y (link), Z (link) to produce this published product. |
Note Please add any addition files relate to computation and reproduction to the
model_reproduction_filesfolder, and describe these in the table below.
Metadata Tags
- this submission includes input files
- this submission includes postprocessing files
- this submission includes a software container (i.e. docker image or dockerfile)
- postprocessing files are linked to M@TE Server (NCI GeoNetwork) through thredds/OpenDap
Model reproduction files
| Filename/pattern | Description | Notes |
|---|---|---|
SubductionTransference_Mechanical_25Km-WeakerLM.ipynb |
Jupyter notebook to run model with 25 km thick arc-crust | Additional info |
ModelGeometry.py |
python script with functions/variables requied by SubductionTransference_Mechanical_25Km-WeakerLM.ipynb |
|
MechanicalProperties.py |
python script with functions/variables requied by `SubductionTransference_Mechanical_25Km-WeakerLM.ipynb | |
Figure_6_Kinematics_Analysis.ipynb |
Jupyter notebook containing workflow to recreate Fig. 6 of Corcho. et al 2022 |
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Metadata Tags
- this submission includes model output data
Note If the above box is ticked, the M@TE team will contact you with details for uploading data to the NCI M@TE Server Please fill out the metadata fields below.
Metadata fields
| Field | Value | Notes |
|---|---|---|
| Dataset format | xmf, xdmf, hdf5 | |
| Temporal extents (if applicable) | --- | |
| Spatial extents (if applicable) | --- | |
| Local NCI file path | Completed once data are available on NCI Geonetwork Catalog | |
| DOI (NCI Internal Field) | Completed once data are available on NCI Geonetwork Catalog | |
| additional notes | E.g., output data ar saved at time/step increments of (100 Kyr) |
Note The following table provides can be used to descibe the output data files associated with this model The more information you record, the better!
Output data files
| Filename/pattern | Description | Notes |
|---|---|---|
| XDMF.fields.00100.xmf | ||
| XDMF.swarms.00100.xmf | ||
| pressureField-100.h5 | ||
| projDensityField-100.h5 | ||
| projMaterialField-100.h5 | ||
| projMeltField-100.h5 | ||
| projPlasticStrain-100.h5 | ||
| projStressField-100.h5 | ||
| projStressTensor-100.h5 | ||
| projTimeField-100.h5 | ||
| projViscosityField-100.h5 | ||
| strainRateField-100.h5 | ||
| test_timestep_100 | ||
| velocityField-100.h5 | ||
| ArcTracers-100.h5 | ||
| ArcTracers-100.xdmf | ||
| ArcTracers_Arc nodes velocity_X-100.h5 | ||
| ArcTracers_Arc nodes velocity_Y-100.h5 | ||
| ArcTracers_Arc stress tensor_X-100.h5 | ||
| ArcTracers_Arc stress tensor_XY-100.h5 | ||
| ArcTracers_Arc stress tensor_Y-100.h5 | ||
| ArcTracers_Time_Arc-100.h5 | ||
| ArcTracers_arc overriding plate strain rate-100.h5 | ||
| ArcTracers_arc overriding plate stress Field-100.h5 | ||
| ArcTracers_global_index-100.h5 | ||
| CratonTracers-100.h5 | ||
| CratonTracers-100.xdmf | ||
| CratonTracers_Craton stress tensor_X-100.h5 | ||
| CratonTracers_Craton stress tensor_XY-100.h5 | ||
| CratonTracers_Craton stress tensor_Y-100.h5 | ||
| CratonTracers_Cratonic overriding plate velocity _X-100.h5 | ||
| CratonTracers_Cratonic overriding plate velocity_Y-100.h5 | ||
| CratonTracers_Time_SP-100.h5 | ||
| CratonTracers_global_index-100.h5 | ||
| OPTracers-100.h5 | ||
| OPTracers-100.xdmf | ||
| OPTracers_Time_OP-100.h5 | ||
| OPTracers_Weak overriding plate strain rate-100.h5 | ||
| OPTracers_Weak overriding plate stress Field-100.h5 | ||
| OPTracers_Weak overriding plate stress tensor_X-100.h5 | ||
| OPTracers_Weak overriding plate stress tensor_XY-100.h5 | ||
| OPTracers_Weak overriding plate stress tensor_Y-100.h5 | ||
| OPTracers_Weak overriding plate velocity_X-100.h5 | ||
| OPTracers_Weak overriding plate velocity_Y-100.h5 | ||
| OPTracers_global_index-100.h5 | ||
| SPTracers-100.h5 | ||
| SPTracers-100.xdmf | ||
| SPTracers_Subducting plate velocity_X-100.h5 | ||
| SPTracers_Subducting plate velocity_Y-100.h5 | ||
| SPTracers_Time_SP-100.h5 | ||
| SPTracers_global_index-100.h5 |
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Note To feature your model on our website (https://mate.science), we will require some images/animations and captions. Please add
web_filesfolder, and describe these files using the following table. The `Purpose' field will be used to direct the content. You do not need to supply all of these, and you may supply multiple files with same purpose, in which case we can scroll images.
| File | Purpose | Caption |
|---|---|---|
graphic_abstract.png |
visual abstract | Schematic illustration of initial model conditions and subsequent post-collisional evolution of the two identified styles of arc-continent collision, whose dynamics are controlled by arc transference and slab-anchoring in less buoyant remnant arcs (see publication for further detail) |
model_setup.jpg |
model setup | (a) Model set up for numerical simulations based on previous research in the dynamics of accretionary continental margins (Moresi et al., 2014). It includes an oceanic subducting plate (dark yellow), an overriding plate composed by a continental (cyan) and cratonic domain (dark blue), and a ribbon of thicker crust representing a remnant = intra-oceanic arc attached to the oceanic plate (red). The upper mantle and the upper-lower mantle boundary are included to capture deep-mantle slab interactions. Orange, yellow, and dark green dots show locations where subducting plate convergence velocity, the trench-retreat velocity and the overriding plate (OP) retreat velocity were measured. The (b–e) profiles show a schematic lithospheric cross-section of the domains considered in our model set-up (see publication for further detail). |
animation_25.gif |
animation | Evolution of material field for model with 25 km arc crust |
animation_35.gif |
animation | Evolution of material field for model with 35 km arc crust |
Note Acceptible formats: JPEG, PNG, PDF, AVI, GIF, MP4 Total size of files will be limited by Github repository constraints
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| Field | Value | Notes |
|---|---|---|
| Associated publication DOI | DOI | |
| Funder(s) | Australian Research Council's ITRH Project IH130200012 and DP150102887. AFRC was supported by a scholarship from the Colombian Government (Ministerio de Ciencia, Tecnología, e Innovación, 783), a research grant from the Colombian Association of Petroleum Geologists and Geophysicists (Asociación Colombiana de Geólogos y Geofísicos del Petróleo) fund and a top-up scholarship form the University of Melbourne (Baragwanath scholarship). This work was enabled by Auscope, the Nectar Research Cloud and the National Computational Infrastructure (projects m18, mw52), which are supported by the Australian Government via the National Collaborative Research Infrastructure Strategy (NCRIS). | |
| Author(s) | Refer to publication | |
| Licence | E.g.,  This work is licensed under a Creative Commons Attribution 4.0 International License. |
Note on Publications Please also add .bib entries for any associated publication to the
CITATIONS.bibfile See Wiki for further information on .bib files
Note on Licence we encourage model creators to issue a single licence that will cover all material sumbitted to M@TE. we recommend a Creative Commons license you can use the following website to choose from a range of options Chttps://creativecommons.org/choose/