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Tag: Subduction initiation

Subduction initiation is explained in this collection of accurate, accessible science graphics, designed to make understanding this key geological process clear and engaging. These visuals explore how and where subduction zones first form, triggering the descent of one tectonic plate beneath another and setting the stage for earthquakes, volcanic arcs, and mountain building. Perfect for educators, students, and geology enthusiasts, this subduction initiation graphic collection turns complex geodynamic concepts into visually rich, easy-to-grasp resources for teaching and learning.

Subduction initiation forcing

The illustration depicts two endmember states in subduction zone initiation: vertically-forced and horizontally-forced subduction initiation.

Illustration of the two endmember states forcing a new subduction zone. The two endmember forcing states characterising subduction zone initiation (SZI) can be described as either vertically-forced or horizontally-forced. As outlined in Crameri et al. (2020), the dominant forcing is either—but never exclusively—vertical (i.e., some combination of plate buoyancy force, the force from any surface load, and vertical mantle-flow force), or horizontal (i.e., some combination of tectonic force and horizontal mantle-flow force).

  • Creator: Fabio Crameri
  • This version: 24.10.2021
  • License: Attribution-ShareAlike 4.0 International (CC BY-SA 4.0)
  • Specific citation: This graphic by Fabio Crameri from Crameri et al. (2020) is available via the open-access s-Ink repository.
  • Related reference: Crameri, F., V. Magni, M. Domeier, G.E. Shephard, K. Chotalia, G. Cooper, C. Eakin, A.G. Grima, D. Gürer, A. Király, E. Mulyukova, K. Peters, B. Robert, and M. Thielmann (2020), A transdisciplinary and community-driven database to unravel subduction zone initiation, Nature Communications, 11, 3750. doi:10.1038/s41467-020-17522-9
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Plume-induced subduction

Temporal evolution of subduction initiation in a global, 3-D spherical numerical experiment showing the cold plates and hot mantle plumes.

Temporal evolution of subduction initiation in a global, 3-D spherical numerical experiment showing the cold plates as viscosity isosurfaces (grey) and mantle plumes as a temperature isosurface (red). Individual snapshots highlight the different phases of plume-induced subduction initiation characterised by (a) onset of hot mantle plumes, (b) local lithospheric thinning, (c-d) development of strong lithosphere-asthenosphere boundary topography through shallow horizontal mantle flow and an additional plume pulse, (e-f) plate failure and, finally, (g-h) buoyancy-driven subduction.

  • Creator: Fabio Crameri
  • This version: 01.09.2021
  • License: Attribution-ShareAlike 4.0 International (CC BY-SA 4.0)
  • Specific citation: This graphic by Fabio Crameri from Crameri and Tackley (2016) is available via the open-access s-Ink repository.
  • Related reference: Crameri, F., and P. J. Tackley (2016), Subduction initiation from a stagnant lid and global overturn: new insights from numerical models with a free surface, Progress in Earth and Planetary Science, 3(1), 1–19, doi:10.1186/s40645-016-0103-8
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SZI geologic evidence

Schematic illustration of the emplacement of subduction zone initiation (SZI)-typical rock evidence during SZI, and a typical SZI ophiolite sequence.

Schematic illustration of the emplacement of subduction zone initiation (SZI)-typical rock evidence during SZI, and a typical SZI ophiolite sequence. Note that this is a text-book example (according to e.g., the Izu-Bonin-Mariana SZI) and that pre-existing structures (e.g., a pre-existing volcanic arc) or variable SZI dynamics (e.g., horizontal compression) could inhibit various stages and therefore their typical rock signatures.

  • Creator: Fabio Crameri
  • This version: 18.08.2021
  • License: Attribution-ShareAlike 4.0 International (CC BY-SA 4.0)
  • Specific citation: This graphic by Fabio Crameri from Crameri et al. (2020) is available via the open-access s-Ink repository.
  • Related reference: Crameri, F., V. Magni, M. Domeier, G.E. Shephard, K. Chotalia, G. Cooper, C. Eakin, A.G. Grima, D. Gürer, A. Király, E. Mulyukova, K. Peters, B. Robert, and M. Thielmann (2020), A transdisciplinary and community-driven database to unravel subduction zone initiation, Nature Communications, 11, 3750. doi:10.1038/s41467-020-17522-9
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Mobile-lid mantle convection

Temporal evolution of a global, fully spherical, 3D model of whole-mantle convection.

Animation showing the temporal evolution of whole-mantle convection including plate tectonics. The convective turnover of the mantle is characterised by hot rising mantle plumes (indicated by a hot, red temperature isosurface), and cold and stiff subduction zones of heavy tectonic surface plates (indicated by grey viscosity isosurfaces). Like on the Earth, in this model the mantle convects including its surface thermal boundary layer, with subduction zones (i.e., the sinking of cold and heavy oceanic plates) being its main driver. The global, fully spherical, 3D mantle convection model has been run by the code StagYY and represents the actual dynamics in the Earth’s mantle under some assumptions and simplifications.

  • Creator: Fabio Crameri
  • This version: 07.08.2021
  • License: Attribution-ShareAlike 4.0 International (CC BY-SA 4.0)
  • Specific citation: This graphic by Fabio Crameri from Crameri and Tackley (2016) is available via the open-access s-ink.org repository.
  • Related reference: Crameri, F., and P. J. Tackley (2016), Subduction initiation from a stagnant lid and global overturn: new insights from numerical models with a free surface, Progress in Earth and Planetary Science, 3(1), 1–19, doi:10.1186/s40645-016-0103-8
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