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  2. Mantle convection - Wikipedia

    en.wikipedia.org/wiki/Mantle_convection

    Simplified model of mantle convection: [1] Whole-mantle convection. Mantle convection is the very slow creep of Earth's solid silicate mantle as convection currents carry heat from the interior to the planet's surface. [2] [3] Mantle convection causes tectonic plates to move around the Earth's surface. [4] The Earth's lithosphere rides atop the ...

  3. Slab suction - Wikipedia

    en.wikipedia.org/wiki/Slab_suction

    This force occurs between two colliding plates where one is subducting beneath the other. As one plate subducts, it sets up convection currents in the upper mantle that exert a net trenchward pull, and acts to suck both the plates together. [2] Slab suction is weaker than slab pull, which is the strongest of the driving forces.

  4. Earth system interactions across mountain belts - Wikipedia

    en.wikipedia.org/wiki/Earth_system_interactions...

    The asthenosphere is the ductile region of the upper mantle. Mantle processes which operate across mountain belts include those related to subduction (e.g., slab break-off, flat-slab subduction, subduction of a triple junction). Volcanism is driven by mantle processes such as partial melting and thermal convection currents.

  5. Convection - Wikipedia

    en.wikipedia.org/wiki/Convection

    Convection within Earth's mantle is the driving force for plate tectonics. Mantle convection is the result of a thermal gradient: the lower mantle is hotter than the upper mantle, and is therefore less dense. This sets up two primary types of instabilities.

  6. Earth's internal heat budget - Wikipedia

    en.wikipedia.org/wiki/Earth's_internal_heat_budget

    Controversy over the exact nature of mantle convection makes the linked evolution of Earth's heat budget and the dynamics and structure of the mantle difficult to unravel. [21] There is evidence that the processes of plate tectonics were not active in the Earth before 3.2 billion years ago, and that early Earth's internal heat loss could have ...

  7. Convection (heat transfer) - Wikipedia

    en.wikipedia.org/wiki/Convection_(Heat_transfer)

    Forced convection: when a fluid is forced to flow over the surface by an internal source such as fans, by stirring, and pumps, creating an artificially induced convection current. [ 3 ] In many real-life applications (e.g. heat losses at solar central receivers or cooling of photovoltaic panels), natural and forced convection occur at the same ...

  8. Slab pull - Wikipedia

    en.wikipedia.org/wiki/Slab_pull

    L is the slab length calculated only for the part above 670 km (the upper/lower mantle boundary); A is the slab age in Ma at the trench. The slab pull force manifests itself between two extreme forms: The aseismic back-arc extension as in the Izu–Bonin–Mariana Arc. And as the Aleutian and Chile tectonics with strong earthquakes and back-arc ...

  9. Mantle plume - Wikipedia

    en.wikipedia.org/wiki/Mantle_plume

    The current mantle plume theory is that material and energy from Earth's interior are exchanged with the surface crust in two distinct and largely independent convective flows: as previously theorized and widely accepted, the predominant, steady state plate tectonic regime driven by upper mantle convection , mainly the sinking of cold plates of ...