dc.contributor
Stein, Claudia
dc.creator
Stein, Claudia
dc.creator
Hansen, Ulrich
dc.date.accessioned
2024-05-07T14:53:02Z
dc.date.available
2024-05-07T14:53:02Z
dc.identifier
https://doi.org/10.35003/MQIYGR
dc.identifier.uri
https://refubium.fu-berlin.de/handle/fub188/43492
dc.identifier.uri
http://dx.doi.org/10.17169/refubium-43209
dc.description
Various structures observed in Earth’s mantle are considered to have a high density and therefore affect the mantle flow and the plate motion. We analyze the onset time
of surface motion for 2D basally heated models with and without dense material. We
find that the first motion is delayed for more, deeper or denser chemical heterogeneities.</br>
Due to a temperature-dependent viscosity, the temperature difference between the cold
surface and a hot mantle leads to a highly viscous surface region. In contrast, in a cold
mantle, the temperature difference is too small to form rigid plates. The heat from the
core first needs to be transported upwards by plumes. Therefore, it takes longer for highly viscous plates to form.</br>
In the period after the Earth’s mantle was (partially) molten, the mantle was hotter than
today. Under these conditions, plate motion can occur within approximately the first 0.5
Gyr if no chemical structures are present or if they are initially located at the surface.
For a system that additionally has deep chemical heterogeneities, the onset of plate motion will be delayed by at least one order of magnitude. The motion will have been less stable than today, probably showing short subduction events.
dc.subject
Earth and Environmental Sciences
dc.subject
mantle convection
dc.subject
onset plate motion
dc.subject
numerical study
dc.title
Replication Data for: Onset of plate motion in the presence of chemical heterogeneities in the mantle and the effect of mantle temperature
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