Abstract
We discuss the equations describing convective motion of a fluid with temperature and pressure dependent rheology. By combining observational constraints from plate tectonics with theoretical constraints deduced from the model equations and parameter values, we are led to the conclusion that shallow upper mantle convection is consistent with the equations of fluid dynamics.
Original language | English |
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Pages (from-to) | 816-819 |
Number of pages | 4 |
Journal | Geophysical Research Letters |
Volume | 9 |
Issue number | 8 |
DOIs | |
Publication status | Published - Aug 1982 |