Research news on heat flow (earth)

Heat flow (Earth) refers to the conductive and convective transfer of thermal energy from Earth’s interior to its surface, quantified as heat flux (typically in mW/m²). It arises from the decay of radiogenic isotopes (primarily U, Th, K) in the crust and mantle, residual primordial heat from accretion and core formation, and secular cooling of the core. Measured using borehole temperature gradients and thermal conductivity of rocks, terrestrial heat flow constrains models of lithospheric thickness, mantle convection, plate tectonics, and the global energy budget, and is spatially heterogeneous, with elevated values at mid-ocean ridges and volcanic regions and lower values in stable cratons.

Subway systems are uncomfortably hot—and worsening, study finds

For millions of commuters, the workday doesn't just begin with a train ride. It also begins with a blast of heat. In one of the largest studies ever conducted on thermal comfort in metro systems, Northwestern University scientists ...

AI sheds light on hard-to-study ocean currents

The Indonesian Throughflow carries both warm water and fresh water from the Pacific into the Indian Ocean. As the only low-latitude current that connects the two bodies of water, it plays a key role in ocean circulation and ...

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