Numerous model simulations reveal that this circulation is quite sensitive to the freshwater budget in the high - latitude regions where deep waters form.
Not exact matches
Numerous teams in the world are developing
models and
simulations, for example to reproduce the physical processes driving the formation of planets in circumstellar discs, the evolution of their orbits through migration or mutual interaction, or the properties of their atmospheres.
Among the
numerous star - planet interaction (SPI)
models that have been developed, magnetohydrodynamic (MHD)
simulations combine state of the art numerical
models of cool star magnetospheres with simplified
models of planets.
Numerous recent studies based on both observations and
model simulations indicate that reduced Barents - Kara sea ice in late fall favors a strengthened and northwestward expansion of the Siberian high, increased poleward heat flux, weakened polar vortex, and ultimately a negative AO.
The ICON
model, which is jointly developed by the Max Planck Institute for Meteorology (MPI - M) and the German Meteorological service (DWD), will serve as the basis for
numerous future research projects and
simulations.
Though each of these outcomes are indeed projected to occur in some climate
model simulations, there are
numerous reasons to doubt those projections.