Recent numerical simulations suggest the coupling between the stratospheric and tropospheric circulations has practical applications for weather forecasting and also implications for tropospheric climate change (see text on Climate Change, below).
The models include a new wind braking law based on
recent numerical simulations of magnetized stellar winds and specific dynamo and mass - loss prescriptions are adopted to tie angular momentum loss to angular velocity.
The models include a new wind braking law based on
recent numerical simulations of magnetized stellar winds and specific dynamo and mass - loss prescriptions a... ▽ More We present new models for the rotational evolution of solar - like stars between 1 Myr and 10 Gyr with the aim to reproduce the distributions of rotational periods observed for star forming regions and young open clusters within this age range.
In particular, Xi points to
recent numerical simulations at Newcastle University where another superfluid, liquid helium, formed waves of turbulence as it flowed over the rough surface of a wire.
Not exact matches
But
recent observations and
numerical simulations suggest that eventually — in a few millennia, maybe — the solar system may plow into a cloud of gas and dust a thousand times denser than the space we travel through now.
Studies such as Otto et al. (2012) display how the
numerical scale of the
simulation numbers allows for clear separation between a climate with lower level of heat - trapping gases (1960s) and the
recent period (2000s), such that the 2010 heat wave in western Russia was more likely to occur with the additional warming due to climate change (Figure 3).
Studies such as Otto et al. (2012) display how the
numerical scale of the
simulation numbers allows for clear separation between a climate with lower level of heat - trapping gases (1960s) and the
recent period (2000s), such that the 2010 heat wave in western Russia was more likely to occur with the additional warming due to climate change (Figure 3).