Code consisting of very «regular» calculations, such as simulating
the atmosphere as a grid of evenly - sized squares, may always work best on vector systems.
Not exact matches
Electric currents that flow into and out of the ionosphere, which AMPERE monitors, have various effects on it
as well
as the
atmosphere in general that can cause problems with tracking LEO space debris, the use of GPS systems, and even terrestrial power plants —
as was the case when a geomagnetic storm took down Quebec's power
grid in 1989, Anderson says, adding, «The operators didn't know what was happening.»
The sun is a tempestuous place prone to proton and electron particle storms that can speed across a 150 - million - kilometer space chasm to bash into Earth's
atmosphere, potentially disrupting satellite service, damaging telecommunications networks, causing power
grid blackouts and endangering high - altitude aircraft
as well
as astronauts on board the International Space Station.
If one divides the earth into 50x50km blocks then I suppose that's about 200k
grid points (times however many layers you want in the
atmosphere) and
as for the oceans I have no idea.
The model -
atmosphere both receives information (about such things
as sea - surface temperature) and produces output (such
as winds, temperatures, and rainfall)
as sets of numbers on a
grid.
So if it is taken
as given that at times
grids in the near future will often have electrical available for times at next to nothing, what's the best way to use it to remove CO2 or other greenhouse gases from the
atmosphere?
The job of the radiation module is to calculate the solar heating rate profiles and the thermal cooling rate profiles, including the energy deposition at the ground surface,
as well
as the energy balance at the top of the
atmosphere for the specified climate variable distribution at each
grid box.
On the other side, Professor Andr e Berger and colleagues developed a mathematical model of the climate system, rated today
as a «model of intermediate complexity» [6, 7] to solve the dynamics of the
atmosphere and ice sheets on a spatial
grid of 19 × 5 elements, with a reasonably extensive treatment of the shortwave and longwave radiative transfers in the
atmosphere.