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What Would Be The Effect Of The Uneven Distribution Of The Sun’S Energy On Earth?

What Would Be The Effect Of The Uneven Distribution Of The Sun’s Energy On Earth?. Varying atmospheric temperatures set air in motion, causing weather to occur. The equator and the poles would both be cool.

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The amount of solar energy that reaches the earth’s surface depends on different factors, the most important of which is the magnitude of. In the right circumstances, an extreme low can form over the atlantic ocean, with. The equator and the poles would both.

In The Right Circumstances, An Extreme Low Can Form Over The Atlantic Ocean, With.


The uneven heating drives all of the weather on earth. Weather typically occurs in the. Solar radiation is absorbed and then put to use to increase the surface temperature, to change the phase of water, and to fuel atmospheric chemistry.

The Effect Of Uneven Heating Of The Earth Is That It Creates Differences In Temperature Throughout The Planet.


The water vapor in the air then starts to condense, clouds form, and rain and snow are results. What are the three factors that determine the unequal distribution of sun energy on earth? The answer is due to uneven heating of the earth by the sun.

What Would Be The Effect Of The Uneven Distribution Of The Sun’s Energy On Earth?


This can cause different parts of the planet to have different temperatures, which. If there's uneven distribution of the sun’s energy on earth then c. The uneven distribution of insolation intro to physical geography chapter 2.

The Earth's Rotation Causes The Deflection Of Both Wind And.


When the earth is the farthest distance. When the earth orbits the sun, the center of the earth gets more direct sunlight than the poles. The equator and the poles would both.

What Would Be The Effect Of The Uneven Distribution Of The Sun’s Energy?


The earth is rotating, and that rotation also causes rotation of the winds on the surface, called the coriolis effect. The equator and the poles would both be cool. There are several things that can happen to [the sun's] energy as it reaches our planet.

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