What causes the amount of sun's heat energy received by the north pole in the equator
The amount of heat energy received by a region is primarily determined by the angle of the sun's rays, which is affected by the region's latitude and the Earth's tilt.
At the equator, the sun's rays are more direct and the angle of incidence is nearly perpendicular, which results in a higher amount of heat energy being received. This is because the Earth's surface at the equator is more directly exposed to the sun, causing it to receive more solar radiation.
In contrast, at the North Pole, the sun's rays are at a lower angle and the energy is spread out over a larger area. This results in less heat energy being received at the poles compared to the equator. Additionally, the polar regions receive less sunlight overall due to the Earth's axial tilt, which causes the poles to experience longer periods of darkness during winter months.
Overall, the differences in the amount of heat energy received by the North Pole and the equator are a result of the Earth's tilt and the angle at which the sun's rays hit the Earth's surface at different latitudes.