Which explains the difference in the distibution of solar energy on earth's surface?
The distribution of solar energy on Earth's surface is primarily influenced by factors such as the angle of the sun's rays, the length of daylight hours, and the amount of atmospheric interference. The angle of the sun's rays varies depending on the latitude of a particular location, with areas closer to the equator receiving more direct sunlight than areas closer to the poles. This results in higher solar energy levels near the equator and lower levels towards the poles.
Additionally, the length of daylight hours also plays a role in the distribution of solar energy. Areas that experience longer hours of sunlight throughout the year, such as those near the poles during summer months, will receive more solar energy than areas with shorter daylight hours.
Atmospheric interference, such as clouds, dust, and pollution, can also affect the distribution of solar energy. These factors can absorb, reflect, or scatter sunlight, reducing the amount of solar energy that reaches the Earth's surface.
Overall, the combination of these factors results in a variation in the distribution of solar energy on Earth's surface, with equatorial regions typically receiving more solar energy than polar regions.