Convective motion refers to the movement of fluids (liquids and gases) as a result of variations in temperature and density. This type of motion occurs in the Earth's atmosphere, oceans, and even in the mantle beneath the Earth's crust. The driving force behind convective motion is the transfer of heat, which causes the fluid to expand and become less dense, leading to upward movement. As the fluid moves to regions of lower temperature, it cools and becomes denser, causing it to sink back down. This circulation pattern creates a continuous cycle of motion.
To better understand convective motion, consider the following study topics:
By delving into these topics, you can gain a comprehensive understanding of convective motion and its significance in various natural systems.
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