What caused the variations in pressure that created the convectional circulation pattern? Heating caused air contraction, which lowers its density and causes buoyancy -- and the air rises Heating caused air expansion, which increases its density and causes the air to sink Heating caused air expansion, which increases its density and buoyancy -- so the air sinks. Heating caused air expansion, which lowers its density and causes buoyancy -- so the air rises
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The variations in pressure that create the convectional circulation pattern are mainly driven by the uneven heating of the Earth's surface. For instance, areas near the equator receive more direct sunlight, leading to greater heating, causing air to expand, lower in density, and rise. This rising air creates a low-pressure zone at the surface, which is filled by cooler, denser air from the surrounding regions, initiating a cycle of air movement that contributes to weather patterns. In real-world applications, this convection process is critical in meteorology and climate science. It helps explain phenomena like trade winds, monsoons, and even cyclone formation. For instance, the warm, moist air rising in tropical regions contributes to the development of storms, while the sinking cooler air in high-pressure zones can lead to clear skies and stable weather. Understanding these dynamics can help predict weather changes and prepare for natural events.