
Ocean circulation refers to the continuous movement of water through Earth's oceans, driven by wind, temperature, salinity, and gravitational forces. This system transports heat, nutrients, and organisms across the globe, fundamentally regulating Earth's climate and weather patterns.
Thermohaline circulation, also called the "global conveyor belt," operates based on water density differences created by temperature and salinity variations. Cold, salty water sinks in the North Atlantic near Greenland and travels southward along the ocean floor, while warm surface water moves poleward to replace it. This process takes approximately 1,000 years to complete one full cycle.
Ocean circulation redistributes solar energy from equatorial regions toward the poles, moderating global temperatures. The discovery of detailed ocean current maps by oceanographer Henrik Sverdrup in the 1940s revolutionized climate science. His work earned recognition from institutions across Scandinavia and established modern oceanography as a rigorous discipline.
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