The Source of Energy for Atmospheric Processes and Its Distribution
The source of energy for all atmospheric processes is the sun. The sun emits a large amount of electromagnetic radiation, which is absorbed by the Earth’s atmosphere and surface. This energy is then distributed around the planet through various processes, such as convection, radiation, and advection (National Aeronautics and Space Administration (NASA)). Convection is the transfer of energy from the Earth’s surface to the atmosphere. This energy is then transferred to other areas through radiation, which is the transfer of energy in the form of light and heat. Finally, advection is the transfer of energy through the transfer of air masses. All of these processes work together to move energy around the planet and make the atmosphere a dynamic system. According to the National Aeronautics and Space Administration (NASA), the Earth’s atmosphere receives around 342 watts per square meter of energy from the sun. This energy is then distributed around the planet through convection, radiation, and advection. These processes act together to create the weather patterns that we experience every day. For example, convection is responsible for the formation of high and low-pressure systems, while radiation is… Cont…
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