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Solar Radiation and Infrared Emission: Earth’s Energy Balance Explained #3043103 (License: Personal Use)
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The image depicts Earth’s radiative energy budget, with yellow wavy lines representing incoming solar radiation (342 W/m² at top of atmosphere), of which 240 W/m² is absorbed by the surface and atmosphere. Red wavy lines illustrate outgoing infrared radiation (102 W/m² shown escaping to space), highlighting the greenhouse effect where some IR is trapped and re-radiated downward.
Used in educational science content, climate change explainers, and environmental physics courses to teach planetary energy balance and the greenhouse effect; matches user intent for understanding Earth’s heat retention mechanisms.
Related Cliparts: Visual explanation of how incoming solar radiation (342 W/m²) interacts with Earth’s atmosphere and surface, and how 102 W/m² is re-emitted as infrared radiation.
(view all Solar Radiation and Infrared Emission: Earth’s Energy Balance Explained)
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