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Solar energy is the process by which electromagnetic radiation generated by thermonuclear fusion reactions in the Sun reaches Earth and is converted into heat and electrical energy. The Sun produces approximately 3.86×10²⁶ watts of power per second, of which about 1.74×10¹⁷ watts reaches Earth’s atmosphere. This amount corresponds to roughly 15,000 times the world’s annual energy demand. Solar radiation spans a broad electromagnetic spectrum including visible, ultraviolet (UV), and infrared (IR)

Sun energy is the process by which electromagnetic radiation generated by thermonuclear fusion reactions in the Sun reaches Earth and is converted into heat and electrical energy. The Sun produces approximately 3.86×10²⁶ watts of power per second, of which about 1.74×10¹⁷ watts reach Earth’s atmosphere. This amount corresponds to roughly 15,000 times the world’s annual energy demand. Solar radiation spans a broad electromagnetic spectrum including visible, ultraviolet (UV), and infrared (IR) reg