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Figure 2: Electromagnetic wave fields and propagation | Figure 3: A wave characterized by frequency and wavelength |
c = f*λ
, where c is light speed.The discovery and understanding of electromagnetic waves have a rich history. In the late 19th century, James Clerk Maxwell's equations provided the theoretical foundation these waves. It was Heinrich Hertz who first demonstrated the existence of elctromagnetic waves in the laboratory in the 1880s. Hertz's experiments showed that electric sparks could produce and detect elctromagnetic waves, marking a significant breakthrough.
However, it was Guglielmo Marconi who made practical use of elctromagnetic waves for wireless communication in the early 20th century. His work led to the development of the first radio transmitters and receivers, paving the way for modern wireless communication systems.
Since the Big Bang elctromagnetic waves have been produced by various natural sources. One of the most prominent natural sources of electromagnetic waves is celestial objects, including stars, planets, and galaxies. Many kinds of telescopes are specialized instruments designed to observe these cosmic emissions, allowing scientists to study the universe's hidden secrets. Earth's atmosphere also emits electromagnetic waves through processes like lightning strikes, which generate lights and radio signals known as sferics (sometimes also spelled "spheric"). These natural electromagnetic emissions can be harnessed for meteorological and atmospheric studies.