Electromagnetic radiation: Difference between revisions

From Citizendium
Jump to navigation Jump to search
imported>Paul Wormer
No edit summary
mNo edit summary
 
(4 intermediate revisions by 2 users not shown)
Line 1: Line 1:
{{subpages}}
{{subpages}}
'''Electromagnetic radiation''' is a collective name for  a set of [[electromagnetic wave]]s. The collection of electromagnetic waves of different [[wavelength]]s constitutes the [[electromagnetic spectrum]]. The part of the electromagnetic spectrum that we can see with our bare eyes is called [[visible light]], or briefly light.
'''Electromagnetic radiation''' (EM) is a collective name for  a set of [[electromagnetic wave]]s. The collection of electromagnetic waves of different [[wavelength]]s constitutes the [[electromagnetic spectrum]]. The part of the electromagnetic spectrum that we can see with our bare eyes is called [[visible light]], or briefly light. The electromagnetic spectrum covers an incredibly large range of wavelengths, from  10<sup>3</sup>  to  10<sup>&minus;12</sup> [[meter]], see the adjacent figure.
{{Image|Electromagnetic-Spectrum.png|right|350px|Fig. 1: Overview of the [[electromagnetic spectrum]]. }}


Since [[Albert Einstein]]'s work of 1905,  electromagnetic radiation is seen as a flux of [[photon]]s (also known as light quanta) through space. This view is reminiscent of [[Isaac Newton]]'s view, who saw light as a stream of corpuscles. This view was rejected in the early 19th century by [[Thomas Young]] and [[Augustin-Jean Fresnel]], who considered light as waves&mdash;later in the 19th century  seen as oscillations of the [[ether (physics)|ether]]. An electromagnetic wave being characterized by its [[frequency]] &nu;, Einstein postulated photons to be packets of energy ''h''&nu;. These massless elementary particles move with the universal [[speed of light]] ''c''. The symbol ''h'' is [[Planck’s constant]]. Photons of the same energy ''h''&nu; are indistinguishable, they are [[boson]]s. The number density of photons corresponds to the intensity of the electromagnetic (EM) radiation.  
Since [[Albert Einstein]]'s work of 1905,  electromagnetic radiation is seen as a flux of [[photon]]s (also known as light quanta) through space. This view is reminiscent of [[Isaac Newton]]'s view, who saw light as a stream of corpuscles. This view was rejected in the early 19th century by [[Thomas Young]] and [[Augustin-Jean Fresnel]], who considered light as waves. Later in the 19th century  these waves were seen as oscillations of the [[ether (physics)|ether]] by physicists  as [[James Clerk Maxwell]], [[Heinrich Rudolf Hertz]], and [[Hendrik Antoon Lorentz]]. In 1861 Maxwell had the great theoretical insight that (visible) light is  nothing but electromagnetic radiation of certain wavelengths; he predicted that (non-visible) electromagnetic waves of other  wavelengths must exist too. This was confirmed experimentally by Hertz in the years 1886–1888.


On Earth the most important source of EM radiation is the the Sun, and it is no coincidence that the maximum sensitivity of the eyes of most animals and humans is exactly at the most abundant part of the electromagnetic energy radiated by the Sun. This is the part of the EM spectrum that is the visible light. All life on Earth depends on the energy received from the Sun and by photosynthesis this energy is converted into plant life and atmospheric oxygen. The fossil fuels that modern society uses&mdash;gas, oil, and coal&mdash;are stored sources of energy received  in the past from the Sun in the form of electromagnetic radiation.
An electromagnetic wave being characterized by its [[frequency]] &nu;, Einstein postulated light quanta  to be packets of [[Energy (science)|energy]] ''h''&nu;. These massless elementary particles move with the universal [[speed of light]] ''c''. The symbol ''h'' is [[Planck's_constant|Planck's constant]]. Photons of the same energy ''h''&nu; are indistinguishable, they are [[boson]]s. The number density of photons corresponds to the intensity of the electromagnetic radiation.
 
Electromagnetic waves play an important role as carriers of information in the form of [[radio]], [[television]], [[cell phone]], etc. signals.
 
On [[Earth]] the most important source of energy is the the [[Sun]], that transmits its energy in the form of electromagnetic radiation. It is no coincidence that the maximum sensitivity of the eyes of most animals and humans is exactly at the most abundant part of the electromagnetic energy radiated by the Sun and not filtered by the [[Earth's atmosphere]]. This is the part of the EM spectrum that is the visible light. All life on Earth depends on the energy received from the Sun and by [[photosynthesis]] this energy is converted into plant life and atmospheric oxygen. The [[fossil fuel]]s that modern society uses&mdash;[[Natural gas|gas]], [[Petroleum crude oil|oil]], and [[coal]]&mdash;are stored sources of energy received  in the past millions of years from the Sun.[[Category:Suggestion Bot Tag]]

Latest revision as of 06:01, 11 August 2024

This article is a stub and thus not approved.
Main Article
Discussion
Related Articles  [?]
Bibliography  [?]
External Links  [?]
Citable Version  [?]
 
This editable Main Article is under development and subject to a disclaimer.

Electromagnetic radiation (EM) is a collective name for a set of electromagnetic waves. The collection of electromagnetic waves of different wavelengths constitutes the electromagnetic spectrum. The part of the electromagnetic spectrum that we can see with our bare eyes is called visible light, or briefly light. The electromagnetic spectrum covers an incredibly large range of wavelengths, from 103 to 10−12 meter, see the adjacent figure.

© Image: Louis Keiner
Fig. 1: Overview of the electromagnetic spectrum.

Since Albert Einstein's work of 1905, electromagnetic radiation is seen as a flux of photons (also known as light quanta) through space. This view is reminiscent of Isaac Newton's view, who saw light as a stream of corpuscles. This view was rejected in the early 19th century by Thomas Young and Augustin-Jean Fresnel, who considered light as waves. Later in the 19th century these waves were seen as oscillations of the ether by physicists as James Clerk Maxwell, Heinrich Rudolf Hertz, and Hendrik Antoon Lorentz. In 1861 Maxwell had the great theoretical insight that (visible) light is nothing but electromagnetic radiation of certain wavelengths; he predicted that (non-visible) electromagnetic waves of other wavelengths must exist too. This was confirmed experimentally by Hertz in the years 1886–1888.

An electromagnetic wave being characterized by its frequency ν, Einstein postulated light quanta to be packets of energy hν. These massless elementary particles move with the universal speed of light c. The symbol h is Planck's constant. Photons of the same energy hν are indistinguishable, they are bosons. The number density of photons corresponds to the intensity of the electromagnetic radiation.

Electromagnetic waves play an important role as carriers of information in the form of radio, television, cell phone, etc. signals.

On Earth the most important source of energy is the the Sun, that transmits its energy in the form of electromagnetic radiation. It is no coincidence that the maximum sensitivity of the eyes of most animals and humans is exactly at the most abundant part of the electromagnetic energy radiated by the Sun and not filtered by the Earth's atmosphere. This is the part of the EM spectrum that is the visible light. All life on Earth depends on the energy received from the Sun and by photosynthesis this energy is converted into plant life and atmospheric oxygen. The fossil fuels that modern society uses—gas, oil, and coal—are stored sources of energy received in the past millions of years from the Sun.