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Что (кто) такое émission de radio - определение
CLOUD OF IONIZED GAS EMITTING LIGHT OF VARIOUS COLORS
Emission nebulas; Emission nebulae
Musée de Radio France
MUSEUM IN FRANCE
Musee de Radio France
The Musée de Radio France was a museum operated by Radio France and located in the Maison de Radio-France, near the Pont de Grenelle in the XVIe arrondissement at 116, avenue du Président Kennedy, Paris, France. The museum was established in 1966, and contained a remarkable collection of radios and televisions from their origins to the present day, including the 1793 telegraph by Claude Chappe and early crystal radios.
Solar radio emission
![[[Murchison Widefield Array]] images of background radiation at 240 MHz (grayscale) with color contours showing Type III bursts at a range of frequencies. The bursts are hundreds of times brighter than the background, and the lower-frequency contours appear at greater heights because the bursts are produced by an electron beam that travels away from the Sun, exciting radio emission of decreasing frequency with increasing distance.](https://commons.wikimedia.org/wiki/Special:FilePath/Images of Type III Solar Radio Bursts.png?width=200 "[[Murchison Widefield Array]] images of background radiation at 240 MHz (grayscale) with color contours showing Type III bursts at a range of frequencies. The bursts are hundreds of times brighter than the background, and the lower-frequency contours appear at greater heights because the bursts are produced by an electron beam that travels away from the Sun, exciting radio emission of decreasing frequency with increasing distance.")
![Low Frequency Array]].](https://commons.wikimedia.org/wiki/Special:FilePath/Low-Frequency Solar Radio Telescopes.jpg?width=200 "Low Frequency Array]].")
![Flowchart outlining the stages of plasma emission, which is responsible for most types of solar radio bursts. In the solar context, the electron beam is accelerated either by [[magnetic reconnection]] or a [[shock wave]]. Adapted from chart by [[Donald Melrose]]<ref name=":5" />](https://commons.wikimedia.org/wiki/Special:FilePath/Plasma Emission Flowchart.svg?width=200 "Flowchart outlining the stages of plasma emission, which is responsible for most types of solar radio bursts. In the solar context, the electron beam is accelerated either by [[magnetic reconnection]] or a [[shock wave]]. Adapted from chart by [[Donald Melrose]]<ref name=\":5\" />")
![Low-Frequency Array]] (LOFAR). The solid circles in the images on the right correspond to the size of the Sun seen in visible light.](https://commons.wikimedia.org/wiki/Special:FilePath/QuietSun RadioImaging.jpg?width=200 "Low-Frequency Array]] (LOFAR). The solid circles in the images on the right correspond to the size of the Sun seen in visible light.")
![radio frequency interference]] from human-generated sources.](https://commons.wikimedia.org/wiki/Special:FilePath/Solar Radio Bursts Types I, II, and III.jpg?width=200 "radio frequency interference]] from human-generated sources.")
RADIO WAVES PRODUCED BY THE SUN
Draft:Solar radio emission; Solar radio burst
Solar radio emission refers to radio waves that are naturally produced by the Sun, primarily from the lower and upper layers of the atmosphere called the chromosphere and corona, respectively. The Sun produces radio emissions through four known mechanisms, each of which operates primarily by converting the energy of moving electrons into radiation.
Ràdio Ciutat de Badalona
MUNICIPAL PUBLIC RADIO STATION OF BARCELONA
Radio Ciutat de Badalona
Ràdio Ciutat de Badalona (RCB) is the municipal public radio station of Badalona (Barcelona). Founded in July 1981, it broadcasts 24 hours a day via FM on frequency 94.
Википедия
Emission nebula
An emission nebula is a nebula formed of ionized gases that emit light of various wavelengths. The most common source of ionization is high-energy ultraviolet photons emitted from a nearby hot star. Among the several different types of emission nebulae are H II regions, in which star formation is taking place and young, massive stars are the source of the ionizing photons; and planetary nebulae, in which a dying star has thrown off its outer layers, with the exposed hot core then ionizing them.
