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background radiation - ترجمة إلى إيطالي
LEVEL OF IONIZING RADIATION PRESENT IN THE NATURAL ENVIRONMENT
Background Radiation; Natural radioactivity; Terrestrial radiation; Natural radiation; Background count; Natural background radiation; Environmental radiation; Radiation background; Ambient radiation
![gamma radiation]] level is 9.8 [[μR/h]] (0.82 mSv/a) This is very close to the world average background radiation of 0.87 mSv/a from cosmic and terrestrial sources.](https://commons.wikimedia.org/wiki/Special:FilePath/Atomic Testing Museum weather display cropped.jpg?width=200 "gamma radiation]] level is 9.8 [[μR/h]] (0.82 mSv/a) This is very close to the world average background radiation of 0.87 mSv/a from cosmic and terrestrial sources.")
background radiation
radiazione di sfondo (radiazione non intensa che si irradia su tutta la terra)
electromagnetic wave
![opacity]]) of various [[wavelength]]s of electromagnetic radiation](https://commons.wikimedia.org/wiki/Special:FilePath/Atmospheric electromagnetic opacity.svg?width=200 "opacity]]) of various [[wavelength]]s of electromagnetic radiation")
![[[Electromagnetic spectrum]] with visible light highlighted](https://commons.wikimedia.org/wiki/Special:FilePath/EM spectrumrevised.png?width=200 "[[Electromagnetic spectrum]] with visible light highlighted")
![far field]] part of the electromagnetic field around a transmitter. A part of the "near-field" close to the transmitter, forms part of the changing [[electromagnetic field]], but does not count as electromagnetic radiation.](https://commons.wikimedia.org/wiki/Special:FilePath/FarNearFields-USP-4998112-1.svg?width=200 "far field]] part of the electromagnetic field around a transmitter. A part of the \"near-field\" close to the transmitter, forms part of the changing [[electromagnetic field]], but does not count as electromagnetic radiation.")
![[[James Clerk Maxwell]]](https://commons.wikimedia.org/wiki/Special:FilePath/James Clerk Maxwell sitting.jpg?width=200 "[[James Clerk Maxwell]]")
!['''Legend:'''<br />
γ = [[Gamma ray]]s<br />
<br />
HX = Hard [[X-ray]]s<br />
SX = Soft X-Rays<br />
<br />
EUV = Extreme-[[ultraviolet]]<br />
NUV = Near-ultraviolet<br />
<br />
[[Visible light]] (colored bands)<br />
<br />
NIR = Near-[[infrared]]<br />
MIR = Mid-infrared<br />
FIR = Far-infrared<br />
<br />
EHF = [[Extremely high frequency]] (microwaves)<br />
SHF = [[Super-high frequency]] (microwaves)<br />
<br />
UHF = [[Ultrahigh frequency]] (radio waves)<br />
VHF = [[Very high frequency]] (radio)<br />
HF = [[High frequency]] (radio)<br />
MF = [[Medium frequency]] (radio)<br />
LF = [[Low frequency]] (radio)<br />
VLF = [[Very low frequency]] (radio)<br />
VF = [[Voice frequency]]<br />
ULF = [[Ultra-low frequency]] (radio)<br />
SLF = [[Super-low frequency]] (radio)<br />
ELF = [[Extremely low frequency]] (radio)](https://commons.wikimedia.org/wiki/Special:FilePath/Light spectrum.svg?width=200 "'''Legend:'''<br />
γ = [[Gamma ray]]s<br />
<br />
HX = Hard [[X-ray]]s<br />
SX = Soft X-Rays<br />
<br />
EUV = Extreme-[[ultraviolet]]<br />
NUV = Near-ultraviolet<br />
<br />
[[Visible light]] (colored bands)<br />
<br />
NIR = Near-[[infrared]]<br />
MIR = Mid-infrared<br />
FIR = Far-infrared<br />
<br />
EHF = [[Extremely high frequency]] (microwaves)<br />
SHF = [[Super-high frequency]] (microwaves)<br />
<br />
UHF = [[Ultrahigh frequency]] (radio waves)<br />
VHF = [[Very high frequency]] (radio)<br />
HF = [[High frequency]] (radio)<br />
MF = [[Medium frequency]] (radio)<br />
LF = [[Low frequency]] (radio)<br />
VLF = [[Very low frequency]] (radio)<br />
VF = [[Voice frequency]]<br />
ULF = [[Ultra-low frequency]] (radio)<br />
SLF = [[Super-low frequency]] (radio)<br />
ELF = [[Extremely low frequency]] (radio)")
![light]] (blue, green, and red) with a distance scale in micrometers along the x-axis.](https://commons.wikimedia.org/wiki/Special:FilePath/VisibleEmrWavelengths.svg?width=200 "light]] (blue, green, and red) with a distance scale in micrometers along the x-axis.")
FORM OF ENERGY EMITTED AND ABSORBED BY PARTICLES WHICH ARE CHARGED WHICH SHOWS WAVE-LIKE BEHAVIOR AS IT TRAVELS THROUGH SPACE
Electromagnectic radiation; Electromagnetic wave; Light wave; Electromagnetic waves; EM radiation; E.M. radiation; E. M. radiation; RF radiation; Electro-magnetic radiation; Magnetoelectric wave; Theory of radiation; Electromagnetic Radiation; Radiation emission; Radiation emissions; Em wave; EM wave; EM Waves; E-M Waves; Em waves; Electronic smog; Electromagnetic Wave; Electromagnetic wave theory; Electro magnetic waves; Emag waves; Electrical smog; Electromagnetic resonance; Electromagnetic Waves; Electro magnetic energy; Electromagnetic emission; Electromagnetic emissions; Photon radiation; Electromagnetic signal; E/M wave
onda elettromagnetica, onda di radiazione dallo spettro elettromagnetico
thermal radiation
![Thermal radiation in visible light can be seen on this hot metalwork. Its emission in the [[infrared]] is invisible to the human eye. [[Infrared cameras]] are capable of capturing this infrared emission (see [[Thermography]]).](https://commons.wikimedia.org/wiki/Special:FilePath/Hot metalwork.jpg?width=200 "Thermal radiation in visible light can be seen on this hot metalwork. Its emission in the [[infrared]] is invisible to the human eye. [[Infrared cameras]] are capable of capturing this infrared emission (see [[Thermography]]).")
![National Research Council]], near [[Ottawa]], [[Ontario]], Canada](https://commons.wikimedia.org/wiki/Special:FilePath/Radiant heat panel nrc ottawa.jpg?width=200 "National Research Council]], near [[Ottawa]], [[Ontario]], Canada")
ELECTROMAGNETIC RADIATION GENERATED BY THE THERMAL MOTION OF CHARGED PARTICLES IN MATTER
Radiant heat; Heat radiator; Thermal radiator; Thermal Radiation; Thermal light; Heat radiation; Radiative heat transfer; Radiation of heat; Thermal emission; Radiation heat transfer; Radiation properties
fenomeno termico
تعريف
microwave background
¦ noun Astronomy a weak uniform microwave radiation which is detectable in nearly every direction of the sky, believed to be evidence of the big bang.
ويكيبيديا
Background radiation
Background radiation is a measure of the level of ionizing radiation present in the environment at a particular location which is not due to deliberate introduction of radiation sources.
Background radiation originates from a variety of sources, both natural and artificial. These include both cosmic radiation and environmental radioactivity from naturally occurring radioactive materials (such as radon and radium), as well as man-made medical X-rays, fallout from nuclear weapons testing and nuclear accidents.
أمثلة من مجموعة نصية لـ٪ 1
1. For the general public, it‘s about what you get from background radiation – 3 mSv per year.
2. Average background radiation over a year nationwide is about 350 milirems a year.
3. The background radiation we can measure today corresponds to a temperature that is barely 2.7 degrees above absolute zero."
4. Rees, for his work studying cosmic microwave background radiation and how galaxies form; and Canadian Arthur B.
5. These were imprinted in the cosmic microwave background radiation, the embers of the Big Bang, when the universe was only 400,000 years old.