long-wavelength radiation oor Spaans

long-wavelength radiation

Vertalings in die woordeboek Engels - Spaans

radiación de onda larga

Termium

Geskatte vertalings

Vertoon algoritmies gegenereerde vertalings

Soortgelyke frases

long wavelength infra-red radiation
radiación de onda larga
long-wavelength ultraviolet radiation
UVA · rayos ultravioleta de tipo A · rayos uva · uva

voorbeelde

wedstryd
woorde
Advanced filtering
Voorbeelde moet herlaai word.
This glass, however, is essentially opaque to long-wavelength radiation above 3 or 4 μm.
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Long-wavelength radiation (above 1 100 nm) was exploited by thermoelectric devices.
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Many white paints are also essentially black for long-wavelength radiation.
Oh mi mi... no confías en mi?Literature Literature
A large surface has α = 0.6 for long-wavelength radiation and α = 0.95 for solar radiation.
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Specifically, the researchers explored new routes for efficiently using mid-infrared pump lasers and producing long-wavelength radiation (up to 60 micrometres).
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Extensive investigations of photo-ionisation, induced in the air by the generation of long-wavelength radiation, allowed them to generate pulses that propagate on curved trajectories.
Vuelvo en un minutocordis cordis
Then the image will have to be assembled out of the long-wavelength Hawking radiation.
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Physicists had learned to prepare coherent radiation for long wavelengths.
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The Earth is warmed by this radiation, and in response radiates infrared (long wavelength) energy back into space.
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Some kinds of radiation have very long wavelengths, being measured in miles.
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This is in the range of infra-red radiation, and is too long a wavelength for our eyes to see.
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Absorption occurs regardless of the wavelength of the radiation entering (as long as it is small compared to the hole).
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When using a synchrotron in crystallography for diffraction experiments at long wavelengths it is necessary to minimise background scatter radiation.
Están tirando piedras a un gigantecordis cordis
On either side of the visible light spectrum are long-wavelength radiations (infrared) and short-wavelength radiations (UV).
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The properties of the waves vary greatly – from extremely low frequency, long wavelength radiation to high frequency, short wavelength radiation.
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Infrared astronomy studies radiation with a wavelength that is too long to be visible to the naked eye but is shorter than radio waves.
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Radiations that have longer wavelengths include heat waves and the very long radio waves.
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At 3.5-metres in diameter the mirror will collect long-wavelength radiation from some of the coldest and most distant objects in the Universe.
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While most of the short wavelength solar radiation passes through the glass, Low-E reflects most of the long wavelength radiation generated by heaters inwards, improving the buildings thermal comfort systems.
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Scientists have known about the natural 'greenhouse effect' for more than a century (Arrhenius 1896): the Earth maintains its equilibrium temperature through a delicate balance between the incoming solar energy (short wavelength radiation) it absorbs and the outgoing infra-red energy (long wavelength radiation) that it emits and some of which escapes into space.
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Thermal cameras, on the other hand, detect radiation with mid-length or long wavelengths, which is called infrared radiation.
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This means, that the carbon dioxide in the atmosphere is transparent to the light and heat coming from the Sun, but is opaque to the long wavelength infrared radiation coming from the hot planet.
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From a point in space called the 2nd Lagrangian Point (or L2), its 3.5-metre diameter mirror will collect long-wavelength infrared radiation from some of the coolest and most distant objects in the Universe.
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From a point in space called the 2nd Lagrangian Point (or L2), its 3.5-m diameter mirror will collect long-wavelength infrared radiation from some of the coolest and most distant objects in the Universe.
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In fact, all objects emit thermal radiation (as long as their temperature is above Absolute Zero, or-# degrees Celsius), but no object emits thermal radiation perfectly; rather, they are better at emitting/absorbing some wavelengths of light than others. These uneven efficiencies make it difficult to study the interaction of light, heat and matter using normal objects
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43 sinne gevind in 12 ms. Hulle kom uit baie bronne en word nie nagegaan nie.