thermal radiation oor Indonesies
thermal radiation
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(physics) The electromagnetic radiation emitted from a body as a consequence of its temperature; increasing the temperature of the body increases the amount of radiation produced, and shifts it to shorter wavelengths (higher frequencies) in a manner explained only by quantum mechanics.
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Radiasi termal
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electromagnetic radiation generated by the thermal motion of charged particles in matter
Many scientists fear that the increased concentrations of greenhouse gases have prevented additional thermal radiation from leaving the Earth.
Banyak ilmuwan waswas bahwa peningkatan konsentrasi gas rumah kaca telah menghambat keluarnya radiasi termal tambahan dari Bumi.
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This is a concept known as thermal radiation.
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In the late 19th century, thermal radiation had been fairly well characterized experimentally.
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He proposed his law of thermal radiation in 1859, and gave a proof in 1861.
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She can sense thermal radiation.
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Black-body radiation is also called thermal radiation, cavity radiation, complete radiation or temperature radiation.
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From the core out to about 0.7 solar radii, thermal radiation is the primary means of energy transfer.
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Central to this ability is being able to manage the thermal radiation that's all around us.
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Many scientists fear that the increased concentrations of greenhouse gases have prevented additional thermal radiation from leaving the Earth.
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He proposed a mathematical model in which the thermal radiation was in equilibrium with a set of harmonic oscillators.
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The radiation represents a conversion of a body's internal energy into electromagnetic energy, and is therefore called thermal radiation.
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Thermal radiation is generated when energy from the movement of charged particles within atoms is converted to electromagnetic radiation.
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The first model that was able to explain the full spectrum of thermal radiation was put forward by Max Planck in 1900.
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The Wien approximation was originally proposed as a description of the complete spectrum of thermal radiation, although it failed to accurately describe long wavelength (low frequency) emission.
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Wien's approximation (also sometimes called Wien's law or the Wien distribution law) is a law of physics used to describe the spectrum of thermal radiation (frequently called the blackbody function).
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Kirchhoff's law has another corollary: the emissivity cannot exceed one (because the absorptivity cannot, by conservation of energy), so it is not possible to thermally radiate more energy than a black body, at equilibrium.
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The sensors installed in forward-looking infrared cameras, as well as those of other thermal imaging cameras, use detection of infrared radiation, typically emitted from a heat source (thermal radiation), to create an image assembled for video output.
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The design essentially consists of a lens to focus the infrared thermal radiation on to a detector, which converts the radiant power to an electrical signal that can be displayed in units of temperature after being compensated for ambient temperature.
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Thermal Radiation (Light and Heat): A nuclear blast creates an intense flash of light that blinds or dazzles people far from the point of explosion —up to 13 miles [21 km] in daytime and 53 miles [85 km] at night in a one-megaton blast.
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For example, the motions and rotations of celestial bodies such as planets may appear perpetual, but are actually subject to many processes that slowly dissipate their kinetic energy, such as solar wind, interstellar medium resistance, gravitational radiation and thermal radiation, so they will not keep moving forever.
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They also look for odd thermal patterns and radiation spikes.
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Each CERES instrument is a radiometer which has three channels – a shortwave (SW) channel to measure reflected sunlight in 0.2–5 μm region, a channel to measure Earth-emitted thermal radiation in the 8–12 μm "window" or "WN" region, and a Total channel to measure entire spectrum of outgoing Earth's radiation (>0.2 μm).
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This is the condition for the applicability of Kirchhoff's law of thermal radiation: the black-body curve is characteristic of thermal light, which depends only on the temperature of the walls of the cavity, provided that the walls of the cavity are completely opaque and are not very reflective, and that the cavity is in thermodynamic equilibrium.
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This means that at thermodynamic equilibrium the amount of every wavelength in every direction of thermal radiation emitted by a body at temperature T, black or not, is equal to the corresponding amount that the body absorbs because it is surrounded by light at temperature T. When the body is black, the absorption is obvious: the amount of light absorbed is all the light that hits the surface.
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Seismic... and radiation... and thermal.
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In quantum mechanics, the black hole emits Hawking radiation and so can come to thermal equilibrium with a gas of radiation (not compulsory).
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43 sinne gevind in 8 ms. Hulle kom uit baie bronne en word nie nagegaan nie.