Radiative flux, also known as radiative flux density or radiation flux (or sometimes power flux density), is the amount of power radiated through a given...
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through a unit area (J·m−2·s−1). The radiative flux and heat flux are specific cases of energy flux. Particle flux, the rate of transfer of particles through...
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the globe. A planet in radiative equilibrium with its parent star and the rest of space can be characterized by net zero radiative forcing and by a planetary...
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used to describe spectral flux density vary between fields, sometimes including adjectives such as "electromagnetic" or "radiative", and sometimes dropping...
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The simplest form of radiative transfer involves a collinear beam of radiation traveling through a sample to a detector. That flux can be reduced by absorption...
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Second law of thermodynamics (section Second law statements, such as the Clausius inequality, involving radiative fluxes)
radiation from all matter, most entropy flux calculations involve incident, reflected and emitted radiative fluxes. The energy and entropy of unpolarized...
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daytime radiative cooling (PDRC) (also passive radiative cooling, daytime passive radiative cooling, radiative sky cooling, photonic radiative cooling...
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sometimes called energy flux density, to distinguish it from the first definition. Radiative flux, heat flux, and sound energy flux density (also sound intensity)...
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daytime radiative cooling (PDRC) (also passive radiative cooling, daytime passive radiative cooling, radiative sky cooling, photonic radiative cooling...
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scattering processes. The equation of radiative transfer describes these interactions mathematically. Equations of radiative transfer have application in a wide...
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radiometry, radiant flux or radiant power is the radiant energy emitted, reflected, transmitted, or received per unit time, and spectral flux or spectral power...
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radiative flux density (that is, radiative flux per unit of frequency) on frequency. Given frequency ν {\displaystyle \nu } in Hz and radiative flux density...
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that will allow the outgoing radiative power, escaping the top of the atmosphere, to be equal to the absorbed radiative power of sunlight. When applied...
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Poynting vector (redirect from Poynting flux)
Poynting vector (or Umov–Poynting vector) represents the directional energy flux (the energy transfer per unit area, per unit time) or power flow of an electromagnetic...
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A radiative zone is a layer of a star's interior where energy is primarily transported toward the exterior by means of radiative diffusion and thermal...
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Heat transfer (section Radiative cooling)
dioxide determines the radiative balance of Earth's atmosphere, carbon dioxide removal techniques can be applied to reduce the radiative forcing. Solar radiation...
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the heat flux. The heat flux can have different origins; in principle convective, radiative as well as conductive heat can be measured. Heat flux sensors...
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Lumen (unit) (redirect from Orders of magnitude (luminous flux))
light source (that uniformly radiates in all directions) with a luminous intensity of one candela has a total luminous flux of 1 cd × 4π sr = 4π cd⋅sr =...
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record of radiative fluxes at the top of the atmosphere (TOA) for climate change analysis. Doubling the accuracy of estimates of radiative fluxes at TOA...
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Electromagnetic flux may refer to one of the following: Flux or flux density of electromagnetic radiation Electric flux and magnetic flux Radiative flux. This disambiguation...
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daytime radiative cooling (PDRC) (also passive radiative cooling, daytime passive radiative cooling, radiative sky cooling, photonic radiative cooling...
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in time. Radiative equilibrium is the specific case of thermal equilibrium, for the case in which the exchange of heat is done by radiative heat transfer...
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Eddington luminosity (redirect from Eddington flux)
with steady winds driven by broad-spectrum radiation is that both the radiative flux and gravitational acceleration scale with r−2. The ratio between these...
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Planetary equilibrium temperature (redirect from Radiative equilibrium temperature)
temperature that a planet would be if it were in radiative equilibrium, typically under the assumption that it radiates as a black body being heated only by its...
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I_{\mathrm {o} }~.} From the fields calculated above, one can find the radiated flux (power per unit area) at any point as the magnitude of the real part...
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Streamer (software) (redirect from Streamer: A Radiative Transfer Model)
atmospheric radiative transfer codes Atmospheric radiative transfer codes DISORT Key, J. and A.J. Schweiger, 1998, Tools for atmospheric radiative transfer:...
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Greenhouse effect (section Radiative balance)
energy flows reduce radiative surface cooling (net upward radiative energy flow). Latent heat transport and thermals provide non-radiative surface cooling...
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it. In pictorial form, this electric field is shown as "lines of flux" being radiated from a dot (the charge). These are called Gauss lines. Note that...
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Thermal radiation (redirect from Radiative heat transfer)
delivery of the heat. Radiative heat flux and effects are given as follows: At distances on the scale of the wavelength of a radiated electromangetic wave...
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above) may differ largely from the effective temperature given by the radiative flux of the stellar surface. For example, the color temperature of an A0V...
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