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alternate case: spectral radiance
Reflectance
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spectral radiance in frequency reflected by that surface; Le,Ω,νi is the spectral radiance received by that surface; Le,Ω,λr is the spectral radianceTransmittance (1,057 words) [view diff] exact match in snippet view article find links to article
the spectral radiance in frequency transmitted by that surface; Le,Ω,νi is the spectral radiance received by that surface; Le,Ω,λt is the spectral radianceAbsorptance (536 words) [view diff] exact match in snippet view article find links to article
spectral radiance in frequency absorbed by that surface; L e , Ω , ν i {\displaystyle L\mathrm {_{e,\Omega ,\nu }^{i}} } is the spectral radianceAttenuation coefficient (2,210 words) [view diff] exact match in snippet view article find links to article
{d} z}},\end{aligned}}} where Le,Ω,ν is the spectral radiance in frequency; Le,Ω,λ is the spectral radiance in wavelength. When a narrow (collimated) beamGRS 1124-683 (476 words) [view diff] no match in snippet view article find links to article
The gamma-ray and X-ray source GRS 1124-683, discovered by the Granat mission and Ginga, is a system containing a black hole candidate. The system alsoEmissivity (4,090 words) [view diff] exact match in snippet view article find links to article
\end{aligned}}} where Le,Ω,ν is the spectral radiance in frequency of that surface; Le,Ω,ν° is the spectral radiance in frequency of a black body at theLuminance (1,336 words) [view diff] exact match in snippet view article find links to article
falls within a given solid angle. The procedure for conversion from spectral radiance to luminance is standardized by the CIE and ISO. Brightness is theWien's displacement law (3,412 words) [view diff] exact match in snippet view article find links to article
the wavelength version of Wien's displacement law states that the spectral radiance of black-body radiation per unit wavelength, peaks at the wavelengthPhosphorus deficiency (1,206 words) [view diff] exact match in snippet view article find links to article
compounds and elements. Additional phosphorus detection methods such as spectral radiance and inductively coupled plasma spectrometry (ICP) are also implementedBlack-body radiation (8,774 words) [view diff] exact match in snippet view article find links to article
(that is, the net amount of radiation leaving its surface, called the spectral radiance) is determined solely by the equilibrium temperature and does notSpectroradiometer (3,091 words) [view diff] exact match in snippet view article find links to article
spectrometer is then able to provide measurements of spectral irradiance, spectral radiance and/or spectral flux. This data is also then used with built in orColorimetry (1,052 words) [view diff] exact match in snippet view article find links to article
tristimulus values of a color. A spectroradiometer measures the absolute spectral radiance (intensity) or irradiance of a light source. A spectrophotometer measuresPlanckian locus (2,259 words) [view diff] exact match in snippet view article find links to article
constant for spectral radiance) instead of c1 (the “regular” first radiation constant), in which case the formula would give the spectral radiance L(λ,T) ofSentinel-4 (1,652 words) [view diff] exact match in snippet view article find links to article
than 0.05%. The in-flight absolute radiometric accuracy of the Earth spectral radiance and of the Sun irradiance is required to be better than 3% with aHyperspectral imaging (4,957 words) [view diff] exact match in snippet view article find links to article
time-averaged spectral radiance at 2078 cm−1 corresponding to a CO2 emission line. Bottom panel: Contour map of the spectral radiance at 2580 cm−1 correspondingList of physical constants (1,713 words) [view diff] exact match in snippet view article find links to article
Retrieved 2024-05-18. "2022 CODATA Value: first radiation constant for spectral radiance". The NIST Reference on Constants, Units, and Uncertainty. NIST. MayStandard illuminant (4,815 words) [view diff] exact match in snippet view article find links to article
method can be applied to. For each of these standard illuminants, spectral radiance factor data are supplied for five pairs of nonfluorescent samplesMelting point (3,069 words) [view diff] exact match in snippet view article find links to article
materials, this may require extrapolation by several hundred degrees. The spectral radiance from an incandescent body is known to be a function of its temperaturePlanck constant (6,180 words) [view diff] exact match in snippet view article find links to article
Planck constant. The expression formulated by Planck showed that the spectral radiance per unit frequency of a body for frequency ν at absolute temperatureAperture (antenna) (3,345 words) [view diff] exact match in snippet view article
being bathed in black-body radiation of temperature T, receives a spectral radiance (power per unit area per unit frequency per unit solid angle) givenLucy (spacecraft) (4,390 words) [view diff] exact match in snippet view article
instrument collects data from 6–75 μm and has a noise equivalent spectral radiance (NESR) of 2.310–8 W cm−2 sr−1 cm−1 between 300 cm−1 (7.4 μm) and 1350 cm−1Heat transfer (8,475 words) [view diff] exact match in snippet view article find links to article
unit or thermal resistance) to temperature difference. Radiance, or spectral radiance, is a measure of the quantity of radiation that passes through orTemperature (13,010 words) [view diff] exact match in snippet view article find links to article
accurate temperature measurement because the frequency of maximum spectral radiance of black-body radiation is directly proportional to the temperatureX-ray astronomy (8,115 words) [view diff] exact match in snippet view article find links to article
results in ever greater demands for finer angular resolution and spectral radiance. There are inherent difficulties in making X-ray/optical, X-ray/radioRemote sensing (oceanography) (4,497 words) [view diff] exact match in snippet view article
}T}}-1}}\cdot \epsilon } With B ( ν , T ) {\displaystyle B(\nu ,T)} the spectral radiance, h {\displaystyle h} the Planck constant; c {\displaystyle c} the