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- '''Irradiance''' is a term in [[Radiometry|radiometry]]. It is defined as the change in Typical units are [<math>\frac{W}{m^2}</math>]. Irradiance typically varies as a function of wavelength.420 bytes (67 words) - 22:17, 2 January 2008
- 12 bytes (1 word) - 22:16, 2 January 2008
- 132 bytes (18 words) - 03:12, 4 September 2009
- Auto-populated based on [[Special:WhatLinksHere/Irradiance]]. Needs checking by a human.588 bytes (74 words) - 17:34, 11 January 2010
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- '''Irradiance''' is a term in [[Radiometry|radiometry]]. It is defined as the change in Typical units are [<math>\frac{W}{m^2}</math>]. Irradiance typically varies as a function of wavelength.420 bytes (67 words) - 22:17, 2 January 2008
- *[[irradiance]]46 bytes (3 words) - 09:55, 19 December 2007
- ...[[Irradiance|exitance]] from the back side of a surface and the incident [[irradiance]] on the front side.555 bytes (82 words) - 16:25, 10 February 2022
- ...[Irradiance|exitance]] from the front side of a surface and the incident [[irradiance]] on the front side.737 bytes (107 words) - 17:00, 25 January 2022
- * [[Irradiance]]428 bytes (39 words) - 15:17, 19 December 2007
- ...nd only for the lambertian case, is it possible to convert directly from [[irradiance]] to [[radiance]] by dividing by a factor of <math>\pi</math>.335 bytes (50 words) - 20:42, 19 December 2007
- ...ty''' is a term in [[radiometry]]. It is the ratio between the observed [[Irradiance|exitance]] and ideal [[Black-body_radiation|blackbody exitance]]:483 bytes (66 words) - 18:55, 30 October 2021
- {{r|Irradiance}}474 bytes (59 words) - 21:04, 11 January 2010
- {{r|Irradiance}}496 bytes (64 words) - 19:53, 11 January 2010
- {{r|Irradiance}}588 bytes (72 words) - 19:54, 11 January 2010
- {{r|Irradiance}}486 bytes (62 words) - 16:17, 11 January 2010
- Auto-populated based on [[Special:WhatLinksHere/Irradiance]]. Needs checking by a human.588 bytes (74 words) - 17:34, 11 January 2010
- ...lectivity]] of 0. The Planck black body equation describes the spectral [[Irradiance|exitance]] of an ideal black body. The study of black-body radiation was a ...\lambda</math> is in meters and that the output is a spectral [[Irradiance|irradiance]] in <math>[W/m^2*m]</math>. Omitting the <math>\pi</math> term from the n4 KB (537 words) - 09:19, 11 September 2022
- ...tal Panel on Climate Change) as the change in net, downward minus upward, irradiance (expressed in Watts per square metre, W/m<sup>2</sup>) at the [[tropopause]1 KB (206 words) - 12:06, 22 August 2008
- ...uthors = KH Schatten| year = 1993| title = A discussion of plausible solar irradiance variations, 1700–1992 | journal = J Geophys Res|volume = 98 | pages ...= ''et al.''| date = 2005 | title = Modeling the sun's magnetic field and irradiance since 1713| journal = Astrophys J| volume = 625 | pages = 522–38| url = h11 KB (1,443 words) - 19:34, 27 November 2012
- ...e level of [[solar radiation]] emitted by the Sun. Changes in total solar irradiance (TSI) are often related to the 11-year sunspot cycle. An increase in the n13 KB (1,869 words) - 22:22, 6 January 2011
- [http://www.spacewx.com/pdf/SET_21348_2004.pdf ISO 21348 Definitions of Solar Irradiance Spectral Categories]25 KB (3,994 words) - 17:54, 17 April 2010
- | heat flux density, irradiance || kg·s<sup>−3</sup>23 KB (3,590 words) - 20:32, 4 February 2024
- ...umference, recreational physical activity, race-ethnicity, regional solar irradiance, and age."<ref name="pmid20219959">{{cite journal| author=Millen AE, Wactaw23 KB (3,357 words) - 00:11, 31 January 2014
- ...nearly twice as distant from the Sun and receives only 25% of the solar [[irradiance]].41 KB (6,454 words) - 10:12, 28 February 2024