irradiance - translation to αραβικά
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irradiance - translation to αραβικά

AREAL DENSITY OF INCOMING RADIANT FLUX
Spectral irradiance; Radiation flux; W/m2; Radiant flux density; W/m²; Photon irradiance

irradiance         
تألق إشعاع
insolation         
  • Insolation variation by month; 1984–1993 averages for January (top) and April (bottom)
  • The shield effect of Earth's atmosphere on solar irradiation. The top image is the annual mean solar irradiation (or insolation) at the top of [[Earth's atmosphere]] (TOA); the bottom image shows the annual insolation reaching the Earth's surface after passing through the atmosphere. The two images use the same color scale.
  • <math>\overline{Q}^\text{day}</math>, the theoretical daily-average irradiation at the top of the atmosphere, where θ is the polar angle of the Earth's orbit, and θ&nbsp;=&nbsp;0 at the vernal equinox, and θ&nbsp;=&nbsp;90° at the summer solstice; φ is the latitude of the Earth. The calculation assumed conditions appropriate for 2000{{nbsp}}A.D.: a solar constant of ''S''<sub>0</sub>&nbsp;=&nbsp;1367&nbsp;W{{nnbsp}}m<sup>−2</sup>, obliquity of ε&nbsp;=&nbsp;23.4398°, longitude of perihelion of ϖ&nbsp;=&nbsp;282.895°, eccentricity ''e''&nbsp;=&nbsp;0.016704. Contour labels (green) are in units of&nbsp;W{{nnbsp}}m<sup>−2</sup>.
  • Variations in Earth's orbit, resulting changes in solar energy flux at high latitude, and the observed glacial cycles.
  • A [[pyranometer]], used to measure global irradiance
  • oblique]] sunbeam distributes its light energy over twice as much area.
  • Spherical triangle for application of the spherical law of cosines for the calculation the solar zenith angle Θ for observer at [[latitude]] φ and [[longitude]] λ from knowledge of the hour angle h and solar declination δ. (δ is latitude of subsolar point, and h is relative longitude of subsolar point).
  • [[Sunlight]] carries radiant energy in the wavelengths of [[visible light]]. Radiant energy may be developed for [[solar power]] generation.
  • Solar irradiance spectrum above atmosphere and at surface
  • Global Map of Direct Normal Radiation <ref name= "Global Solar Atlas" />
  • Global Map of Global Horizontal Radiation <ref name="Global Solar Atlas">World Bank. 2017. Global Solar Atlas. https://globalsolaratlas.info</ref>
POWER PER UNIT AREA RECEIVED FROM THE SUN IN THE FORM OF ELECTROMAGNETIC RADIATION
Solar radiation; Insolation; Solar Radiation; Solar radiance; Solar irradiation; Solar insolation; Solar incidence; Earth's insolation; Solar flux; Total solar irradiance; Total Solar Irradiance; Global insolation; Horizontal irradiation; Global Horizontal Irradiance; Solar potential
تشميس ، تعريض للشمس
insolation         
  • Insolation variation by month; 1984–1993 averages for January (top) and April (bottom)
  • The shield effect of Earth's atmosphere on solar irradiation. The top image is the annual mean solar irradiation (or insolation) at the top of [[Earth's atmosphere]] (TOA); the bottom image shows the annual insolation reaching the Earth's surface after passing through the atmosphere. The two images use the same color scale.
  • <math>\overline{Q}^\text{day}</math>, the theoretical daily-average irradiation at the top of the atmosphere, where θ is the polar angle of the Earth's orbit, and θ&nbsp;=&nbsp;0 at the vernal equinox, and θ&nbsp;=&nbsp;90° at the summer solstice; φ is the latitude of the Earth. The calculation assumed conditions appropriate for 2000{{nbsp}}A.D.: a solar constant of ''S''<sub>0</sub>&nbsp;=&nbsp;1367&nbsp;W{{nnbsp}}m<sup>−2</sup>, obliquity of ε&nbsp;=&nbsp;23.4398°, longitude of perihelion of ϖ&nbsp;=&nbsp;282.895°, eccentricity ''e''&nbsp;=&nbsp;0.016704. Contour labels (green) are in units of&nbsp;W{{nnbsp}}m<sup>−2</sup>.
  • Variations in Earth's orbit, resulting changes in solar energy flux at high latitude, and the observed glacial cycles.
  • A [[pyranometer]], used to measure global irradiance
  • oblique]] sunbeam distributes its light energy over twice as much area.
  • Spherical triangle for application of the spherical law of cosines for the calculation the solar zenith angle Θ for observer at [[latitude]] φ and [[longitude]] λ from knowledge of the hour angle h and solar declination δ. (δ is latitude of subsolar point, and h is relative longitude of subsolar point).
  • [[Sunlight]] carries radiant energy in the wavelengths of [[visible light]]. Radiant energy may be developed for [[solar power]] generation.
  • Solar irradiance spectrum above atmosphere and at surface
  • Global Map of Direct Normal Radiation <ref name= "Global Solar Atlas" />
  • Global Map of Global Horizontal Radiation <ref name="Global Solar Atlas">World Bank. 2017. Global Solar Atlas. https://globalsolaratlas.info</ref>
POWER PER UNIT AREA RECEIVED FROM THE SUN IN THE FORM OF ELECTROMAGNETIC RADIATION
Solar radiation; Insolation; Solar Radiation; Solar radiance; Solar irradiation; Solar insolation; Solar incidence; Earth's insolation; Solar flux; Total solar irradiance; Total Solar Irradiance; Global insolation; Horizontal irradiation; Global Horizontal Irradiance; Solar potential
‎ تَشْميس:مُعالَجَةٌ شَمْسِيَّة, ضَرْبَةُ الشَّمْس‎

Ορισμός

Irradiance

Βικιπαίδεια

Irradiance

In radiometry, irradiance is the radiant flux received by a surface per unit area. The SI unit of irradiance is the watt per square metre (W⋅m−2). The CGS unit erg per square centimetre per second (erg⋅cm−2⋅s−1) is often used in astronomy. Irradiance is often called intensity, but this term is avoided in radiometry where such usage leads to confusion with radiant intensity. In astrophysics, irradiance is called radiant flux.

Spectral irradiance is the irradiance of a surface per unit frequency or wavelength, depending on whether the spectrum is taken as a function of frequency or of wavelength. The two forms have different dimensions and units: spectral irradiance of a frequency spectrum is measured in watts per square metre per hertz (W⋅m−2⋅Hz−1), while spectral irradiance of a wavelength spectrum is measured in watts per square metre per metre (W⋅m−3), or more commonly watts per square metre per nanometre (W⋅m−2⋅nm−1).

Παραδείγματα από το σώμα κειμένου για irradiance
1. Many have published evidence suggesting changes are due to either a natural 1,500 year climate cycle or variations in the sun‘s irradiance.
2. These particles disrupt satellites and are hazardous to astronauts outside the protection of Earth‘s magnetic field. – Monitoring the sun‘s energy output (the "total solar irradiance" or "solar constant") as well as variations in the sun‘s extreme ultraviolet radiation, both of which are important to understand the impact of solar variability on Earth‘s climate. – Identifying the source regions and acceleration mechanisms of the solar wind, a thin stream of ionized gas that constantly flows from the sun and buffets Earth‘s magnetosphere.