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irradiance$40844$ - translation to ιταλικό
![A drawing of a sunspot in the Chronicles of [[John of Worcester]], ca. 1100.](https://commons.wikimedia.org/wiki/Special:FilePath/ChroniclesofJohnofWorcester.jpg?width=200 "A drawing of a sunspot in the Chronicles of [[John of Worcester]], ca. 1100.")
![This version of the sunspot butterfly diagram was constructed by the solar group at NASA Marshall Space Flight Center. The newest version can be found at [http://solarcyclescience.com/solarcycle.html solarcyclescience.com]](https://commons.wikimedia.org/wiki/Special:FilePath/Sunspot-bfly.gif?width=200 "This version of the sunspot butterfly diagram was constructed by the solar group at NASA Marshall Space Flight Center. The newest version can be found at [http://solarcyclescience.com/solarcycle.html solarcyclescience.com]")
![Time vs. solar latitude diagram of the radial component of the solar magnetic field, averaged over successive solar rotation. The "butterfly" signature of sunspots is clearly visible at low latitudes. Diagram constructed by the solar group at NASA Marshall Space Flight Center. The newest version can be found at [http://solarcyclescience.com/solarcycle.html solarcyclescience.com]](https://commons.wikimedia.org/wiki/Special:FilePath/Synoptic-solmag.jpg?width=200 "Time vs. solar latitude diagram of the radial component of the solar magnetic field, averaged over successive solar rotation. The \"butterfly\" signature of sunspots is clearly visible at low latitudes. Diagram constructed by the solar group at NASA Marshall Space Flight Center. The newest version can be found at [http://solarcyclescience.com/solarcycle.html solarcyclescience.com]")
![ISAS]] (Japan) and [[NASA]] (US).](https://commons.wikimedia.org/wiki/Special:FilePath/The Solar Cycle XRay hi.jpg?width=200 "ISAS]] (Japan) and [[NASA]] (US).")
Βικιπαίδεια
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).
