File:Solar spectrum es.svg
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Español: Esta figura muestra el espectro de la radiación solar para la luz directa tanto en la parte superior de la atmósfera de la tierra y al nivel del mar. El sol produce luz con una distribución similar a lo que se esperaría de un cuerpo negro a 5525 ºK (5250 °C), que es aproximadamente temperatura de la superficie del sol. Cuando la luz pasa a través de la atmósfera, parte es absorbida por los gases con bandas de absorción específicas. La luz adicional se redistribuye por dispersión de Raleigh, que es responsable del color azul de la atmósfera. Estas curvas se basan en la Sociedad Americana de Pruebas y Materiales (ASTM) espectros de referencia terrestre, que son normas adoptadas por la industria fotovoltaica para asegurar condiciones de prueba consistentes y son similares a la luz que se podía esperar en América del Norte. También se distinguen las regiones de la luz ultravioleta, visible e infrarroja.
English: This figure shows the solar radiation spectrum for direct light at both the top of the Earth's atmosphere and at sea level. The sun produces light with a distribution similar to what would be expected from a 5525 K (5250 °C) blackbody, which is approximately the sun's surface temperature. As light passes through the atmosphere, some is absorbed by gases with specific absorption bands. Additional light is redistributed by Raleigh scattering, which is responsible for the atmosphere's blue color. These curves are based on the American Society for Testing and Materials (ASTM) Terrestrial Reference Spectra, which are standards adopted by the photovoltaics industry to ensure consistent test conditions and are similar to the light that could be expected in North America. Regions for ultraviolet, visible and infrared light are indicated.
Italiano: La figura mostra lo spettro della radiazione solare per illuminazione diretta sia all'inizio che alla fine del'atmosfera terrestra. Il sole produce una luce con una distribuzione simile a quella che ci si attenderebbe da un corpo nero a 5525 K (5250 °C), che è approssimativamente la temperatura superficiale del sole. Mano a mano che la luce passa attraverso l'atmosfera, parte della radiazione è assorbita dai gas in specifiche bande di assorbimento. Un contributo additivo è dovuto allo scattering Raleigh, che è responsabile per il colore blu dell'atmosfera. Le curve sono basate sugli spettri di riferimento dell'American Society for Testing and Materials (ASTM), che sono standard adottati dall'industria fotovoltaica per assicurare condizioni di prova consistenti e sono simili al tipo di radiazione che è possibile aspettarsi nell'America del nord. Sono indicate le regioni per l'ultravioletto, il visibile e la luce infrarossa. |
| Date | |
| Source | File:Solar_spectrum_en.svg |
| Author | Nick84 |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 14:20, 25 February 2019 | | 800 × 600 (47 KB) | Tuvalkin (talk | contribs) | W → kW |
| 11:02, 20 June 2016 |  | 800 × 600 (47 KB) | Mabrigar (talk | contribs) | User created page with UploadWizard |
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