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  • Deutsch: Die Effektivtemperatur der Sonne (5777 K) ist die Temperatur, die ein gleich großer Schwarzer Körper haben müsste, um dieselbe Strahlungsleistung abzugeben.
  • English: The effective temperature, or blackbody temperature, of the Sun (5777 K) is the temperature a black body of the same size must have to yield the same total emissive power.
Date
Source
  • Deutsch: Selbst erstellt. Sonnenspektrum nach dem WRC-Spektrum in M. Iqbal: An Introduction to Solar Radiation, Academic Press 1983, Tabelle C1. Spektrale Bestrahlungsstärke des Schwarzen Körpers berechnet aus Planckspektrum für T gleich 5777 K und Quellenausdehnung 6.8e-5 steradian (Sonnenscheibe).
  • English: Drawn by myself. The solar spectrum is the WRC spectrum provided by M. Iqbal: An Introduction to Solar Radiation, Academic Press 1983, Table C1. The black body spectral irradiance has been computed from a black-body spectrum for T equal 5777 K and assuming a solid angle of 6.8e-5 steradian for the source (the solar disk).
Author Sch
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current09:54, 5 May 2006Thumbnail for version as of 09:54, 5 May 20063,000 × 2,200 (65 KB)Sch*Description: {{german}} Die Effektivtemperatur der Sonne (5777 K) ist die Temperatur, die ein gleich großer Schwarzer Körper haben müsste, um dieselbe Strahlungsleistung abzugeben.<br>{{english}} The effective temperature, or blackbody temperature, of
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