Exercise
https://texercises.raemilab.ch/exercise/heat-radiation-from-the-earth/
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The following quantities appear in the problem: Temperatur \(T\) / Leistung \(P, \Phi\) / Fläche \(A\) / Radius \(r\) / Oberfläche \(S\) /
The following formulas must be used to solve the exercise: \(S = 4 \pi r^2 \quad \) \(\Phi = \epsilon\sigma A T^4 \quad \)
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Exercise:
The mean surface temperature of the Earth rO radius is TO. Calculate the total radiant power emitted by the Earth asing it behaves as a perfect blackbody.

Solution:
al Phi PF ncS qtyTQ^ A P approx PS
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Exercise:
The mean surface temperature of the Earth rO radius is TO. Calculate the total radiant power emitted by the Earth asing it behaves as a perfect blackbody.

Solution:
al Phi PF ncS qtyTQ^ A P approx PS
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Heat Transfer
Tags
erde, kugel, kugeloberfläche, physik, stefan-boltzmann-gesetz, thermodynamik, wärmelehre, wärmestrahlung
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(2, default)
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2 (default)
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ENG (English)
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Calculative / Quantity
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