stefan_boltzmann_law: Calculates the radiant emittance of a body as a function of...

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stefan_boltzmann_lawR Documentation

Calculates the radiant emittance of a body as a function of its temperature

Description

Calculates the radiant emittance of a body as a function of its absolute temperature.

Usage

stefan_boltzmann_law(temp, epsilon = 1)

Arguments

temp

absolute temperature (K)

epsilon

body's emissivity (adimensional between 0 and 1). A value of 1 calculates black body radiant emittance.


jvitorpinto/agmet documentation built on Jan. 30, 2023, 6:33 a.m.