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Summary

Description
English: Graph of a function of total emitted energy of a black body proportional to the fourth power of its thermodynamic temperature , according to the Stefan–Boltzmann law. In blue is a total energy according to the Wien approximation, equals .
Date
Source Own work
Author Netheril96

Created with Asymptote. Code:

import graph;
size(400,370,(0,0),(12000,6e8));
usepackage("amsmath,txfonts");
real sigma=5.670400e-8;real a=90/(pi^4);
xaxis("$T/\mathrm{K}$",axis=YZero,0,10000,arrow=EndArrow,ticks=RightTicks(N=5,n=4,beginlabel=false,begin=false,end=false));
yaxis(Label("$j/\mathrm{W\cdot m^{-2}}$",align=N),axis=XZero,0,5.4e8,arrow=EndArrow,ticks=RightTicks,autorotate=false);
real j1(real T){return sigma*(T^4);};
real j2(real T){return a*j1(T);};

draw(graph(j1,0,10000));
draw(graph(j2,0,10000),lightblue);

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Taste's greatness in words

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4 July 2011

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Date/TimeThumbnailDimensionsUserComment
current13:07, 4 July 2011Thumbnail for version as of 13:07, 4 July 2011606 × 603 (60 KB)Netheril96{{Information |Description ={{en|1=Graph of a function of total emitted energy of a black body <math>j^{\star}</math> proportional to the fourth power of its thermodynamic temeprature <math>T</math>, according to the Stefan–Boltzmann law. In blue is

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