Computes the total energy radiated by a body with given parameters.

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Interface

#include <codecogs/engineering/thermodynamics/radiation/energy.h>

using namespace Engineering::Thermodynamics::Radiation;

This module calculates the total energy radiated by a body per unit surface area in unit time.

The total radiative energy E_0 of a black body is given by the Stefan-Boltzmann law

E_0 = \int_0^{\infty} I(\lambda) {\rm d}\lambda
\qquad \left[\frac{W}{m^2}\right]
(1)

where I(\lambda) is the radiative intensity of the black body.

In practice, the following formula due to Kirchoff is used

E_0 = e c_0 \left(\frac{T}{100}\right)^4
\qquad \left[\frac{W}{m^2}\right]
(2)

where C_0 is the emissivity constant of the black body \displaystyle \left(C_0 \approx 5.669 \left[\frac{W}{m^2 K^4}\right]\right), e is the emissivity factor of the body (0 < e \leq 1) and T is its absolute temperature.

Example 1

The following example calculates the total radiative energy emitted by the Wolfram filament of an incandescent light bulb at 3573.16 degrees Kelvin.

#include <codecogs/engineering/heat_transfer/radiation/energy.h>
#include <stdio.h>

int main()
{
  // the temperature of the Wolfram filament
  double T = 3573.16;

  // emissivity factor of the filament
  double e = 0.39;

  // display the total radiative energy
  printf("Energy = %.5lf kW per sq. meter\n",
  Engineering::Heat_Transfer::Radiation::energy(T, e)/1000.0);

  return 0;
}

Output

Energy = 3603.96794 kW per sq. meter

Parameters

T
the absolute temperature of the body (Kelvin)
e
Default value = 1.0

Returns

the total radiative energy emitted by the body (Watt per square meter)

A table with the emissivity factors of various materials at different temperatures can be found at the following link http://www.monarchserver.com/TableofEmissivity.pdf

References

Dan Stefanescu, Mircea Marinescu - "Termotehnica"

GPL Licence — free for non commercial use. See Licence details.

Interactive Calculator

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