According to Planck's law of black- body radiation, the spectral energy density R as a function...

 

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According to Planck's law of black- body radiation, the spectral energy density R as a function of wavelength (m) and temperature 7 (K) is given by: 2ch 1 R = 15 he/NkT -1 where c=3108 m/s is the speed of light, h=6,626 10-34 J-s is Planck constant, and k=1.3810 23 J/K is Spectral Energy Density (W/m) 5 1013 0.5 T=3,000K --T=4,000K T=5,000K 1 1.5 2 2.5 Wavelength (m) Boltzmann constant. Make the shown figure that contains plots of R as a function of for 0.1A3 m for three temperatures 7=3,000K, T=4,000K, and T=5,000K. Write a script file to make the plot as shown with single plot command and different color for each curve. Use 100 points for the domain. The line styles, axes labels, axes limits, and legend must be the same as that shown in Figure. According to Planck's law of black- body radiation, the spectral energy density R as a function of wavelength (m) and temperature 7 (K) is given by: 2ch 1 R = 15 he/NkT -1 where c=3108 m/s is the speed of light, h=6,626 10-34 J-s is Planck constant, and k=1.3810 23 J/K is Spectral Energy Density (W/m) 5 1013 0.5 T=3,000K --T=4,000K T=5,000K 1 1.5 2 2.5 Wavelength (m) Boltzmann constant. Make the shown figure that contains plots of R as a function of for 0.1A3 m for three temperatures 7=3,000K, T=4,000K, and T=5,000K. Write a script file to make the plot as shown with single plot command and different color for each curve. Use 100 points for the domain. The line styles, axes labels, axes limits, and legend must be the same as that shown in Figure.