Difference between revisions of "Blackbody Radiation Mathematica"
(Created page with "Mathematica is an excellent software package to visualize equations. In this activity, you will ultimately reproduce the Figure 1.2 from your textbook (Engle/Reed) showing the...") |
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4) Now use the "Manipulate" function in Mathematica to produce an interactive plot for temperature ranging from 3000 - 4000 K. | 4) Now use the "Manipulate" function in Mathematica to produce an interactive plot for temperature ranging from 3000 - 4000 K. | ||
| − | All of the above graphs are plots of frequency vs. spectral density...can we then do the same as above (1-4) for a function that uses wavelength as opposed to frequency? See | + | All of the above graphs are plots of frequency vs. spectral density...can we then do the same as above (1-4) for a function that uses wavelength as opposed to frequency? See this wiki page: |
https://en.wikipedia.org/wiki/Planck%27s_law | https://en.wikipedia.org/wiki/Planck%27s_law | ||
Revision as of 18:42, 18 January 2018
Mathematica is an excellent software package to visualize equations. In this activity, you will ultimately reproduce the Figure 1.2 from your textbook (Engle/Reed) showing the variation in the frequency output from a blackbody radiator. But first...
1) Plot the frequency vs. spectral density when the blackbody is at 3000 K.
2) Now plot 2 functions (as in part 1) on the same graph for 3000 K and 4000 K.
3) Expand on this plot in part 2 to reproduce Figure 1.2 in your text.
4) Now use the "Manipulate" function in Mathematica to produce an interactive plot for temperature ranging from 3000 - 4000 K.
All of the above graphs are plots of frequency vs. spectral density...can we then do the same as above (1-4) for a function that uses wavelength as opposed to frequency? See this wiki page: https://en.wikipedia.org/wiki/Planck%27s_law