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author | Eugeniy E. Mikhailov <evgmik@gmail.com> | 2020-09-17 09:55:22 -0400 |
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committer | Eugeniy E. Mikhailov <evgmik@gmail.com> | 2020-09-17 09:55:22 -0400 |
commit | 4dfcc8bd35c5881988f4b09fa2131448214e5513 (patch) | |
tree | 254dc59de40c4b594750a5f415ac8dd78fbae5ac /blackbody_new.tex | |
parent | 3598bbeb1f11117acb7de81dbab1052ab546d72a (diff) | |
download | manual_for_Experimental_Atomic_Physics-4dfcc8bd35c5881988f4b09fa2131448214e5513.tar.gz manual_for_Experimental_Atomic_Physics-4dfcc8bd35c5881988f4b09fa2131448214e5513.zip |
modified the assignment for black body
Diffstat (limited to 'blackbody_new.tex')
-rw-r--r-- | blackbody_new.tex | 12 |
1 files changed, 11 insertions, 1 deletions
diff --git a/blackbody_new.tex b/blackbody_new.tex index c3bf73d..102a027 100644 --- a/blackbody_new.tex +++ b/blackbody_new.tex @@ -155,7 +155,17 @@ In the lab report plot the reading from the radiation sensor (convert to $W/m^2$ \begin{equation}\label{SBlmod} S =\epsilon\sigma T^4 \end{equation} -where the coefficient $\epsilon$ is called \emph{emissivity} and is defined as the ratio of the energy radiated from a material's surface to that radiated by a perfect blackbody at the same temperature. The values of $\epsilon$ vary from 0 to 1, with one corresponding to an ideal blackbody. All real materials have $\epsilon<1$, although some come quite close to the ideal (for example, carbon black has $\epsilon=0.95$). However, emissivity of a tungsten wire varies from $\epsilon=0.032$ (at $30^{\circ} C$) to $\epsilon=0.35$ (at $3300^{\circ}C$). Using the result of your fit, and assuming we know the Stephan-Boltzman constant $\sigma$ by some other means, what is $\epsilon$ and what is the uncertainty on it? Is it consistent with tungsten? What else could be affecting this measurement? +where the coefficient $\epsilon$ is called \emph{emissivity} and is defined as the ratio of the energy radiated from a material's surface to that radiated by a perfect blackbody at the same temperature. The values of $\epsilon$ vary from 0 to 1, with one corresponding to an ideal blackbody. All real materials have $\epsilon<1$, although some come quite close to the ideal (for example, carbon black has $\epsilon=0.95$). However, emissivity of a tungsten wire varies from $\epsilon=0.032$ (at $30^{\circ} C$) to $\epsilon=0.35$ (at $3300^{\circ}C$). + +Unfortunately, it is impossible to measure the exact value of emissivity +from the experimental data, as one needs to know the surface area of the +filament and the precise distance from it to the detector. However, we +should be able to qualitatively verify the validity of Eq.~(\ref{SBlmod}). From +fitting experimental data, find the proportionality coefficient between the +emitted radiation and the filament temperature $T^4$ and its uncertainty. +Estimate the quality of the linear fit (a linear fit would assume that the +emissivity does not depend on temperature). + Let us examine the quality of the fit more carefully. For that it is convenient to make a separate plot of the \emph{residual} - the difference between the experimental points and the fit values. For a proper fit function, we expect the residuals to be randomly distributed around zero. Analyze your results. Do the points seem to systematically differ from the fit line in a particular region? Can you think of a reason why that would be? |