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authorEugeniy Mikhailov <evgmik@gmail.com>2014-09-26 09:48:34 -0400
committerEugeniy Mikhailov <evgmik@gmail.com>2014-09-26 09:48:34 -0400
commitb8a81f6487f34e682b1dc7517ef18fa97178fec6 (patch)
tree653009044bca6c39063e6e8230fd324af89c489c
parenta88626c3ab25c99f5efe57d146ff2858123e30d2 (diff)
downloadmanual_for_Experimental_Atomic_Physics-b8a81f6487f34e682b1dc7517ef18fa97178fec6.tar.gz
manual_for_Experimental_Atomic_Physics-b8a81f6487f34e682b1dc7517ef18fa97178fec6.zip
typo fixed, thanks Kevin and Calvin
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\begin{enumerate}
\item
-Use the table in Fig.~\ref{fig:mercury_spectrum} to find the exact frequencies and wavelengths of the spectral lines you used and plot the measured stopping potential values versus light frequency for of measurements of the first and second order lines (can be on same graph).
+Use the table in Fig.~\ref{fig:mercury_spectrum} to find the exact frequencies and wavelengths of the spectral lines you used and plot the measured stopping potential values versus light frequency for measurements of the first and second order lines (can be on same graph).
\item Fit the plots according to $eV_0 = h\nu-\phi$, extracting values for slopes and intercepts. Find the average value for slope and its uncertainty. From the slope, determine $h$ counting $e=1.6\cdot10^{-19}$~C. Do your measured values agree with the accepted value of $h=2\pi\cdot 10^{-34}$J$\cdot$s within experimental uncertainty?