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| author | Christian Kolset <christian.kolset@gmail.com> | 2025-11-17 09:24:55 -0700 |
|---|---|---|
| committer | Christian Kolset <christian.kolset@gmail.com> | 2025-11-17 10:27:54 -0700 |
| commit | d78171c31310f73a1b189e0946b744accdfb4850 (patch) | |
| tree | 5ad8286ff08ec61869ec8e918e844d8df4456c81 /tutorials/module_4/Spectroscopy problem.md | |
| parent | 8f81b92b4942879edb32f9420514b7e402144a44 (diff) | |
Updated meeting notes, fixed typo in scpectroscopy problem and changed integration method to simpson.
Ammended meeting note commit.
Diffstat (limited to 'tutorials/module_4/Spectroscopy problem.md')
| -rw-r--r-- | tutorials/module_4/Spectroscopy problem.md | 4 |
1 files changed, 1 insertions, 3 deletions
diff --git a/tutorials/module_4/Spectroscopy problem.md b/tutorials/module_4/Spectroscopy problem.md index 5252d46..29d26f5 100644 --- a/tutorials/module_4/Spectroscopy problem.md +++ b/tutorials/module_4/Spectroscopy problem.md @@ -99,7 +99,7 @@ Calibrate wavelength by converting the length dimension from pixels to nm. $$ \lambda_p=I+C_1p+C_2p^2+C_3p^3 $$ -- Solve for C1 C2 and C3, use $I=195.54$ +- Solve for C1, C2 and C3, use $I=195.54$ Well-known/defined Hg lines: @@ -154,5 +154,3 @@ $$ $$ n_{1,2}=\frac{\int_{\lambda_0-\Delta\lambda}^{\lambda_0+\Delta\lambda} I(\lambda)d\lambda}{\frac{1}{4\pi}hv_{1,2}A_{1,2}l}\tag{1} $$ - -|
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