From d78171c31310f73a1b189e0946b744accdfb4850 Mon Sep 17 00:00:00 2001 From: Christian Kolset Date: Mon, 17 Nov 2025 09:24:55 -0700 Subject: Updated meeting notes, fixed typo in scpectroscopy problem and changed integration method to simpson. Ammended meeting note commit. --- tutorials/module_4/Spectroscopy problem.md | 4 +--- 1 file changed, 1 insertion(+), 3 deletions(-) (limited to 'tutorials/module_4/Spectroscopy problem.md') 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} $$ - -| \ No newline at end of file -- cgit v1.2.3