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author | priyanka | 2015-06-24 15:03:17 +0530 |
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committer | priyanka | 2015-06-24 15:03:17 +0530 |
commit | b1f5c3f8d6671b4331cef1dcebdf63b7a43a3a2b (patch) | |
tree | ab291cffc65280e58ac82470ba63fbcca7805165 /1271/CH2/EX2.36/example2_36.sce | |
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-rwxr-xr-x | 1271/CH2/EX2.36/example2_36.sce | 10 |
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diff --git a/1271/CH2/EX2.36/example2_36.sce b/1271/CH2/EX2.36/example2_36.sce new file mode 100755 index 000000000..7c102fb46 --- /dev/null +++ b/1271/CH2/EX2.36/example2_36.sce @@ -0,0 +1,10 @@ +clc +// Given that +N = 400000 // no. of lines in grating per meter +lambda = 5e-7 // wavelength of incident radiation in meter +n = 3 // no. of order +// Sample Problem 36 on page no. 2.52 +printf("\n # PROBLEM 36 # \n") +p = (n * N) / (sqrt(1 - (N * n * lambda)))// dispersive power (p) = d(theta)/d(lambda) +printf("\n Standard formula used \n p = (n * N) / (sqrt(1 - (N * n * lambda))). \n") +printf("\n Dispersive power = %e rad/m",p) |