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| author | priyanka | 2015-06-24 15:03:17 +0530 |
|---|---|---|
| committer | priyanka | 2015-06-24 15:03:17 +0530 |
| commit | b1f5c3f8d6671b4331cef1dcebdf63b7a43a3a2b (patch) | |
| tree | ab291cffc65280e58ac82470ba63fbcca7805165 /1958/CH10 | |
| download | Scilab-TBC-Uploads-b1f5c3f8d6671b4331cef1dcebdf63b7a43a3a2b.tar.gz Scilab-TBC-Uploads-b1f5c3f8d6671b4331cef1dcebdf63b7a43a3a2b.tar.bz2 Scilab-TBC-Uploads-b1f5c3f8d6671b4331cef1dcebdf63b7a43a3a2b.zip | |
initial commit / add all books
Diffstat (limited to '1958/CH10')
| -rwxr-xr-x | 1958/CH10/EX10.1/Chapter10_example1.sce | 12 | ||||
| -rwxr-xr-x | 1958/CH10/EX10.2/Chapter10_example2.sce | 12 | ||||
| -rwxr-xr-x | 1958/CH10/EX10.3/Chapter10_example3.sce | 11 | ||||
| -rwxr-xr-x | 1958/CH10/EX10.4/Chapter10_example4.sce | 10 | ||||
| -rwxr-xr-x | 1958/CH10/EX10.5/Chapter10_example5.sce | 13 |
5 files changed, 58 insertions, 0 deletions
diff --git a/1958/CH10/EX10.1/Chapter10_example1.sce b/1958/CH10/EX10.1/Chapter10_example1.sce new file mode 100755 index 000000000..734cfe72b --- /dev/null +++ b/1958/CH10/EX10.1/Chapter10_example1.sce @@ -0,0 +1,12 @@ +clc
+clear
+//Input data
+D=1//Distance of screen from the slit in m
+w=6000//Wavelength in Angstrom
+w1=0.6//Slit width in mm
+
+//Calculations
+x=((2*D*w*10^-10)/(w1*10^-3))*1000//Width of central band in mm
+
+//Output
+printf('Width of central band is %i mm',x)
diff --git a/1958/CH10/EX10.2/Chapter10_example2.sce b/1958/CH10/EX10.2/Chapter10_example2.sce new file mode 100755 index 000000000..45ac6fdfd --- /dev/null +++ b/1958/CH10/EX10.2/Chapter10_example2.sce @@ -0,0 +1,12 @@ +clc
+clear
+//Input data
+d1=6000//Diffraction grating have number of lines per cm
+q=50//Diffracted second order spectral line observed in degrees
+n=2//Second order
+
+//Calculations
+w=(sind(q)/(d1*n))*10^8//Wavelength of radiation in Angstrom
+
+//Output
+printf('Wavelength of radiation is %3.1f Angstrom',w)
diff --git a/1958/CH10/EX10.3/Chapter10_example3.sce b/1958/CH10/EX10.3/Chapter10_example3.sce new file mode 100755 index 000000000..25066cbfc --- /dev/null +++ b/1958/CH10/EX10.3/Chapter10_example3.sce @@ -0,0 +1,11 @@ +clc
+clear
+//Input data
+d1=6000//Diffraction grating have number of lines per cm
+w=6000//Wavelength in Angstrom
+
+//Calculations
+n=(1/(d1*w*10^-8))//Maxmum order of diffraction
+
+//Output
+printf('Maximum order of diffraction that can be observed is %i',n)
diff --git a/1958/CH10/EX10.4/Chapter10_example4.sce b/1958/CH10/EX10.4/Chapter10_example4.sce new file mode 100755 index 000000000..18cc64977 --- /dev/null +++ b/1958/CH10/EX10.4/Chapter10_example4.sce @@ -0,0 +1,10 @@ +clc
+clear
+//Input data
+B=(3*3.14)/2//First secondary maxima at B
+
+//Calculations
+I=(sin(B)/B)^2//Ratio of intensity of central maxima to first secondary maxima
+
+//Output
+printf('Ratio of intensity of central maxima to first secondary maxima is %3.3f',I)
diff --git a/1958/CH10/EX10.5/Chapter10_example5.sce b/1958/CH10/EX10.5/Chapter10_example5.sce new file mode 100755 index 000000000..fad1ceda7 --- /dev/null +++ b/1958/CH10/EX10.5/Chapter10_example5.sce @@ -0,0 +1,13 @@ +clc
+clear
+//Input data
+w=6400//Wave length of light in Angstrom
+w1=0.3//Slit width in mm
+d=110//Distance of screen from the slit in cm
+n=3//order
+
+//Calculations
+x=((n*w*10^-10*(d/100))/(w1*10^-3))*1000//Distance between the centre of the central maximum and the third dark fringe in mm
+
+//Output
+printf('Distance between the centre of the central maximum and the third dark fringe is %3.2f mm',x)
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