From b1f5c3f8d6671b4331cef1dcebdf63b7a43a3a2b Mon Sep 17 00:00:00 2001
From: priyanka
Date: Wed, 24 Jun 2015 15:03:17 +0530
Subject: initial commit / add all books

---
 1958/CH10/EX10.1/Chapter10_example1.sce | 12 ++++++++++++
 1958/CH10/EX10.2/Chapter10_example2.sce | 12 ++++++++++++
 1958/CH10/EX10.3/Chapter10_example3.sce | 11 +++++++++++
 1958/CH10/EX10.4/Chapter10_example4.sce | 10 ++++++++++
 1958/CH10/EX10.5/Chapter10_example5.sce | 13 +++++++++++++
 5 files changed, 58 insertions(+)
 create mode 100755 1958/CH10/EX10.1/Chapter10_example1.sce
 create mode 100755 1958/CH10/EX10.2/Chapter10_example2.sce
 create mode 100755 1958/CH10/EX10.3/Chapter10_example3.sce
 create mode 100755 1958/CH10/EX10.4/Chapter10_example4.sce
 create mode 100755 1958/CH10/EX10.5/Chapter10_example5.sce

(limited to '1958/CH10')

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)
-- 
cgit