From 53f72e6790ff23b43c8f6a0b69d6386940671429 Mon Sep 17 00:00:00 2001
From: hardythe1
Date: Wed, 28 Jan 2015 14:31:21 +0530
Subject: added books

---
 Principles_of_physics/chapter10.ipynb | 203 ++++++++++++++++++++++++++++++++++
 1 file changed, 203 insertions(+)
 create mode 100755 Principles_of_physics/chapter10.ipynb

(limited to 'Principles_of_physics/chapter10.ipynb')

diff --git a/Principles_of_physics/chapter10.ipynb b/Principles_of_physics/chapter10.ipynb
new file mode 100755
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--- /dev/null
+++ b/Principles_of_physics/chapter10.ipynb
@@ -0,0 +1,203 @@
+{
+ "metadata": {
+  "name": "",
+  "signature": "sha256:3f76c4dafe83129bfa41f6667339b27d23cec6e550015e787119c4ce10873761"
+ },
+ "nbformat": 3,
+ "nbformat_minor": 0,
+ "worksheets": [
+  {
+   "cells": [
+    {
+     "cell_type": "heading",
+     "level": 1,
+     "metadata": {},
+     "source": [
+      "Chapter 10 Difraction"
+     ]
+    },
+    {
+     "cell_type": "heading",
+     "level": 2,
+     "metadata": {},
+     "source": [
+      "Example 10.1 Page no 154"
+     ]
+    },
+    {
+     "cell_type": "code",
+     "collapsed": false,
+     "input": [
+      "#given\n",
+      "D=1                                   #Distance of screen from the slit in m\n",
+      "w=6000                                #Wavelength in Angstrom\n",
+      "w1=0.6                                #Slit width in mm\n",
+      "\n",
+      "#Calculations\n",
+      "x=((2*D*w*10**-10)/(w1*10**-3))*1000\n",
+      "\n",
+      "#Output\n",
+      "print\"Width of central band is \",x,\"mm\"\n"
+     ],
+     "language": "python",
+     "metadata": {},
+     "outputs": [
+      {
+       "output_type": "stream",
+       "stream": "stdout",
+       "text": [
+        "Width of central band is  2.0 mm\n"
+       ]
+      }
+     ],
+     "prompt_number": 1
+    },
+    {
+     "cell_type": "heading",
+     "level": 2,
+     "metadata": {},
+     "source": [
+      "Example 10.2 Page no 155"
+     ]
+    },
+    {
+     "cell_type": "code",
+     "collapsed": false,
+     "input": [
+      "#given\n",
+      "d1=6000.0                             #Diffraction grating have number of lines per cm\n",
+      "q=50                                  #Diffracted second order spectral line observed in degrees\n",
+      "n=2                                   #Second order\n",
+      "\n",
+      "#Calculations\n",
+      "import math\n",
+      "w=(math.sin(q*3.14/180.0)/(d1*n))*10**8\n",
+      "\n",
+      "#Output\n",
+      "print\"Wavelength of radiation is \",round(w,1),\"Angstrom\"\n"
+     ],
+     "language": "python",
+     "metadata": {},
+     "outputs": [
+      {
+       "output_type": "stream",
+       "stream": "stdout",
+       "text": [
+        "Wavelength of radiation is  6381.3 Angstrom\n"
+       ]
+      }
+     ],
+     "prompt_number": 1
+    },
+    {
+     "cell_type": "heading",
+     "level": 2,
+     "metadata": {},
+     "source": [
+      "Example 10.3 Page no 155"
+     ]
+    },
+    {
+     "cell_type": "code",
+     "collapsed": false,
+     "input": [
+      "#given\n",
+      "d1=6000                      #Diffraction grating have number of lines per cm\n",
+      "w=6000                       #Wavelength in Angstrom\n",
+      "\n",
+      "#Calculations\n",
+      "n=(1/(d1*w*10**-8))\n",
+      "\n",
+      "#Output\n",
+      "print\"Maximum order of diffraction that can be observed is \",round(n,2)\n"
+     ],
+     "language": "python",
+     "metadata": {},
+     "outputs": [
+      {
+       "output_type": "stream",
+       "stream": "stdout",
+       "text": [
+        "Maximum order of diffraction that can be observed is  2.78\n"
+       ]
+      }
+     ],
+     "prompt_number": 5
+    },
+    {
+     "cell_type": "heading",
+     "level": 2,
+     "metadata": {},
+     "source": [
+      "Example 10.4 Page no 155"
+     ]
+    },
+    {
+     "cell_type": "code",
+     "collapsed": false,
+     "input": [
+      "#given\n",
+      "B=(3*3.14)/2                           #First secondary maxima at B\n",
+      "\n",
+      "#Calculations\n",
+      "import math\n",
+      "I=(math.sin(B)/B)**2\n",
+      "\n",
+      "#Output\n",
+      "print\"Ratio of intensity of central maxima to first secondary maxima is \",round(I,3)\n"
+     ],
+     "language": "python",
+     "metadata": {},
+     "outputs": [
+      {
+       "output_type": "stream",
+       "stream": "stdout",
+       "text": [
+        "Ratio of intensity of central maxima to first secondary maxima is  0.045\n"
+       ]
+      }
+     ],
+     "prompt_number": 7
+    },
+    {
+     "cell_type": "heading",
+     "level": 2,
+     "metadata": {},
+     "source": [
+      "Example 10.5 Page no 155"
+     ]
+    },
+    {
+     "cell_type": "code",
+     "collapsed": false,
+     "input": [
+      "#given\n",
+      "w=6400                                        #Wave length of light in Angstrom\n",
+      "w1=0.3                                        #Slit width in mm\n",
+      "d=110                                         #Distance of screen from the slit in cm\n",
+      "n=3                                           #order\n",
+      "\n",
+      "#Calculations\n",
+      "x=((n*w*10**-10*(d/100.0))/(w1*10**-3))*1000\n",
+      "\n",
+      "#Output\n",
+      "print\"Distance between the centre of the central maximum and the third dark fringe is \",x,\"mm\"\n"
+     ],
+     "language": "python",
+     "metadata": {},
+     "outputs": [
+      {
+       "output_type": "stream",
+       "stream": "stdout",
+       "text": [
+        "Distance between the centre of the central maximum and the third dark fringe is  7.04 mm\n"
+       ]
+      }
+     ],
+     "prompt_number": 8
+    }
+   ],
+   "metadata": {}
+  }
+ ]
+}
\ No newline at end of file
-- 
cgit