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+{
+ "metadata": {
+ "celltoolbar": "Raw Cell Format",
+ "name": "",
+ "signature": "sha256:257a8f491d964b9b4b60a222b425920b6deeb80bc5dff761617e08199ac997af"
+ },
+ "nbformat": 3,
+ "nbformat_minor": 0,
+ "worksheets": [
+ {
+ "cells": [
+ {
+ "cell_type": "heading",
+ "level": 1,
+ "metadata": {},
+ "source": [
+ "SAMPLE EXAMPLES"
+ ]
+ },
+ {
+ "cell_type": "heading",
+ "level": 2,
+ "metadata": {},
+ "source": [
+ "EXAMPLE NUMBER 1"
+ ]
+ },
+ {
+ "cell_type": "code",
+ "collapsed": false,
+ "input": [
+ "import math\n",
+ "#Given that\n",
+ "D=80# separation between source and screen in cm\n",
+ "d=0.18# separation between sources in cm \n",
+ "n=4# order of fringe\n",
+ "x_n=1.08# distance from central bright fringe in cm \n",
+ "print \"Standard formula used x_n= n*lambda1*D/d \"\n",
+ "\n",
+ "lambda1=d*x_n/(D*n)*1e7\n",
+ "print \"Wavelength of light used is\" ,lambda1, \"Angstrom.\""
+ ],
+ "language": "python",
+ "metadata": {},
+ "outputs": [
+ {
+ "output_type": "stream",
+ "stream": "stdout",
+ "text": [
+ "Standard formula used x_n= n*lambda1*D/d \n",
+ "Wavelength of light used is 6075.0 Angstrom.\n"
+ ]
+ }
+ ],
+ "prompt_number": 7
+ },
+ {
+ "cell_type": "heading",
+ "level": 2,
+ "metadata": {},
+ "source": [
+ "EXAMPLE NUMBER 2"
+ ]
+ },
+ {
+ "cell_type": "code",
+ "collapsed": false,
+ "input": [
+ "import math\n",
+ "#Given that\n",
+ "beta=0.0320#fringe width in cm\n",
+ "D=100# separation between source and screen in cm\n",
+ "d=0.184# separation between sources in cm \n",
+ "print \" Standard formula used beta=lambda1*D/d \"\n",
+ "lambda1=d*beta/D*1e8\n",
+ "print \"Wavelength of light used is\" ,lambda1,\"Angstrom.\""
+ ],
+ "language": "python",
+ "metadata": {},
+ "outputs": [
+ {
+ "output_type": "stream",
+ "stream": "stdout",
+ "text": [
+ " Standard formula used beta=lambda1*D/d \n",
+ "Wavelength of light used is 5888.0 Angstrom.\n"
+ ]
+ }
+ ],
+ "prompt_number": 6
+ },
+ {
+ "cell_type": "heading",
+ "level": 2,
+ "metadata": {},
+ "source": [
+ "EXAMPLE NUMBER 3"
+ ]
+ },
+ {
+ "cell_type": "code",
+ "collapsed": false,
+ "input": [
+ "import math\n",
+ " #Given that\n",
+ "beta=0.02 #fringe width in cm\n",
+ "D=100 # separation between source and screen in cm\n",
+ "u=30 # separation between slit and convex lens in cm\n",
+ "I=0.7 # separation between two images of slits on screen in cm\n",
+ "print\" Standard formula used beta=lambda1*D/d \" \n",
+ "v=100-u\n",
+ "O=I*u/v\n",
+ "d=O\n",
+ "lambda1=d*beta/D*1e8\n",
+ "print\" Wavelength of light used is\",lambda1, \"Angstrom.\""
+ ],
+ "language": "python",
+ "metadata": {},
+ "outputs": [
+ {
+ "output_type": "stream",
+ "stream": "stdout",
+ "text": [
+ " Standard formula used beta=lambda1*D/d \n",
+ " Wavelength of light used is 6000.0 Angstrom.\n"
+ ]
+ }
+ ],
+ "prompt_number": 8
+ },
+ {
+ "cell_type": "heading",
+ "level": 2,
+ "metadata": {},
+ "source": [
+ "EXAMPLE NUMBER 4"
+ ]
+ },
+ {
+ "cell_type": "code",
+ "collapsed": false,
+ "input": [
+ "import math\n",
+ "#Given that\n",
+ "x_n=1.88# fringe separation of nth fringe from central fringe in cm \n",
+ "N=20# order of fringe\n",
+ "beta=0.02#fringe width in cm\n",
+ "D=120# separation between source and eyepiece in cm\n",
+ "d=0.076# separation between sources in cm \n",
+ "print \" Standard formula used beta= lambda1*D/d \"\n",
+ "beta=x_n/N # calculation of angle formed\n",
+ "lambda1=d*beta/D*1e8 # calculation of Wavelength of light\n",
+ "print \" Wavelength of light used is\", round(lambda1,4) , \"Angstrom.\""
+ ],
+ "language": "python",
+ "metadata": {},
+ "outputs": [
+ {
+ "output_type": "stream",
+ "stream": "stdout",
+ "text": [
+ " Standard formula used beta= lambda1*D/d \n",
+ " Wavelength of light used is 5953.3333 Angstrom.\n"
+ ]
+ }
+ ],
+ "prompt_number": 10
+ },
+ {
+ "cell_type": "code",
+ "collapsed": false,
+ "input": [],
+ "language": "python",
+ "metadata": {},
+ "outputs": []
+ }
+ ],
+ "metadata": {}
+ }
+ ]
+} \ No newline at end of file