{ "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": {} } ] }