{ "metadata": { "name": "", "signature": "sha256:fd3a71d11d7e73e323877019a1c5f0e92d8e8b30b7f927fde2bcadd4742b58c1" }, "nbformat": 3, "nbformat_minor": 0, "worksheets": [ { "cells": [ { "cell_type": "heading", "level": 1, "metadata": {}, "source": [ "Chapter 23 Optical instruments" ] }, { "cell_type": "heading", "level": 2, "metadata": {}, "source": [ "Example 23.1 Page no 704" ] }, { "cell_type": "code", "collapsed": false, "input": [ "#Given\n", "f=5.0 #cm\n", "D=25\n", "\n", "#Calculation\n", "M=1+(D/f)\n", "\n", "#Result\n", "print\"Magnifying power is\",M" ], "language": "python", "metadata": {}, "outputs": [ { "output_type": "stream", "stream": "stdout", "text": [ "Magnifying power is 6.0\n" ] } ], "prompt_number": 1 }, { "cell_type": "heading", "level": 2, "metadata": {}, "source": [ "Example 23.2 Page no 704" ] }, { "cell_type": "code", "collapsed": false, "input": [ "#Given\n", "f=6.25 #cm\n", "v=-25\n", "\n", "#Calculation\n", "u=v*f/(v-f)\n", "M=1+(D/f)\n", "M1=D/f\n", "\n", "#Result\n", "print\"(i) The distance of the object from the lens is\", M\n", "print\"(ii) Anguar magnification is\",M1" ], "language": "python", "metadata": {}, "outputs": [ { "output_type": "stream", "stream": "stdout", "text": [ "(i) The distance of the object from the lens is 5.0\n", "(ii) Anguar magnification is 4.0\n" ] } ], "prompt_number": 6 }, { "cell_type": "heading", "level": 2, "metadata": {}, "source": [ "Example 23.3 Page no 704" ] }, { "cell_type": "code", "collapsed": false, "input": [ "#Given\n", "u=-9\n", "f=10 #cm\n", "v1=-25.0\n", "\n", "#Calculation\n", "v=u*f/(u+f)\n", "M=v/u\n", "u=-v1*f/(v1-f)\n", "M1=1-(v1/f)\n", "\n", "#Result\n", "print\"(i) Magnification is\", M,\"\\n Size of each square in the image will appear as 100 mm**2\"\n", "print\"(ii) Magnification is\",M1" ], "language": "python", "metadata": {}, "outputs": [ { "output_type": "stream", "stream": "stdout", "text": [ "(i) Magnification is 10 \n", " Size of each square in the image will appear as 100 mm**2\n", "(ii) Magnification is 3.5\n" ] } ], "prompt_number": 15 }, { "cell_type": "heading", "level": 2, "metadata": {}, "source": [ "Example 23.4 Page no 704" ] }, { "cell_type": "code", "collapsed": false, "input": [ "#Given\n", "v=-25\n", "f=10.0\n", "\n", "#Calculation\n", "u=-v*f/(f-v)\n", "m=-v/u\n", "M=1-(v/f)\n", "\n", "#Result\n", "print\"(a) Distance is\", round(u,2),\"cm\"\n", "print\"(b) Magnification is\",m\n", "print\"(c) Magnification is\",M" ], "language": "python", "metadata": {}, "outputs": [ { "output_type": "stream", "stream": "stdout", "text": [ "(a) Distance is 7.14 cm\n", "(b) Magnification is 3.5\n", "(c) Magnification is 3.5\n" ] } ], "prompt_number": 28 }, { "cell_type": "heading", "level": 2, "metadata": {}, "source": [ "Example 23.5 Page no 705" ] }, { "cell_type": "code", "collapsed": false, "input": [ "#Given\n", "M=-30\n", "fe=5 #cm\n", "D=25 #cm\n", "\n", "#Calculation\n", "m0=M/(1+(D/fe))\n", "\n", "#Result\n", "print\"Magnification produced is\",m0" ], "language": "python", "metadata": {}, "outputs": [ { "output_type": "stream", "stream": "stdout", "text": [ "Magnification produced is -5\n" ] } ], "prompt_number": 29 }, { "cell_type": "heading", "level": 2, "metadata": {}, "source": [ "Example 23.6 Page no 705" ] }, { "cell_type": "code", "collapsed": false, "input": [ "#Given\n", "f0=4\n", "u0=-6\n", "D=25\n", "fe=6.0\n", "\n", "#Calculation\n", "v0=f0*u0/(f0+u0)\n", "M=v0/u0*(1+(D/fe))\n", "\n", "#Result\n", "print\"Magnification produceed by the microscope is\", round(M,2)" ], "language": "python", "metadata": {}, "outputs": [ { "output_type": "stream", "stream": "stdout", "text": [ "Magnification produceed by the microscope is -10.33\n" ] } ], "prompt_number": 34 }, { "cell_type": "heading", "level": 2, "metadata": {}, "source": [ "Example 23.7 Page no 705" ] }, { "cell_type": "code", "collapsed": false, "input": [ "#Given\n", "L=20\n", "fe=5\n", "f0=1.0 \n", "\n", "#Calculation\n", "v01=L-fe\n", "u0=v01*f0/(f0-v01)\n", "M=v01*D/(u0*fe)\n", "\n", "#Result\n", "print\"Magnification power is\", M,\"\\nThe -ve sigh shows that the image formed is inverted and real\"" ], "language": "python", "metadata": {}, "outputs": [ { "output_type": "stream", "stream": "stdout", "text": [ "Magnification power is -70.0 \n", "The -ve sigh shows that the image formed is inverted and real\n" ] } ], "prompt_number": 41 }, { "cell_type": "heading", "level": 2, "metadata": {}, "source": [ "Example 23.8 Page no 705" ] }, { "cell_type": "code", "collapsed": false, "input": [ "#Given\n", "f=36 #cm\n", "M=-8\n", "\n", "#Calculation\n", "fe=-f/(M-1)\n", "f0=-M*fe\n", "\n", "#Result\n", "print\"Focal length of the lenses is\", fe,\"cm and\",f0,\"cm\"" ], "language": "python", "metadata": {}, "outputs": [ { "output_type": "stream", "stream": "stdout", "text": [ "Focal length of the lenses is 4 cm and 32 cm\n" ] } ], "prompt_number": 46 }, { "cell_type": "heading", "level": 2, "metadata": {}, "source": [ "Example 23.9 Page no 705" ] }, { "cell_type": "code", "collapsed": false, "input": [ "#Given\n", "f=75 #cm\n", "fe=5.0\n", "D=25 \n", "\n", "#Calculation\n", "M=-f/fe*(1+(fe/D))\n", "\n", "#Result\n", "print\"Magnying power is\",M" ], "language": "python", "metadata": {}, "outputs": [ { "output_type": "stream", "stream": "stdout", "text": [ "Magnying power is -18.0\n" ] } ], "prompt_number": 49 }, { "cell_type": "heading", "level": 2, "metadata": {}, "source": [ "Example 23.10 Page no 705" ] }, { "cell_type": "code", "collapsed": false, "input": [ "#Given\n", "f0=140\n", "fe=5\n", "D=25.0\n", "\n", "#Calculation\n", "M=-f0/fe\n", "M1=-(f0/fe)*(1+(fe/D))\n", "\n", "#Result\n", "print\"(a) Magnefying power, when telescope is in normal adjustment is\", M\n", "print\"(b) Magnifying power, when image is formed at least distance of distinct vision is is\",M1" ], "language": "python", "metadata": {}, "outputs": [ { "output_type": "stream", "stream": "stdout", "text": [ "(a) Magnefying power, when telescope is in normal adjustment is -28\n", "(b) Magnifying power, when image is formed at least distance of distinct vision is is -33.6\n" ] } ], "prompt_number": 54 }, { "cell_type": "heading", "level": 2, "metadata": {}, "source": [ "Example 23.11 Page no 706" ] }, { "cell_type": "code", "collapsed": false, "input": [ "#Given\n", "f0=1 #m\n", "fe=0.05\n", "I=0.92*10**-2\n", "u0=38*10**-7\n", "fe1=5.0 #cm\n", "ve=-25\n", "\n", "#Calculation\n", "d=I*u0/f0\n", "L=f0+fe\n", "ue=ve*fe1/(fe1-ve)\n", "L1=(f0*10**2)-ue\n", "\n", "#Result\n", "print\"(i) Distance between two lenses is\", L*10**2,\"cm\"\n", "print\"(ii) Distance when final image at 25 cm from the eye is\",round(L1,2),\"cm\"" ], "language": "python", "metadata": {}, "outputs": [ { "output_type": "stream", "stream": "stdout", "text": [ "(i) Distance between two lenses is 105.0 cm\n", "(ii) Distance when final image at 25 cm from the eye is 104.17 cm\n" ] } ], "prompt_number": 71 }, { "cell_type": "heading", "level": 2, "metadata": {}, "source": [ "Example 23.12 Page no 706" ] }, { "cell_type": "code", "collapsed": false, "input": [ "#Given\n", "M=-20\n", "R=120\n", "\n", "#Calculation\n", "f0=R/2.0\n", "fe=-f0/M\n", "\n", "#Result\n", "print\"Focal length of the eye piece is\",fe,\"cm\"" ], "language": "python", "metadata": {}, "outputs": [ { "output_type": "stream", "stream": "stdout", "text": [ "Focal length of the eye piece is 3.0 cm\n" ] } ], "prompt_number": 74 }, { "cell_type": "heading", "level": 2, "metadata": {}, "source": [ "Example 23.13 Page no 706" ] }, { "cell_type": "code", "collapsed": false, "input": [ "#Given\n", "d=0.8 #cm\n", "D=508\n", "\n", "#Calculation\n", "B=D**2/d**2\n", "\n", "#Result\n", "print\"The telescope can see a star \",B,\"time sfarther than the faintest star that can be seen with naked eye.\"" ], "language": "python", "metadata": {}, "outputs": [ { "output_type": "stream", "stream": "stdout", "text": [ "The telescope can see a star 403225.0 time sfarther than the faintest star that can be seen with naked eye.\n" ] } ], "prompt_number": 76 }, { "cell_type": "heading", "level": 2, "metadata": {}, "source": [ "Example 23.14 Page no 706" ] }, { "cell_type": "code", "collapsed": false, "input": [ "#Given\n", "ve=-25 #cm\n", "fe=6.25\n", "a=15\n", "f0=2\n", "\n", "#Calculation\n", "ue=-ve*fe/(ve-fe)\n", "v0=a+ue\n", "u0=f0*v0/(f0-v0)\n", "v01=a-fe\n", "u01=v01*f0/(f0-v01)\n", "\n", "#Result\n", "print\"(a) Distance when final image at least distance of distinct vision is\", u0,\"cm\"\n", "print\"(b) Distance when final image is at infinity is\",round(u01,2),\"cm\"" ], "language": "python", "metadata": {}, "outputs": [ { "output_type": "stream", "stream": "stdout", "text": [ "(a) Distance when final image at least distance of distinct vision is -2.5 cm\n", "(b) Distance when final image is at infinity is -2.59 cm\n" ] } ], "prompt_number": 87 }, { "cell_type": "heading", "level": 2, "metadata": {}, "source": [ "Example 23.15 Page no 707" ] }, { "cell_type": "code", "collapsed": false, "input": [ "#Given\n", "a=10\n", "D=24\n", "fe=20.0\n", "\n", "#Calculation\n", "import math\n", "A=a/(1+(D/fe))/100.0\n", "\n", "#Result\n", "print\"Angle is\", round(A,4),\"radian\"" ], "language": "python", "metadata": {}, "outputs": [ { "output_type": "stream", "stream": "stdout", "text": [ "Angle is 0.0455 radian\n" ] } ], "prompt_number": 95 }, { "cell_type": "heading", "level": 2, "metadata": {}, "source": [ "Example 23.16 Page no 707" ] }, { "cell_type": "code", "collapsed": false, "input": [ "#Given\n", "f0=-0.5 #m\n", "fe=0.01\n", "d=3.48*10**6\n", "r=3.8*10**8\n", "a1=15\n", "\n", "#Calculation\n", "M=f0/fe\n", "a=d/r\n", "I=a*a1\n", "\n", "#Result\n", "print\"(a) Angular Magnification of the telescope is\",M\n", "print\"(b) Diameter of the image is\", round(I,3),\"m\"" ], "language": "python", "metadata": {}, "outputs": [ { "output_type": "stream", "stream": "stdout", "text": [ "(a) Angular Magnification of the telescope is -50.0\n", "(b) Diameter of the image is 0.137 m\n" ] } ], "prompt_number": 103 } ], "metadata": {} } ] }