PHYSICAL OPTICS
Excel Documentation
Excel Tables



(Frefl1.xls)

By using the electromagnetic approach of propagation of light at an interface, a relationship between the electric field and magnetic field of the incident, reflected, and refracted light can be obtained. These relationships are obtained by using the continuity of the wave at the boundary. Interpretation of the wave in a linear, isotropic, and homogenous media leads to the determination of amplitude, reflection, and transmission coefficents. These coefficients are different for different polarization of the wave. The spreadsheet program shows the variation of the coefficients at an air-glass interface. Animation of the reflection coefficients for different refractive indicies is used to show the variation of the Brewster angle.
1. Using a spreadsheet, show how the reflection and transmission coefficients change when light passes form glass to air.
2. Using the spread sheet determine the Brewster angle when light passes from glass to air.
Going Further:
3. Create an animation that shows the change in the reflection coefficients due to different indicies of refraction.


Reflection and transmission coefficients at an interface

 

 

 

 

 

 

 

 

Air-Glass Interface

 

 

 

 

 

 

 

 

 

 

n1 =

1

n2 =

1.5

 

 

 

Pi =

3.1415927

 

 

 

 

 

 

 

 

 

 

R (Per)

T(Per)

R(Par)

T(Par)

1

0.0174533

0.0400162

0.9599838

0.0399838

0.9600162

4

0.0698132

0.0402608

0.9597392

0.03974

0.96026

7

0.122173

0.0408044

0.9591956

0.039203

0.960797

10

0.1745329

0.0416595

0.9583405

0.0383715

0.9616285

13

0.2268928

0.0428462

0.9571538

0.0372437

0.9627563

16

0.2792527

0.0443927

0.9556073

0.035818

0.964182

19

0.3316126

0.0463366

0.9536634

0.034093

0.965907

22

0.3839724

0.0487264

0.9512736

0.0320691

0.9679309

25

0.4363323

0.0516235

0.9483765

0.0297493

0.9702507

28

0.4886922

0.0551046

0.9448954

0.0271412

0.9728588

31

0.5410521

0.0592653

0.9407347

0.0242594

0.9757406

34

0.5934119

0.0642241

0.9357759

0.0211292

0.9788708

37

0.6457718

0.0701276

0.9298724

0.0177915

0.9822085

40

0.6981317

0.0771577

0.9228423

0.0143095

0.9856905

43

0.7504916

0.0855395

0.9144605

0.0107792

0.9892208

46

0.8028515

0.0955518

0.9044482

0.0073425

0.9926575

49

0.8552113

0.1075411

0.8924589

0.004207

0.995793

52

0.9075712

0.1219371

0.8780629

0.0016741

0.9983259

55

0.9599311

0.1392735

0.8607265

0.0001778

0.9998222

58

1.012291

0.1602126

0.8397874

0.0003422

0.9996578

61

1.0646508

0.1855756

0.8144244

0.0030623

0.9969377

64

1.1170107

0.216378

0.783622

0.0096236

0.9903764

67

1.1693706

0.253872

0.746128

0.0218757

0.9781243

70

1.2217305

0.2995947

0.7004053

0.0424904

0.9575096

73

1.2740904

0.3554213

0.6445787

0.0753494

0.9246506

76

1.3264502

0.4236234

0.5763766

0.126135

0.873865

79

1.3788101

0.5069272

0.4930728

0.2032463

0.7967537

82

1.43117

0.6085697

0.3914303

0.3192525

0.6807475

85

1.4835299

0.7323455

0.2676545

0.4932538

0.5067462

88

1.5358897

0.8826381

0.1173619

0.754831

0.245169

89

1.553343

0.9394722

0.0605278

0.8688977

0.1311023

90

1.5707963

1

-7.338E-10

1

-1.651E-09

 

Identifying Brewster's angle

 

 

 

 

 

 

 

48

0.837758

0.1033004

0.8966996

0.0052024

0.9947976

49

0.8552113

0.1075411

0.8924589

0.004207

0.995793

50

0.8726646

0.1120484

0.8879516

0.0032775

0.9967225

51

0.8901179

0.1168405

0.8831595

0.0024279

0.9975721

52

0.9075712

0.1219371

0.8780629

0.0016741

0.9983259

53

0.9250245

0.1273594

0.8726406

0.0010339

0.9989661

54

0.9424778

0.13313

0.86687

0.0005276

0.9994724

55

0.9599311

0.1392735

0.8607265

0.0001778

0.9998222

56

0.9773844

0.1458159

0.8541841

1.044E-05

0.9999896

57

0.9948377

0.1527856

0.8472144

5.433E-05

0.9999457

58

1.012291

0.1602126

0.8397874

0.0003422

0.9996578

59

1.0297443

0.1681296

0.8318704

0.0009109

0.9990891

60

1.0471976

0.1765715

0.8234285

0.0018019

0.9981981

61

1.0646508

0.1855756

0.8144244

0.0030623

0.9969377

 

The cells below are for a slide show which demonstrates the effects of a changing index of refraction.

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

1.3

1.35

1.4

1.45

1.5

1.55

1.6

1.65

1.7

1.75

1.8

 

 

 

 

 

 

 

 

 

 

 

 

 

45

0.7853982

0.0020755

0.0032348

0.004688

0.0064341

0.0084665

0.0107746

0.0133454

0.0161642

0.0192155

0.0224832

0.0259515

46

0.8028515

0.0016305

0.0026349

0.0039212

0.0054917

0.0073425

0.0094654

0.011849

0.0144803

0.0173449

0.0204276

0.0237135

47

0.8203047

0.0012204

0.0020712

0.0031904

0.0045841

0.0062512

0.008186

0.010379

0.0128188

0.0154921

0.0183851

0.0214835

48

0.837758

0.0008531

0.001552

0.0025047

0.0037208

0.0052024

0.0069464

0.0089454

0.0111896

0.0136674

0.0163658

0.0192715

49

0.8552113

0.0005375

0.0010872

0.0018743

0.0029124

0.004207

0.0057578

0.0075596

0.0096044

0.011882

0.014381

0.0170887

50

0.8726646

0.0002837

0.0006877

0.0013108

0.002171

0.0032775

0.0046328

0.0062343

0.0080759

0.0101491

0.0124436

0.014948

51

0.8901179

0.0001035

0.000366

0.0008274

0.0015103

0.0024279

0.0035858

0.004984

0.0066187

0.008483

0.0105682

0.0128639

52

0.9075712

9.892E-06

0.0001363

0.000439

0.0009458

0.0016741

0.0026329

0.0038251

0.0052492

0.0069003

0.0087711

0.0108527

53

0.9250245

1.81E-05

1.47E-05

0.0001625

0.000495

0.0010339

0.0017922

0.0027759

0.003986

0.0054195

0.007071

0.0089328

54

0.9424778

0.0001452

1.948E-05

1.706E-05

0.0001775

0.0005276

0.0010843

0.0018572

0.0028498

0.0040615

0.0054885

0.007125

55

0.9599311

0.0004108

0.0001714

2.425E-05

1.562E-05

0.0001778

0.0005324

0.0010922

0.0018641

0.0028497

0.0040473

0.0054526

56

0.9773844

0.000837

0.0004939

0.0002086

3.462E-05

1.044E-05

0.0001624

0.0005074

0.0010553

0.0018106

0.0027738

0.0039421

57

0.9948377

0.0014492

0.0010137

0.0005977

0.0002629

5.433E-05

3.646E-06

0.0001322

0.0004532

0.0009742

0.0016977

0.0026231

58

1.012291

0.0022762

0.0017611

0.001223

0.0007326

0.0003422

8.933E-05

4.058E-09

9.137E-05

0.0003738

0.0008527

0.0015293

59

1.0297443

0.0033508

0.0027704

0.0021198

0.0014799

0.0009109

0.0004567

0.0001485

7.478E-06

4.751E-05

0.0002766

0.0006983

60

1.0471976

0.0047104

0.0040807

0.0033284

0.0025458

0.0018019

0.0011477

0.0006198

0.0002441

3.778E-05

1.197E-05

0.0001727

61

1.0646508

0.0063975

0.0057359

0.0048941

0.0039766

0.0030623

0.0022098

0.0014618

0.000849

0.0003927

0.000107

6.037E-07

62

1.0821041

0.0084607

0.0077865

0.0068683

0.0058246

0.004745

0.0036964

0.0027282

0.0018764

0.0011664

0.0006158

0.0002362

63

1.0995574

0.0109551

0.0102893

0.0093092

0.0081487

0.0069096

0.0056677

0.0044796

0.003387

0.0024199

0.0015995

0.0009405

64

1.1170107

0.0139439

0.013309

0.0122826

0.011016

0.0096236

0.0081917

0.0067844

0.0054496

0.0042221

0.0031272

0.0021827

65

1.134464

0.0174987

0.0169192

0.0158633

0.0145017

0.0129634

0.0113452

0.0097198

0.0081416

0.0066507

0.0052768

0.0040409


(Sphmir.xls)

Mirrors can be one of the simplest optical tools that we use every day but they can also be the msot complicted tools. A common example is a plane mirror, where as the side mirrors in an automobile are more complex. These are mirrors used in the headlight of a car which are carefully designed. The shape of the mirror and its size dictate the specific application of the mirror. The maple/mathematica exercises allow the students to experience in a simple way one of the problems in the imaging property of spherical and parabolic mirrors. The abberation the students will learn about is spherical abberation.

Exercises:
1. How far away do two rays, one close to the optical axis (paraxial ray) and the other, at quite a distance from the optic axis (marginal ray), that are parallel to the optical axis, intersect the optical axis for a spherical mirror.
2. What happens if the mirror is parabolic in shape?


     
 

Reflection from a spherical mirror

Radius of curvature 'R'

Distance from the optic axis 'y'

Angle of reflection is theta

x' indicates variation in focal length

 

 

 

 

 

 

 

 

y

R

DC

R'

q

q1

Dq

x'

0

100

0

100

0

1.5707963

1.5707963

0

1.5

100

0.0112506

99.988749

0.0150023

1.5557941

1.5407918

49.977496

3

100

0.0450101

99.95499

0.030018

1.5407783

1.5107603

49.909939

4.5

100

0.1013013

99.898699

0.0450609

1.5257354

1.4806746

49.797192

6

100

0.1801623

99.819838

0.0601445

1.5106518

1.4505072

49.639023

7.5

100

0.2816466

99.718353

0.0752829

1.4955134

1.4202305

49.435109

9

100

0.4058235

99.594177

0.0904902

1.4803062

1.389816

49.185025

10.5

100

0.5527778

99.447222

0.1057808

1.4650155

1.3592347

48.888247

12

100

0.7226108

99.277389

0.1211697

1.4496266

1.3284569

48.544143

13.5

100

0.9154402

99.08456

0.1366724

1.434124

1.2974516

48.151966

15

100

1.1314003

98.8686

0.1523047

1.4184917

1.266187

47.710851

16.5

100

1.3706433

98.629357

0.1680833

1.402713

1.2346297

47.219802

18

100

1.633339

98.366661

0.1840258

1.3867706

1.2027448

46.677685

19.5

100

1.9196758

98.080324

0.2001503

1.370646

1.1704957

46.08321

21

100

2.2298614

97.770139

0.2164763

1.35432

1.1378437

45.434924

22.5

100

2.5641237

97.435876

0.2330243

1.3377721

1.1047478

44.731186

24

100

2.9227112

97.077289

0.249816

1.3209803

1.0711643

43.970153

25.5

100

3.3058947

96.694105

0.2668749

1.3039214

1.0370465

43.149749

27

100

3.7139678

96.286032

0.2842259

1.2865704

1.0023445

42.267644

28.5

100

4.1472483

95.852752

0.3018961

1.2689003

0.9670042

41.321216

30

100

4.6060799

95.39392

0.3199146

1.2508818

0.9309672

40.307507

31.5

100

5.0908329

94.909167

0.3383131

1.2324832

0.8941701

39.223182

33

100

5.6019068

94.398093

0.3571263

1.21367

0.8565436

38.064463

34.5

100

6.1397315

93.860268

0.3763922

1.1944041

0.8180118

36.827063

36

100

6.7047697

93.29523

0.3961526

1.1746437

0.778491

35.506091

37.5

100

7.2975189

92.702481

0.4164538

1.1543425

0.7378887

34.095952

39

100

7.9185143

92.081486

0.4373473

1.1334491

0.6961018

32.590207

40.5

100

8.5683315

91.431668

0.4588906

1.1119057

0.6530151

30.981405

42

100

9.2475896

90.75241

0.4811485

1.0896478

0.6084992

29.260868

43.5

100

9.9569547

90.043045

0.5041944

1.0666019

0.5624075

27.418413

45

100

10.697145

89.302855

0.5281118

1.0426846

0.5145728

25.441996

46.5

100

11.468932

88.531068

0.5529964

1.0178

0.4648036

23.317232

48

100

12.273151

87.726849

0.578959

0.9918373

0.4128783

21.02676

49.5

100

13.110703

86.889297

0.6061291

0.9646672

0.3585381

18.549369

51

100

13.98256

86.01744

0.6346591

0.9361372

0.3014782

15.858786

52.5

100

14.889777

85.110223

0.6647307

0.9060657

0.241335

12.921935

54

100

15.833498

84.166502

0.6965634

0.8742329

0.1776696

9.696399

55.5

100

16.814965

83.185035

0.7304264

0.8403699

0.1099435

6.126571

57

100

17.835531

82.164469

0.7666558

0.8041405

0.0374847

2.1376296

58.5

100

18.896671

81.103329

0.8056804

0.7651159

-0.0405645

-2.374326

60

100

20

80

0.8480621

0.7227342

-0.1253278

-7.5592895


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