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UNCLASSIFIED AD NUMBER AD363641 CLASSIFICATION CHANGES TO: unclassified FROM: secret LIMITATION CHANGES TO: Approved for public release, distribution unlimited FROM: Distribution: Further dissemination only as directed by Defense Atomic Support Agency, Washington, DC 20301, JUL 1954, or higher DoD authority. AUTHORITY DNA ltr, 21 Dec 1984; DNA ltr, 21 Dec 1984 THIS PAGE IS UNCLASSIFIED

UNCLASSIFIED AD NUMBER CLASSIFICATION CHANGES · 12.3 Teletronic Image, Mike Shot 56 APPENDIX A BLOCK DIAGRAMS OF PHOTOSTATIONS A.1 Photographic Installation, Janet, Mike Shot 61

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Page 1: UNCLASSIFIED AD NUMBER CLASSIFICATION CHANGES · 12.3 Teletronic Image, Mike Shot 56 APPENDIX A BLOCK DIAGRAMS OF PHOTOSTATIONS A.1 Photographic Installation, Janet, Mike Shot 61

UNCLASSIFIED

AD NUMBER

AD363641

CLASSIFICATION CHANGES

TO: unclassified

FROM: secret

LIMITATION CHANGES

TO:Approved for public release, distributionunlimited

FROM:

Distribution: Further dissemination onlyas directed by Defense Atomic SupportAgency, Washington, DC 20301, JUL 1954, orhigher DoD authority.

AUTHORITYDNA ltr, 21 Dec 1984; DNA ltr, 21 Dec 1984

THIS PAGE IS UNCLASSIFIED

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WT7639

Copy No. A

IVY~~~ cv T71

November 1952

TECHNICAL PHOTOGRAPHY

__ RESTRICTED DATAThis document contains restricted data as

_______defined in the Atomic Energy Act of 1954._________Its transmittal or the disclosure of its

______________contents in any manner to an unauthorized

person is prohibited.

JOINT TASK FORCE 132 1

DODCL SECRETI

=bdovqanqcddccxcuded from MutOwatid A

IoynL

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SECRET __"@ •-1639 \,

This document consists of 101 pages

No. 1 5 3 of 200 copies, Series A

Report to the Scientific Director

&•- TECHNICAL PHOTOGRAPHY •IL "

By

Staff of

Edgerton, Germeshausen & Grier, Inc.

ALL DTR, BTN OF THIS REPORT IS CONTROLLED. QUALM .,,

UsERS SHALL REQUEST THROUG1n \ ik..

Defense Atomc support' Washing•ton, D. C. 20301

Edgerton, Germeshausen GrierBoston, MasstI

RESTRICTED DATA kThis document contains restricted data as de-fined in the Atomic Energy Act of 1954. Itstransmittal or the disclosure of its contents inany manner to an unauthorized person is pro- .hibited.

SECRETI~Ewldt ommcntomatioI

ldvwurdiitq anddeclrawilicadon~

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GSH 4

A Alice BogalluaB Belle BogombogoC Clara Ruchi ovD Daisy Cochiti iWE Edna Sani ldefonsoF Flora ElugelabG Gene TeiteiripucchiH Helen BogairikkI Irene BogonJ Janet EngebiK Kate MuzinbaarikkuNL Lucy KirinianM Mary BokonaarappuN Nancy Yeiri ,iZO Olive Aitsu AA Alvin Chinieero %.P Pearl Rujoru BB Bruce Aniyaanii It IR Ruby Eberiru CC Clyde Chinimi \4AAS Sally Aomon DD David Japtan 4T Tilda Biijiri EE Elmer ParryBBU Ursula Rojoa FF Fred EniwetokV Vera Aaraanbiru GG Glenn Igurin ICCW Wilma Piiraai HH Henry MuiY Yvonme Runit II Irwin PokonZ Zona Site M JJ James Ribaion

fLL KK Keith GiriinienV LL LeRoy Rigili fEE

I

"J(K,JJ

"• HH'•-, GG

ENIWETOK ATOLL

2

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ASTRACT

Edgarl= Ge&i-es- " m.I , n.aa=y 'om the folling photograr .ic activities on Operation Ivy. , .re ' oti" -

ý 11 Determine fireball yield from high-speed cameras and Rapatronics. .,S2.` Record cloud-rise and -drift phenomena.

,3. Determine luminous emittance of the fireball.-4.4 Ietermine time to the minimum by means of Bhangmeters •

D•. Determine position of burst for King shot.Q6. Record mortar and gun bursts for J-10.---':7i Record water wave from Mike shot.,8i Record smoke rocket trails on King s

9: iRecord the television monitor sc n on-kike shot from M- I hr to zero time.,10. In addition, -E r perated experimental GMX-9 camera, an experimenta'Tele-

scopic Rapatronic camera, and image-converter camera. . -

Fireball yield was de r'mined to be 10,900 ± 500 KT for mE 5 KT forKing shot.,

The Mike c d reached a maximum height of slightly over 100,000 ft in about 4 min, atwhich time. e diameter had become about 100,000 ft. At the end of 1 hr the cloud ha( spreadout oa range of 300,000 ft. The King cloud attained its maximum height of 65,000 ft inAI.ghtly over 4 min, while growing to a 40,000-ft diameter

Bhangmeter records on Mike shot were not adequate -,termine tne time to the minimum.King Bhangmeters gave an average time to the minimum of 6 s'ec, which is scaled to a yieldof 440 ± 90 KT.

King position of bursc with respect to the Coral Survey Statioif (N 100,000, E 100,000) wasdetermined to be

N 108,450 ± 30, an error of 300' NE 123,650 ±: 20, an error of 480' WHeight, 1480 ± 20 ft above sea level

This position corresponds to latitude N 11033144" and longitude E 162021,09".The disposition of the film prints is outlined in Appendix B.

3-4

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a

CONTENTSPage

ABSTRACT 3

CHAPTER 1 INTRODUCTION 9

CHAPTER 2 FILM HANDLING . . . . . . 14

CHAPTER 3 PROJECT 3.1: FIREBALL YIELD DETERMINATION . . . 16

3.1 Procedures . . . . . . . . . . . 163.1.1 Mike Shot I . . . . . . . . . 16

3.1.2 King Shot . . . . . . . . . . . 18

3.2 Camera, and Exposures . . . . . . . . 183.2.1 Mike Shot . . .. 183.2.2 King Shot 18

3.3 Fireball Diameter-Time Characteristics 20

3.4 Fireball Scaling 21

3.4.1 Mike Shot . . 26

3.4.2 King Shot 29

CHAPTER 4 PROJECT 3.2: CLOUD RISE 30

4.1 Mike Shot . 304.2 King Shot . 314.3 Results 31

CHP.A--r ER 5 PROJECT 3.5; LUMINOUS EMITTANCE VS TIMAE 38

CHAPTER 6 PROJECT 3.6: BiHANGMETERS, MODII 39

CHAPTER 7 PROJECT 3.8: POSITION OF BURST 42

CHAPTER 8 PROJ-ECT 6.2: MORTAUR AND GUN BURST 44

CHAPTER 9 PROJECT 6.4a: WATER-WAVE PHOTOGRAPHY 47

CHAPTER 10 PROJECT 6.14: ROCKET PHOTOGRAPHY 48

CHAPTER 1I PROJECT 10.1: TELEVISION AND WORLD TIM4, 49

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CONTENTS (Continued) Page

CHAPTER 12 MISCELLANEOUS . . . . . . . . . . 53

12.1 GMX-9 Model 7 Camera . . . . . . . . 5312.% Image-converter Camera I . . . . . . . . 5312.3 Teletronic Camera . . . . . . 57

APPENDIX A BLOCK DIAGRAMS OF PHOTOSTATIONS . . . . 59

APPENDIX B FILM COMPOSITION AND DISPOSITION . . . . . . 67

APPENDIX C METEOROLOGICAL DATA . . . . . . . . 69

APPENDIX D CAMERA DATA SHEETS . . . . . . . . 71

ILLUSTRATIONS

CHAPTER 1 INTRODUCTION

1.1 Elmer Phototower, Station 301 . . . . . . . . 10

1.2 Camera Installation, Station 301 . . . . . . . . 11

1.3 Map of Photostations .. . . . . . . . . 121.4 Typical Shielded-camera Installation 13

CHAPTER 2 FILM HANDLING

2.1 Hauser Profile Measuring Microscope 15

CHAPTER 3 PROJECT 3.1: FIREBALL YIELD DETERMINATION

3.1 Shielded-yield-camera Installation . 173.2 Fireball Diameter Vs Time, Mike Shot 223.3 Fireball Diameter Vs Time, King Shot 233.4 4 Vs Time, Mike Shot 243.5 0 Vs Time, King Shot 27

CHAPTER 4 PROJECT 3.2: CLOUD RISE

4.1 Sketch of Cloud Form on Mike Shot 324.2 Diameter and Height of Mike Cloud As a Function of Time 34.3 Mike Cloud, 1 Min, 40 Sec . 344.4 Diameter and Height of King Cloud As a Function of Time 354.5 King Cloud, 3 Min, 20 Sec . 36

CHAPTER 6 PROJECT 3.6: BHANGMETERS, MOD II

6.1 Bhangmeter Records, Mike and King Shots 406.2 Calibration Curve, Time t j M inimum Vs Yield . 41

CHAPTER 7 PROJECT 3.8: POSITON OF BURST

S7.1 Theo'lote-eamera Locations, King Shot 43

6

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ILLUSTRATIONS (Continued)Page

CHAPTER A PROJECT 6.?: MORTAR AND GUN BURST

8.1 Mortar-photography Camera Stations 4.

8.2 Camera Fields of View, Gun-burst Photography 46

CHAPTER 11 PROJECT 10.1: TELEVISION AN15 WORLD TIME

11.1 Data Monitoring Panel with Television Monitoring Record,Mike Shot 50

11.2 World-time Photography Installatioi 5111.3 World-time Records, Mike Shot 52

CHAPTER 12 MISCELLANEOUS

12.1 GMX-camera Record, Mike Shot 5412.2 Image-converter-camera Installation 5512.3 Teletronic Image, Mike Shot 56

APPENDIX A BLOCK DIAGRAMS OF PHOTOSTATIONS

A.1 Photographic Installation, Janet, Mike Shot 61A.2 Photographic Installation, Yvonne, Mike Shot 62A.3 Photographic Installation, Elmer Tower, Mike and King Shots 63A.4 Photographic Installation, Elmer Ground, Mike and King Shots 64A.5 Photographic Installation, Elmer CP, Mike and King Shots 65A.6 Photographic installation, Ursula, Mike and King Shots . 66

TABLES

CHAPTER 3 PROJECT 3.1: FIREBALL YIELD DETERMINATION

3.1 Summary of Eastman Operation, Mike Shot 183.2 Summary of Rapatronic Operation, Mike Shot 19

3.3 Summary of Eastman Operation, King Shot 193.4 Summary of Rapatronic Operation, King Shot 203.5 Fireball Diameter As a Function of Time, Mike Shot 253.6 Fireball Diameter As a Function of Time from Rapatronics,

Mike Shot . 253.7 Fireball Diameter As a Function of Time, King Shot. 253.8 Fireball Diameter As a Function of Time from Rapatronics,

King Shot . 253.9 0 As a Function of Time, Mike Shot . 253.10 4, As a Function of Time from Rapatronics, Mike Shot 253.11 Statistical Analysis of Mike Fireball Data. . 28

3.12 4) As a Function of Time, King Shot 283.13 (A As a Function of Time from Rapatronics, King Shot 283.14 Statistical Analysis of King Fireball Data . 28

CHAPTER 4 PROJECT 3.2: CLOUD RISE

4.1 Summary of Photostations. 31

SE E R 7

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TABLES (Continued)Page

CHAPTER 6 PROJECT 3.6: BHANGMETERS, MOD Ii

6.1 Bhangmeter Results, King Shot . 39

APPENDIX B FILM COMPOSITION AND DISPOSITION

B.1 Mike Release-print Assemblies 68B.2 King Release-print Assemblies 68

APPENDIX C METEOROLOGICAL DATA

C.1 Meteorological Conditions, Operation Ivy . 69

8

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SECRET

CHAPTER 1

INTRODUCTION

Various types of photostations were used in Operation Ivy. A 125-ft tower (Station 301),shown in Fig. 1.1, was located on Elmer. Figure 1.2 shows some of the cameras installed inthe racks. A second photostation (Station 302) was set up on a concrete pier at the foot of thistower, with cameras enclosed in heavy lead boxes mounted on top of the pier. The lead boxeswere employed as shielding against the possible heavy fall-out radiation. A third station onElmer (Station 308) was located inside the control-room compound. Three other major photo-stations constructed dimilarly to Station 302 were built on top of existing timing stations onJanet (Station 303), Ursula (Station 306), and Yvonne (Station 307). In addition, an EastmanCine Special camera was mounted on a special concrete column on Ursula (Station 305) torecord water-wave motion on Mike shot. For King shot the coral station Oscar (Station 304)was activated with two Galileo phototheodolites to record position of burst. Figure 1.3 indi-cates the positions of the sever•a ground stations.

Supplementary yield cameras were operated on Mike shot from the USS Estes, primarilyto provide a means of determining yield quickly should reentry to the atoll be delayed. Cloud-rise photography on Mike shot was documented from both the USS Curtiss and the USS Estes,as well as from two C-47 aircraft flying at varying distances from Ground Zero.

Because of the high levels of fall-out radiation that could be expected from Mike shot, allthe ground-.sation cameras were shielded by lead boxes whose sides consisted of 11/2 in. oflead sandwiched between '/2 in. of steel plate. These boxes were made in two sizes, one for thelarger cameras and the other for the smaller ones. Figure 1.4 illustrates a typical shielded-camera installation.

Timing signals were sent from the master timing station on Flora through cables eitherdirect to the photostation or relayed through auxiliary timing stations. These signals, occur-ring at -15 rain and -15, -2.5, -1.5, and -0.5 sec, closed DN-11 relays, which caused variousof the camera electricel circuits to be closed, thereby making the cameras operate at theproper time. Block diagrams of the various photostations are presented in Appendix A. 'Fur-ther.information on the timing and ccntrol systems of Ivy may be found in Report WT-609,Timing and Firing and Fiducial Markers.

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II

-40

4�-

* N

0.A-

U2

-4'-4

IL

10

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IN

SECRT -RSTRCTEDDAT

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G _I

A~ ~ EIA, tHSTA.303

STA. 300 L 0K

STA. 300)VSTA. 306

A i• STA. 307

STAS 004

,hz

4AA

#BB

GCC

*DD

SLL STA. 301k•STA. 302 E ESTA. 308

J(K

"* HH

ENIWETOK ATOLL

Fig. 1.3-Map of photostations.

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IA

IcEiI

~ t93k

oh

13

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CHAPTER 2

FILM HANDLING

A fully equipped photo-processing trailer belonging to Edgerton, Gernieshausen & Grier,Inc. (EG&G), was shipped to Eniwetok to take care of all black-and-white processing require-ments. Films were stored in refrigerators on Elmer until needed. At least one completecamera dry run was made before each shot, and films used for this run were perforated,loaded, and processed just as for a live run. Film was taken out of th? refrigerators, perfo-rated with the appropriate EG&G identification number, exposed to a sensitometric strip andreticle, and readied for loading into cameras at least 24 hr before the scheduled shot time.

As soon as possible after the shot was fired, recovery parties returned to the photo-stations and removed all film from the cameras, checked to be sure which cameras had oper-ated properly, and noted any improper operation.

Since the processing trailer was located on Elmer, the films from the stations on thisisland were unloaded immediately and processing was commenced. The processing plan wasto develop all films in order of importance, i.e., Rapatronics and Eastman yield films first, sothat a quick preliminary analysis could be made. Films from the slower motion-picture cam-eras, as well as any other glass plates, would then be developed according to size and emulsion.

On Mike shot, because of the unusually wide range of light levels, many of the films werebadly under- or overexposed during some portions of interest. Thus each Eastman film wasdeveloped individually to make sure that the most information possible was obtained.

As soon as the major films were dry, they were analyzed for a preliminary yield figure.Analysis facilities consisted of a small light box and rewinds built into one end of the photo-trailer and a Hauser Profile Measuring Microscope, Fig. 2.1. Position of burst was also de-termined here for King shot, and a preliminary report was issued.

After the preliminary analysis work had been done, motion-picture films were shipped toHollywood for printing before being returned to Boston for final analysis. It should be pointedout that the field processing facilities could handle only black-and-white development, so thefinal step of converting some footage to color by rehalogenation (Eastman Color Negative) wasdeferred until EG&G personnel could direct this step at the Air Force Lookout Mountain Labo-ratory in Hollywood.

The process for preparing a single-topic reel of typical black-and-white films for releasewas as follows:

Original camera negative was spliced into a convenient roll no longer than about 1000 ft,including perforated identification numbers, gray scales, and graticules. Fine-grain masterpositive contact prints were made in sufficient number and variation with experimental ex-posures to allow editing and intercutting of one best standard master. The range of exposuresused, sometimes within a few-foot length, was from the least exposure commercially availableto more than 40 per cent above the highest standard exposure. Duplicate negative footage was

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then generated in camera position to act as printing master for release films and was editedfurther for the screen.

A titled negative show was then prepared by cutting in slates, credits, maps, ar,d securityleader negatives that were separately prepared fion field notes. Release prints were issued,after one or two trial prints to ascertain the best screen effects. These were further edited onthe basis of the net effect of a whole show and the particular detail it was possible to preserva

Fig. 2.1 -Hauser Profile Measuring Microscope.

at various light levels. (The pictures that are issued are really a copy of a copy of a copy, andthe original negatives are never printed for release.)

Preparation for the laboratory and cutting-room work for this operation required themanufacture of titles. Worcester Film Corporation made '15 black-and-white titles for indi-vidual film slates, to which were added scale bars to give dimension to the various camerafields of view. EG&G prepared 10 main titles and 12 maps to identify camera purposes, posi-tions, and "targets. For Mike and King shots, 800 ft of titles was required.

A cutting room with Movieola and projector was rented from the Hollywood Film CompanyEditing Film Center. Consolidated Film Industries printed and developed the film. CinemaResearch ran two sets of optical prints required for title and scene. On the holidays andweek ends, Lookout Mountain Laboratory provided additional space and equipment where se-curity required.

A total of approximately 17,000 ft of release prints was made and released to the interestedagencivs. Distribution of the various reels is listed in Appendix B.

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i

CHAPTER 3

DDOp IEIT 1 1. rID.tAtI VIIE 1" iTI:TDAAIkIATIftM

As on previous operations, fireball diameter was measured from various types of photo-graphic records and plotted as a function of time. These data are used in the determination ofthe energy release of the nuclear device (so-called fireball scaling) and in the determination offrpe-air overpressures by the hydrodynamic relations between pressure and shock velocity.

3.1 PROCEDURES

3.1.1 Mike Shot

The techniques necessary for satisfactory photographic coverage of Mike shot were com-plicated by the gross uncertainty of the expected yield. It was necessary to plan the photo-graphic coverage on the basis of a probable yield of 4.5 MT and on the basis of possible limitsof from 50 KT to 40 MT. The primary determination was obtained from six Eastman high-speed cameras located at Station 302, the ground station on Parry Island. Each camera wasshielded against fall-ot radiation by a factor of approximately 100. Backup photography wasprovided by a group of 12 unshielded Rapatronic cameras in Station 301, the 125-ft-high Parryphototower.

In order to cover the eventuality of a low-order explosion, a photostation was set up onEngebi (Station 303) with five Eastman high-speed cameras, each shielded against fall-outradiation by a factor of 100. This station was only 19,400 ft from Mike zero as compared to adistance of 114,000 ft for the Parry stations. Three of the Eastman cameras were providedwith long-focus lenses to cover the possibility of a low-order detonation; the other two wereprovided with short lenses to back up the measurements being made from the two Parry sta-tions.

The problem of being able to determine a quick, reliable yield figure, in the event that re-entry to the atoll would be delayed, was met by mounting two Eastman cameras on a stabilizedplatform on the kingpost of the USS Estes. These cameras were set to run at approximately1000 frames/sec.

Figure 3.1 shows a typical installation of shielded cameras, in this instance Station 302 onParry. To position these cameras, they were faced away from Ground Zero, then rotated 900to a vertical position and mounted on the rear panel of the lead boxes. This method of cameraarrangement meant that images received were reversed left to right from the normal image.Mirrors were mounted on the tops of the lead boxes and adjusted to approximately a 450 angle bymeans of setscrews. Each mirror was held in a closed position by means of a wire; when apredetermined signal was received, the wire burst and a counterweight caused the mirror toopep and maintain its correct position. A thick lead-glass plate in the top of the lead box al-lowed the mirror object image to be viewed by the camera. It was felt that these elaborate

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- MY-

rv4.2

;i,,ý -- - -

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iip ,~eatioria ~ ~ ~f~-oni i :s a radiation fail-out were necessary0, 1m , r t~'e7 w't4 of' e the expli slon.

1.). 2 r. ; Sh o

For King shot the fireball diatc werc to be obtmi-rid irew Ea••iuan and Rapatronic camerason Parry. Since King shot was aa airdrop, the Eastman cameras were run in throe time groupsto allow 'or possible errors in time of fall.

3.2 CAMERAS AND LXPOSURES

Data describing the operation of all cameras used on both shots have been issued -s Re-port EG&G-OUT 1517, Ivy Film DW Sheet Catalog, 24 February 1954, and are given in partialform in Appendix D, Camera Data Sheets.

3.2 1 Mike Shot

Tables 3.1 and 3.2 summarize the operation of the Eastaan and RaptAronic cameras, re-spectively. The films, in general, suffer from being underexposed owing to the unexpeced low

Tabhe 3.1-SUMMARY OF EASTMAN OPERATION, MIKE SHOT

Camera Film Effective Speed at zero, HorizontalNo. No. Station aperture frames/sec field, meters Ranr irks

E20 16101 302 4 3060 No timing marksE15 16102 302 8 2280 3060E12 16103 -302 18 2180 3060E18 16104 302 2.7 1055 3060 Best record fox minimumE24 16105 302 12 Did not runE10 16106 302 40 Did not run

E16 16107 303 5.6 2090 525E9 16108 303 1? 2760 525E25 16109 303 80 2570 525E27 16110 303 5.6 2580 2100Ell 16111 333 L1 2560 2100

E26 16112 USS Estes 5.6 1240 4950E7 16127 USS Estes 5.6 1250 8020

radiant emittance of the fi '1. Three of the primary Eastman cameras on Parry ran prop-erly. One camera ran, but elocity-marker spark failed to give any indication. Two cam-eras did not run owing to a I contactor. Of the three good records, only one was exposedheavily enough to show fireball detail into the minimum. The two high-order backup camerasat Station 303 ran properly and yielded useful records. Both Eastman cameras on the USSEstes operated properly, although one was slightly misaimed.

One Rapatronic camera failed because of a faulty me'hanical capping shutter, and threeothers triggered satisfactorily but do not show images owing to underexposure. One camera,R19, ei idenced a fauity time delay.

3.2.2 King Shot

Tables 3.3 and 3.4 summarize the operation of the Eastman and Rapatronic cameras, re-spectively. The six Eastman cameras used on King shot to record fireball data were 100 percent satisfactory in opbration. Because of the staggered time sequence of operation, only four

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ITable 3.2- SUMMARY OF RAPATRONIC OPEPATION, MIKE SHOT

ExpisurePlate time, Time, Background Image

No. Emulsion* •..,'e msee density density Remarks

16141 HRHS i 0.028 Capping-shutterfailure

16142 MF 4 0.101 0.50 Underexposed16143 MF 4 0.305 0.50 Underexposed J

16144 M? 4 0.910 0.38 Underexposed16145 MF 4 2.98t 0.50 0.62

16146 HRHS 4 10.3 1.75 2.00 Only skirt of fire-ball is imaged

16147 hRHS 4 20.2 1.00 1.20 Only skirt of fire-ball is imaged

16148 Tri X 4 39.5 0.30 0.32-0.65 Bright skirt,faint top16149 Tri X 40 68.8 0.30 1.03 Excellent picture

16150 Tri X 40 35.0* 0.29 1.04-1.50 Bright skirt,faint top

16151 Tri X 40 153.0 0.28 0.33-0.4116152 Tri X 40 205.3 0.30 0.32 Very faint image

* The sensitometric characteristics of these ermulsions have been presented in Ball-of-fire Obser-vations, Greenhouse Report, Annex 1.4, WT-101.

tThe fireball diameter is not consistent with this time of operation, and it is concluded that the timedelay was faulty.

tSalt water leaking through the tower-cab roof altered the delay of this camera from its set-in valueof 103.5 to 35.0 msec, as measured after the shot.

Table 3.3 -SUMMARY OF EASTMAN OPERATION, KING SHOT

Camera Film Time Effective Speed at zero, HorizontalNo. No. sequence aperture frames/see field, meters Remarks

E20 16201 First 4 3050 1480El5 16202 First 8 2870 1480E12 16203 Second 4 1295 1480 Best record at minimumEl8 16204 Second 8 1820 1480E24 16205 Third 5.6 1480 Started after zeroEl0 16206 Third 11 1480 Started after zero

cameras show the initial burst and fireball growth. Twelve Rapatronic cameras were used,and all show images. Five of these (in the interval 0.1 to 10 msec) give good measurable im-ages, four others are too weak to read, ard the remaining three clearly show the fireball aftershock separation and minimum time. These last three cameras show interesting pictures, butthey are not useful for fireball scaling. Camera R19 again evidenced a faulty time delay.

It had originally been intended to operate all Rapatronic cameras in the time range priorto minimum time, but, owing to the lack of time between shots, it was not possible to changethe time delay of the cameras from their Mike shot settings. For this reason Rapatronic datasuitable for scaling were not obtained.

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Table 3.4 -SUMMARY OF RAPATRONIC OPERATION, KING SHOT

ExposurePlate time, Time, Background ImageNo. Emulsion* psec msee density density Remarks

16241 HRHS 4 0.028 0.13 0.16 Weak image16242 MF 4 0.101 0.10 0.15 Weak image16243 MF 4 0.305 0.10 0.63 Good image16244 MF 4 0.910t 0.10 0.52 Good image16245 HRHS 4 2.98 0.15 1.24 Good image

16246 HRHS 4 10.3 0.11 0.45 Good image16247 HRHS 4 20.2 0.11 0.15-0.23 Weak imaget16248 Tri X 4 39.5 0.28 0.23-0.48 Weak image'16249 Tri X 40 68.8 0.32 0.34-0.39 Weak image16250 Tri X 40 103.5 0.29 0.85 After minimum16251 Tri X 40 153.0 0.29 1.08 After minimum16252 Tri X 40 205.3 0.28 0.30-0.38 After minimum

* The sensitometric characteristics of these emulsions have been presented in Ball-of-fire Obser-vations, Greenhouse Report, Annex 1.4, WT-101.

tThe fireball diameter is not consistent with this time of operation, and it is concluded that the timedelay was faulty.

!Cor- brighter than periphery.

3.3 FIREBALL DIAMETER-TIME CHARACTERISTICS

The basic elements that go into the precise determination of fireball diameter-time char-acteristics are the selection, processing, and subsequent handling of a photosensitive emulsion;the maintenance and operation of camera and control circuits; the determination ol space andtime scales; the accurate measurement of the images; and the mathematics of data analysis.The techniques used in Operation Ivy were essentir.lly identical to those employed in OperationTumbler-Snapper with the following important diZ_-rences.

1. Owing to the large minimum time of both Mike ana King shots, it is not necessary tocalculate an accurate zero-time correction for the first frame of an Eastman record.

2. The Eastman cameras at the ground station on Parry (Station 302) could not see theground at the shot island owing to curvature and refraction. In measuring the fireballs it wasassumed that the surface war 'iemispherical and matched concentric circles on the readingcomparator to the upper por i of the fireba'l that could be seen above the horizon.

3. The size of the Mike fireball was sigrijicant compared to the distance of the fireballfrom the Eas3tman cameras at Engebi (Station ý03). The effect of tVhs is that the magnificationfactor changes with fireball size. This effect was compensated for by introducing a correctionfacto , the maximum magnitude of which was about 2 per cent. The correction is calculated asfollows:

TRUE PICTURE PLANE

k ASSUMED PICTURE PLANE

i j- OPTICAL AXIS

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Let D = distance from camera to center of fireball (on the assuwption that the optical axispoints at the center of the fireball)

f = focal length of optical systemR = true radius of fireball

RI = incorrect radius of fireball, calculated without correctionM = magnification = D/fr = R/M = fictitious image radius corresponding to true fireball radius

r' = R'/M = measured image radiustan a = R'/D = r'/f = tangent of measured semiangle

The angle a is essentially determined from measurements on the film. If it is assumedthat the picture plane was a distance D from the camera, the fireball radius would be R'. Thetrue radius is R. The relation between R and R' is as follows:

R = D sin a (3.1)

R' = D tan a (3.2)

Therefore

R _r r? YP21~= = Cos a = +1 (3.3)

This correction factor is employed to correct the Engebi measurements for the effect ofcamera proximity.

All measurements and calculations from the various Eastman records have been publishedin detail in EG&G Report 1083, Ivy Fireball Diameter-Time Characteristics. However, a sum-mzry plot of fireball diameter vs time for Mike shot is presented in Fig. 3.2 and for King shotin Fig. 3.3. Tables 3.5 and 3.7 give the same data in tabular form. Diameter measurementsfrom Rapatronics are shown in Tables 3.6 and 3.8.

3.4 FIREBALL SCALING

The techniques of scaling yields of nuclear detonations by means of the fireball diameter-time relation have been discussed in t".e various ball-of-fire reports for previous operations.We shall, therefore, only treat the sabject superficially here.

The general diameter-time relation is of the form

D = Ktn (3.4)

The parameter 0 is defined as the proportionality constant in Eq. 3.4 when the exponcnt nis equal to 0.4.

D = Ot°' 4 (3.5)

In the time interval where r = 0.4, the yield is proportional to the fifth power of (P. It hasbeen shown in previous work on fireball scaling that the yield may be determined from therelation

W = .294 x 10-1 p 0' (3.6)

where W = total energy release, kilotons

p = air density at burst, grams per literS= average value of diameter (meters)/time2"S (milliseconds) for all films (averaged

over the region of 0.4 slope)

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I

Table 3.5--FIREBALL DIAMETER AS A FUNCTION Table 3.6-FIREBALL DIAMETER AS A FUNCTIONOF TIME, MIKE SHOT OF TIME FROM RAPATRONICS, MIKE SHOT

Time, Diameter, Time, Diameter,msec meters Plate No. msec meters

1 311 16145 2.98* 4252 402 16146 10.3 7005 563 16147 20.2 916

10 728 16148 39.5 120220 941 16149 68.8 149250 1320 16150 35.0 114370 1492 16151 153.0 2036

100 1721 16152 205.3 2320

150 2024 *This tme is suspect.200 2271250 2482

Table 3.7-FIREBALL DIAMETER AS A FUNCTION Table 3.8-FIREBALL DIAMETER AS A FUNCTIONOF TIME, KING SHOT OF TIME FROM RAPATRONICS, KING SHOT

Time, Diameter, Time, Diameter,msec meters Plate No. msec meters

1 155 16242 0.101 70.82 195 16243 0.305 98.75 266 16244 0.910 138

10 342 1624t 2.98* 21220 441 16246 10.3 34440 577 16250 103.5 73760 679 16251 153.0 88370 722

*This time is suspect.

Table 3.9--( AS A FUNCTION OF TIME, MIKE SHOT Table 3.10-4 AS A FUNCTION OF TIME FROMRAPATRONICS, MIKE SHOT

Time,msec 4,meters/msec Time,

Plate No. msee p, meters/msec1 3112 305 16145 2.98* 2755 296 16146 10.3 275

10 290 16147 20.2 27520 284 16148 39.5 276

16149 68.8 275516150 35.0 276S70 272.8 S16:1 153.0 272

100 272.8150 272.8 16152 205.3 276200 272.8250 272.8 *This time is suspect.S250 272.8

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The average value of 4 in the region of 0.4 slope is obtained simply and accurately byarithmetical averaging since 0 is constant in this region.

3.4.1 Mike Shot

The 0 vs time data for Mike shot are presented in Fig. 3.4 and in Table 3.9. The P dataas calculated from the Rapatronic pictures are presented in Table 3.10.

From Fig. 3.4 and Table 3.9 it is seen that the value of 0 in the region of constant 4 (t - 60msec) is equal to 272.8 for Mike shot. The yield can be determined from Eq. 3.6 with a modifi-cation due to the fact that the device was detonated on the ground and that the energy was con-centrated in a hemisphere.

Because of the large size of the Mike fireball, it was felt that an average air density overthe entire fireball should be used rather than the simple value of air density at burst heightwhich suffices for smaller detonations. It was therefore decided to use the density of air at thecenter of gravity of the hemisphere, or 0.3473 times its radius. This radius was chosen at thetime t which is the logarithmic midpoint of the constant q5 region (t = /'tl t 2). At this time(127 msec) the radius was 3051 ft, giving a center of gravity of 1060 ft above ground. The airdensity at this level was 1.118 g/liter. Scaling wa.s then accomplished according to Eq. 3.6 withan added factor of 0.5, p"ompted both by theoretical considerations of surface shots and by ex-perience on Jangle J shot. Therefore

W = '/2(1.294 x 10-8)(1.118)(27'4 8)5 = 10,900 KT

The method of calculating the probable error ip yield of detonations exhibiting a region ofgrowth of constant 0 has been explained in detail in Greenhouse Report WT-101, Ball-of-fireObservations. One considers only the data in the region of constant P and calculates the stand-ard deviation of a single reading from the average 0 fcr the particular film. By weighting thesevalues according to the number of readiihgs made of a film, one can calculate the standard devi-ation of a single reading considering all films as the population. It is preferable to performthis calculation in two steps since there are errors in the magnification and time scales and itis not correct to assume that all films are from the same pop .lation. By dividing the stapdarddeviation of one reading for all films by the square root of the number of film readings con-sidered in the determination of the average 4, one determines the deviation of this averagevalue of 4P, d. Additional errors are introduced by systematic errors, such as film shrinkage,errors in magnification of the reading comparator, and errors in the calculated optical-axisdistances. We assign a standard deviation of 0.2 per cent to these errors. We also assign astandard deviation of 0.1 per cent to systematic errors in focal length.

There is also an additional error due co possible errors in the evaluation of air density towhich we assign a standard deviation of 0.5 per cent. The yield is proportional to the fifthpower of 4 and the first power of air density. Thus the standard deviation of the yield measure-ment is expressed by

•yield = 25 [7 + (0.2)2 + (0.1)2] + (0.5)2

= 25 U7- + 1.50

and the probable error is

PEyield = 0.67 [2_5 U2 + 1.50 (3.7)

The data from which the probable error in the yield of the Mike shot is calculated are pre-sented in Table 3.11.

It is believed that a probable error in yield of ±0.8 per cent is smaller than the real proba-ble error owing to (1) possible uncertainties in the factor of 2, introduced to take account ofground reflection, (2) possible errors in the scaling law in this yield range, and (3) possible ef-

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I

Table 3.13 -STATISTICAL ANALYSIS OF MIKE FIREBALL DATA

No. readings, (0 - 7)2, Probable errorFilm No. time >60 msec % C, % i yield, %

16111 272.6 20 13.4516110 271.9 16 20.7516304 273.6 17 8.6616103 273.9 14 7.0816102 272.1 26 24.48

Z = 93 0.0091 *0.82

Table 3.12 - AS A FUNCTION OF TIME, KING SHOT

Time,msec €, meters/msec%

1 1552 1485 140

10 13620 13340 132.060 132.070 132.0

Table 3.13--p AS A FUNCTION OF TIME FROM RAPATRONICS,KING SHOT

Time,Plate No. msec 0, meters/msece

16242 0.101 17716243 0.305 15916244 0.910 14316245 2.98* 13716246 10.3 13516250 103.5 119.8t16251 153.0 118.01"

*This time is suspect.

tAfter minimum.

Table 3.14--STATISTICAL ANALYSIS OF KING FIREBALL DATA

No. readings, z((A - 4)2, Probable errorFilm No. time >40 msec % U!, % in yield, %

16201 131.9 15 2.2416202 131.9 3 0.5616203 131.8 10 6.5816204 132.5 3 2.53

Z = 31 0.0108 *0.82

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fects resulting from the considerable change in atmospheric pressure, temperature, and den-sity with fireball altitude (4500 ft at time of minimum). We feei that a probable error of +5 percent is more realistic.

3.4.2 King Shot

The p vs time data for King shot are presented in Fig. 3.5 and in Table 3.12.The P data as calculated from the Rapatronic pictures are presented In Table 3.13.From Fig. 3.5 and Table 3.12 it is seen that the value of (A in the region of constant (A is

equal to 132.0 for King shot. The yield can be determined from Eq. 3.6 using 1.109 g/liter asair density as given in Appendix C. Therefore

W = 1.294 x 10-8 (1.109)(132.0)' = 575 ± 5 KT

The probable error in yield is determined by means of Eq. 3.7. This calculation is illus-trated by Table 3.14. We feel that the statistically derived error is valid in this case since theunknown factors mentioned in the evaluation of the Mike shot errors are much smaller for Kingshot.

Iy

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CHAPTER 4

PROJECT 3.2: CLOUD RISE

The cloud-rise program, Project 3.2, was devised to supply intert sted groups with infor-mation pertaining to the rate of rise and the various dimensions and height attained by the cloud

and stem resulting fron the detonation of Mike and King shots. An extensive analysis was madeof the photographs obtained on both shots. Results of this analysis appear in EG&G Report 1136,Cloud and Stem Phenomena, Operation Ivy, 23 April 1954. A summary of this report is pre-sented here.

4.1 MIKE SHOT

One C-47 aircraft flew approximately 80 nautical miles to the east of Ground Zero on asouth-to-north course at the time of burst at an altitude of 10,000 ft. An A6 35-mm movie cam-era started at M-15 sec and ran until approximately M +1 min. Pictures were also taken atthe rate of one a minute by a hand-held Speed Graphic camera from zero time until M+1 hr;however, no record was obtained at M + 1 min. At zero time the aircraft ran into a thunderhead,causing turbulence and poor visibility. Many of the late-stage photographs are of no value owingto interference from normal clouds passing between the plane and the bomb cloud.

A second C-47 was about 68 nautical miles south-scuthwest of the zero point at zero time,

flying a west-to-east course at 12,300 ft. Pictures were taken from this aircraft every minuteby a hand-held Speed Graphic from M + 1 min to M + 1 hr.

In gr ieral, the C-47 to the south gave better early coverage, and the later stages werebest recorded from the C-47 to the east.

Speed Graphics were also set to record cloud progress at 1-min intervals from the USSCurtiss and the USS Estes. The Curtiss gave a much better group oi Seeed Graphic records ofthe Mike cloud than did the Estes. At zero time the Curtiss was 214,000 ft due east of GroundZero, proceeding at approximately 2 knots on a bearing of 090'. A Speed Graphic was utilized torecord a picture of the cloud formation once every minute, as was done in the C-47 aircraft.Only those pictures taken up to about M + 10 min proved valuable since the cloud had extendedbeyond the field of view of the camera by this tinme.

The USS Estes, which was 184,000 ft south of the zero point, was cruising at 5 knots on abearing of 1500 and a course of 3300 at the time of detonation. The intention was to take one

photograph every minute with a Speed Graphic, but, owing to the interference from the normalcloud cover, pictures were taken only when a break in the clouds gave a reasonable view of thebomb cloud. Of these films only those taken at M+3 and M+5 min gave valuable information.

Further coverage of the Mike cloud was supplied by three Mitchell 35-mm cameras located

on Parry Island. Two low-6peed Mitchells were located at Station 308, 115,040 ft from the zero

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point, and were set to expose one frame every 2 sec. These records provided a series of highlyvaluable and spectacular pictures of the stem formation and cloud rise. However, the first 17frames in each camera were in fogged leader; measurements consequently began at 34 sec.

The third Mitchell, a 100 frame/sec camera, was located at Station 301 (the Parry Islandphototower), 114,510 ft from Ground Zero, and provided valuable information on the earlystages of the stem and the cloud.

Table .1. gives a summary of the photostations used.

Table 4.1-SUMMARY OF PHOTOSTATIONS

Film Camera Approximate direc- Distance f-om GroundNo. location tion at zero time Zero at zero time, ft

Still-camera Stations

16000 C-47 East 484,00016010 C-47 South-southwest 415,00016020 USS Estes South-southeast 184,00016030 USS Curtiss East 214,000

Motion-picture-camera Stations

16119 Station 308 South-southeast 115,04016120 Station 308 South-southeast 115,04016121 Station 301 South-southeast 114,510

4.2 WNG SHOT

Photographic coverage of the King cloud consisted of two Speed Graphics, three low-speed35-mm Mitchell cameras, one high-speed Mitchell, and a manually operated Eastman CineSpecial. These cameras were located in a C-47 and at Stations 302 and 308.

A C-47 flying at 10,000 ft on a west-to-east course 30 nautical miles due south of GroundZero at zero time covered the King cloud. A 48 frame/sec A6 camera ran from zero time untilK + 45 sec, and a Speed Graphic recorded at varying intervals from K 4 1 min to K + 1 hr.Both of these cameras were hand held.

Cameras were also operated from Stations 302 and 308 on Parry Island. Station 308 con-tained two low-speed Mitchells for cloud-recording purposes; however, these did not operateowing to power failure before zero time. Station 302 contained one high-speed Mitchell whichran at 140 frames/sec, one Speed Graphic, and one Eastman Cine Special which r- n at 24frames/bec.

On the aerial photographs it was impossible to see any ground reference point, owinglargely to the normal cloud-cover interference. However, it was possible to locate a referencepoint or the cloud stem, visible on both an aerial -,cord and a Parry Island Speed Graphicrecord. Thus, knowing the altitude of this reference point from the ground photograph providedan altitude aetermination for the aeria shots. Two such points were located, and the attitudewas averaged.

4.3 RESULTS

Because results obtained from the cloud films have been reported in detail elsewhere, onlythe highlights of the analysis will be mentioned here. The Mike cloud reached its maximum

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height of slightly over 100,000 ft in about 4 min, at which time the diameter had spread to morethan 100,000 ft. At the end of 1 hr the cloud had spread out over a range of 300,000 ft. Figure4.1 sketches the progress of the cloud during the first 10 min. Figure 4.2 shows four curves:maximum diameter, maximum height, height of maximum diameter, and height to bottom ofcloud. The curve showing the maximum height of the cloud splits and gives a separate valuefor the thunderhead as it pusl• .s on above the main cloud. A typical frame from a Parry cam-era appears in Fig. 4.3.

The King cloud attained its maximum height of 65,000 ft in slightiy over 4 min, while grow-ing to a 40,000-ft diameter. Figure 4.4 gives the diameter, height of top, height to bottom, andheight of maximum diameter of the cloud throughout a 10-min period. A photograph from theC-47 Speed Graphic, Fig. 4.5, shows the cloud just before it reaches maximum height. The icecap which formed above the cloud is also clearly visible.

The results as presented should be considered reliable to :L10 per cent for 10 min on bothshots.

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II

CHAPTER 5

PROJECT 3.5: LUMINOUS EMITTANCE VS TIME

Two General Radio slit cameras of the same type used on previous operations, viz., Opera-tions Ranger, Greenhouse, Buster-Jangle, and Tumbler-Snapper, were operated on both shotsfrom Station 301, the Parry pnototower. Discussion of the principles and method of operation ofthese cameras appears in Technical Photography, Buster-langle Project 10.3 Report, WT-417.Location and operation of the two cameras were identical for both Mike and King shots, with theexception that the cameras were set for a much slower running speed for King shot because ofthe uncertainty in expected zero time. Six slit channels were employed on each camera, filteredin even steps from ND-0 (no filter) to ND-3.0 (light attenuated 1000 times). One camera usedblack-and-white microfile film, whereas the other used Eastman Color Negative in an attemptto record data over a wide spectral band.

Owing to the fact that the light levels were much lower than anticipated on Mike shot, theEastman Color Negative record blanked out some time before minimum, but the black-and-white film provides a useful record on two channels through the minimum. Neither of the cam-eras operated on King shot.

As yet, no attempt has been made to analyze the one useful record obtained from Mike shot,owing to the problems of film sensitivity in the various wavelength bands, as outlined in Tech-nical Photography, Tumbler-Snapper Project 12.1 Report, WT-569.

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4CHAPTER 6

PROJECT %3.6: BHANGMETERS, MOD II

Bhangmeters similax to those used on Operations Buster-Jangle ; ,Umbler-Snapperwere used on Ivy. The evaluation of this instrument can be traced thr ,i previous reports.1

Bhangmeters used on Mike shot incorporated special modifications of the old Bhangmetersin view of the extremely leng minimum time expected, the circuit time constants of the stand-ard models being inadequate. Standard units were used on King shot, although new sweep andoscillator parameters were required.

Four Bhangmeters, ali using a 110-volt a-c power supply, were operated from the USSEstes on Mike shot. Three of these used 100 cycle/sec marks, and the fourth used 250cycle/see marks to cover the eventuality of a possible low-order burst. Only one of the fo'urBhangmeters triggered, and the time to minimum was so long that this record showed only acontinuous decrease in light level beyond the recording time. This record appears in Fig. 6.1.

Five Bhangmeters, all operating on 110 a-c volts, were used for King shot, one at Station302 at the foot of the phototower, two at Station 308, and two in the Parry control room, Sta-tion 311. All five of these units gave satisfactory records. Table 6.1 summarizes results ob-tained from the King shot Bhangmetfcrs. Time to minimum is converted to yield by means ofthe calibration curve shown in Fig. 0.2, which was obtained with the aid of radiochemical dataon Operations Sandstone, Ranger, Greenhouse, Buster-Jangle, and Tumbler-Snapper. King shotBhangmeter records are reproduced in Fig. 6.1.

Table 6.1-BHANGMETER RESULTS, KING SHOT

Time to minimum, BhangmeterLocation msec yield

Statior 308 68 440 + 90 KTStation 308 68 440 ± 90 KTStation 302 68 440 • 90 KTStation 311 68 440 ± 90 KTStation 311 68 440 • 90 KT

REFERENCE

1. Air Drop Instrumentation: Bhangmeter, Greenhouse Report, Annex 1.9, Part I, WT-92;Bhangmeter Mod II, Buster-Iangle Project 10.3b Report, WT-403; Bhangmeter Mod H,Tumbler-Snapper Project 12.1 Report, WT-562.

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MIKE TMIN. UNKNOWN KING TMIN.- 68MSU SS ESTES STA. 308

KING TMIN. 68MS KING TMIN. =68MnS

STA. 308 STA. 302

KING TMIN. 68ms KING TMIN. 68ms

STA. 311 STA. 311

Fig. 6.1-Bhetngmeter records, Mike and King shots.

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sa003S-1 Pnl 01 ; ;31NU 03AUSN

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CHAPTER 7

PROJECT 3.8: POSITION OF BURST

Position-of-burst determination was required for the King airdrop. One Wild theodolitecamera was set up at Station 306 on Rojoa, backed up by a Galileo phototheodolite at the samestation. Two Galileo type phototheodolites were set up on the Holmes and Narver (H&AN) coralsurvey station (Station 304) to provide approximately 900 coverage. A second Wild phototheodo-lite was located at Station 302, the Parry ground station. Figure 7.1 illustrates approximatecamera positions. All cameras were equipped with faster shutters than were used on previousoperations in an attempt to gain more precise determination, although any gain here would beoffset by the greater distances over which the cameras were to operate,

Of the five cameras, only the Wild at Station 302 operated satisfactorily. The others weredamaged by rust due to the heavy rains on the days previous to shot day, with consequent jam-ming of the mechanisms. Triangulation was accomplished using the record from one of theGSAP cameras of the Naval Research Laboratory, aimed at rocket trails from Station Mack,in conjunction with the one good theodolite record.

Burst coordinates were determined in a coordinate system using the H&N coral surveystation 304 as origin (N 100,000; E 100,000). This station is located at latitude 11032,20," N andlongitude 162017111" E. In this system the King burst was determined to be

N 108,450 ± 30'E 123,650 ± 20'Height: 1480 ± 20 ft above sea level

These coordinates correspond to a value of latitude 11*33'44" N and longitude 162o21109" E.Drop error was computed to be

300 ± 30 ft north480 ± 20 ft west570 + 30 ft radially

42

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CE

A Alce BgalU STA. 306 -AIEB Belle Bogombogo

C Clara RuchiD Daisy Cochiti bw

E Edna SanildefonsoF Flora Elugelab

G Gene TeiteiripucchiH Helen Bogairikk

I Irene Bogon MACK

J Janet Engebi GK Kate Muzinbaarikku GSAP(NRL) A STA. 304

L Lucy Kirinian 2-GALILEOS

M Mary BokonaarappuN Nancy Yeiri ,6Z0 Olive AitsuP Pearl RujoruR Ruby Eberiru AA Alvin Chinieero 1AAS Sally Aomon Ak Brucn AhiniieroT Tilda Biijiri BB Bruce ACiniy i 'BB

U Ursula Rojoa CC Clyde Chinimi

V Vera Aaraanbiru DD David Japtan iccW Wilma Piiraai EE Elmer Parry

Y Yvonne Runit FF Fred Eniwetok

Z Zona Site M GG Glenn Igurin *DDHH Henry Mui

VLL II Irwin P"kon STA. 302

"JJ James Ribaion i-WILD EE

KK Keith Giriinien

K LL LeRoy Rigili

"GGG

ENIWETOK ATOLL

Fig. 7.1-- Theodolite- camera locations, King shot.

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CHAPTER 8

PROJECT 6.2: MORTAR AND GUN BURST

As in Operation Tumbler-Snapper, Group J-10 of the Lcs Alamos Scientific Laboratory(LASL) undertook to measure free-air pressures by observing the motion of smoke-labeled airparticles under the influence of the shock wave. For Mike shot, Mitchell high-speed cameras,shielded against fall-out radiation L, the same manner as described in Chap. 1, were set up onfour different islands to observe the motion of mortar and gun puffs. Each camera viewed twopuffs, some of which were at high altitudes (5000-26,000 ft) and others at low altitudes (ap-proximately 400 ft above ground). On King shot, only the low-altitude puffs were used, and allthe cameras were located on Rojoa. All cameras operated successfully, and films from thisproject provide a good record of motion and shock progress.

Figures 8.1 and 8.2 show puff locations and camera fields of view.

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a-0-

cnd

2 00

U,- s 0. 3j 0

' 5 0

45

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40

GUN BURSTS VIEWED

- -- ---- --- FROM "U"152 mm I -

LENS I ._FINAL Showing initialI -position of lower

burst and final

"I INITLAL1 position of upperSI burst, together

I i with limiting

30 . -t camera flelds

II(D I

L !

CIl I.j 204

Cr L-- 4-

0-

L \

---------------------------------\-------.

0. IOmmII LENS

10h ------------- i

SEA RAT ON

20 10 LEFT 0 SIGHT 10

DEGREES RE GROUND ZERO

Fig. 8.2-Camera fleid3 of view, gun-burst photography.

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I4

CHAPTER 9

PROJECT 6.4a: WATER-WAVE PHOTOGRAPHY

Becaus i of the high energy release anticipated from Mike shot, a water wave was expectedto result from the detonation. In order to study the passage and dimensions of the wave, GroupJ-10 of LASL installed poles, rafts, and b-.,rels at varying water depths and distances fromGround Zero. Eastman 1,1-mm Cine Special cameras, driven by governor-controlled motors,were aimed at these markers frotm four separate stations (Stations 303, 305, 302, and 307) andwere set to run at 12 frames/sec, allowing a total running time of about 10 min. This longrunning time was necessary because of the uncertainty in time of arrival of the water wave atthe different stations and of the exact nature of the phenomena. The cameras were shieldedagainst fall-out radiation by lead boxes as described in Chap. 3.

Three of the cameras recorded the wave motion. The mirror for the fourth camera (Station303) was destroyed by the blast, and the fiim shows nothing of interest. Two of the camerasshowed a slight change in water level and a disturbance of the barrels. The third showed nodisturbance.

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CHAPTER I0

PROJECT 6.14: ROCKET PHOTOGRAPHY

For King Shot t•,e Naval Ordnance Laboratory (NOL) set up a fan-shaped array of smokerockets on the shot island, so positioned that the fireball would ippear in front of the rockettrails.

Three 35-mm Mitchell cameras running at approximately 100 frames/sec and equippedwith 2-cycle velocity markers were operated from Station 306 on Rojoa. Two of these camerasoporated satisfactorily, one giving an excellent record of hooks :n the trails. The third cameradid not run owing to damage caused by the heavy rains previous to shot day. Original negatives

were turned over to NOL for analysis.Space reference markers, which had been requested by NOL, were not installed because

the high level of radioactivity at the photostations following Mike shot severely limited thenumber of man-hours that could be spent on this project.

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CHAPTER 11

PROJECT 10.1: TELEVISION AND WORLD TIME

Two Eastman Cine Special cameras mounted on fixed pediestals recorded the televisionmonitor screen on the USS Estes from M-1 hr to Mike zero, taking two pictures per secondfrom M-60 min to M-2 min. then eight per second until the explosion destroyed the trans-mitter in the zero station. Figure 11.1 shows the tolevision monitor panel and a typical filmrecord of the television screen.

The world-time rack was installed in the control room aboard the USS Estes for Mikeshot, Fig. 11.2, and in the Elmer Control Point (CP) for King shot. This rack was equippedwith a short-wave receiver for picking up WWV time signals and contained two clock panels,one indicating the hour, minute, and second 'nd the other indicating seconds and hundredthsof seconds. These clocks were each photographed by an EG&G scope camera. A Blue Boxcaused a flash tube to discharge at shot time and record images of the clock faces. In orderto calibrate the clocks , pictures were taken before and after the shot, the flash discharge inthese cases being controlled by WWVY. The necessary correction factors were determined bymeand of these calibration picttres.

Both cameras operated satisfactorily on Mike shot. The records are shown in Fig. 11.3,the middle image being the shot pi'.ture in both cases. The corrected clock reading is 07: 14:59.225. However, owing to a power failuie aboard ship at M-,40 min, the operation of the clockdriving circuits was unstable, and it ei thought that the world-time reading is uncertain byAO.2 sec.

The datermbiation for King shot was unsuccessful because the Blue Box did not trigger.A manually operated stop watch show-rs the burst to have occurred within 2 sec of target time(11:30).

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CP

50

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Im

Fig. 11.2-World-time photography installrtion.

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IlI~z-1x

Z0

520

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-TTA PrrR 12

MISCELLANEOUS

12.1 GMX-9 MODEL 7 CAMERA

One of these ultra high speed cameras was used on Mike shot and two on King shot. Thesecond King shot camera was loaded with Eastman Color Negative film in an effort to recordvery high speed photographs of the fireball in color. The cameras were run in series with aHeiland recorder which traced the spoed of camera rotation on a strip of tape. Markers attwo different frequencies (110 and 200 cycles) were employed as a check on each other and toguarantee a time scale for the films.

The GMX-9 Model 7 camera is an experimental high-speed camera developed at LASL.The image formed by the primary optical system is formed on the surface of a rotating mirrorwhich sweeps the light across a second bank of lenses, each one of which forms an image forone position of the mirror. A blast-wave capping shutter is used to prevent recycling or multi-ple exposures. The speed of the mirror can be adjusted so as to attain a maximum picture-taking rate of 90,000 frames/see.

Satisfactory records were obtained from the GMX camera on Mike shot only. A sampleframe from this record is presented in Fig. 12.1.

12.2 IMAGE-CONVERTER CAMERA

One experimental image-converter camera was set up in the Elmer tower (Station 301) forMike shot. In this arrangement the image- converter tube acts as a photographic shutter. Theimage-converter tube takes an optical image, converts it to an Plectron image, and, by means ofphosphors, reconverts the image into an optical image which can be photographed. During theconversion process the intensity of the original image can ba increased several times. This isa great advantage cver standard optical systems, where only a reduction in light intensity iSpossible as the image passes through various lenses. W.th this system it is also possible toattain extremely short exposure times by placing a positive potential on the anode of the tubeior the desired time. This causes the electrons to flow toward the anode, with consequent con-version of the electron image to an optical image.

The operation of this type of camera is described in detail elsewhere.' In this installp"•nthe tube and associated power supply were operated using a 72-in. -focal-length Newtonian Lypetelescope lens as the field lens. This was mounted (see Fig. 12.2) beside the tube and camera

assembly, with a mirror arranged so as to direct the Newtonian image to the image-convertertube. Because of the extremely high light levels expected from a blast the size of Mike, it wasnecessary to use several types of shutters to guarantee that no fogging of the film resulted afterthe picture had been exposed. One of these was a Rapatronic type 1-gsec shutter which wasplaced between the camera and the tube. A second setup used a wire positioned between two

53

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Fig.1. - M -a arcrMk ht

54

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II,It

~c

4)l

55

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(a)

(b)

Fig. 12.3-Teletronic image, Mike shlot. (a) Prezera. (b) Postzero.

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piecs o glss.An lecricl plsethrough the wire caused the glass to break and craze, thus

effctielyblokin th pasag oflight throuigh the glass. A mechanical shutter was alsoplaed exttothelen o th scpecamera. The first two, combined with the natural shuttereffct i te iageconertr tbewere required to assure that the light was cut off immediately

aftr te dsird eposre.Thethird, a slower mechanical type, operated to be sure that noleaingof igh ocured etwenexposure time and time of recovery of the film.

Becase f te unertint inthe expected light level, it was decided to use an ND-2 filterin front c" the lens to make sure the bomb light would not burn an image into the tube. Un-fortunately, this gues., resulted in too heavy filtering, so that no image appeared on the film.Operation of the equipment components was completeiy satisfactory, however, and the heavyfiltering was believed to be the only reason why no picture w;3s obtained.

12.3 TELETARONIC CAMERA

An experimental camera similar in operation to the Rapatronic and equipped with a 160-in. -focal-length Cassegrainian type telescope lens was installed in the bunker at Station 300 for useon Mike shot. Similar camneras had been successfully employed on previous operations to re-cord detail of action iii the cab at the instant of detonation. A special 1-Ajsec. shutter, used inplace of the conventional Rapatronic shutter, was required because of the extremely high speedwith which such early visible reactions take place. Camera operation was completely satisfac-tory. The resulting photograph, taken at approximately 51 Asec after zero, appears in Fig. 12.3.

Because of the uncertainty in burst time and location for King shot, no attempt was made torecord data with the Tele'tronic camera.

REFERENCE

1. N'-vOrd Report 1311, HighL Speed Photography with the 1P25A Image Converter Tube, NavalOrdnance Laboratory, White Oak, Md., Nov. 23, 1951.

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I

APPENDIX A

BLOCK DIAGRAMS OF PHOTOSTATIONS

4

59-60ER

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RAC PAEL. fCOTAC} ......~LiIIIr -C CONIAC IOR RP'K PANELl1

PA 0CK NANEL FcýCONTACTS A VM NO k NO 6 CONTACTS QT a 24V D-C

12"R-16 NO. 2 C0.T&ACTS +155S O T 04ATT IE

DA CIEST -153 15S TWINDOW

TOA ET2 0-CI: 2-TATO El D N-t- OI CA CONTACT T4

CFRE ZIINO.4CONTACTSI2ATTER -ES

0- ~ -C CONTACTORi SO -3CI - OTCO A OTC BATTERIES

NO 5 CONTACTS -'G 3 O OTCS N.S4NLLAN SIPE

0-CALE COCCOONTACTSOL A CNAT AK AE

0" -C CONTACTOR 0l C AMCA CNTCTIIER O

ARGER~~~~~- CONTACTORT 5 ........

J E C D N T A CN

O.R C O N T A C TSD

C- C-.5s.~~SFE SWsC SGA

5-5 - ONTACTOR D 4 WINDAT11OW . q!ATRC AE

ATRESNRCONTACTS ID2CI 15N 1 0

CAM ONTCT -C CONTýACTOR 0-C CNACTO

NO ~ ~ _ LT / O1 OTCS NO, 10 OIOPNSPIM-153 +15S OTO

SECRET RESNTRICT ED D T

ON-1- 3 OONCT-AE N0ST/

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D-C CONTACTOR RACK PANEL2'- VM NOI t NO 6 ( ONTACTS IT2 a~ 20 -C

L -- 15S .isS DIST

SAFETY SW

FN-'- COHv IL fCAM CONTACT TIT

tB [,A BýATTEI2.ES

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CONTACT3 CAML CONTACT 5V Go--tS S +35 O ONAT NOL ST4 N/C ISLAND SUPPLY

.AL _IS +3S OPEN +SS

0NI- COL CAM CONTACT- 15S +45S1 NO ST5 AKPNLj ______ 0-V

NAL~~~~~1 -i - IS 0 IAMVENTS01ST -ISM +3S

[ -C CAM CAM CONACTrSHORT TIMER NO 2T0 2 O-VN~

ON- 1-2 -4COTCSA-C SAFETY CONTIA-TS ý20:0 VM El

-ISS +ISS CONTACTTS E3 ATA

- 1VELOCITY0- CMCAM CONTACT JMARKER

MOTOR 070S CONVERTER NOT2 PLATES128V 0C--ES

CAM CONITACTNo LTI0-COTTR

+3-5$ +3SM

DH Il-I 0CCOACP0,_ -C CONTACSNIOL

0-C CONKTACTORr2- VM NO 3 NO,.= COTACTS-15 +IS 1S a-E

IIATEERIES

CNlARGER

1155 -60--ISLAAC SUPPLY

0- OTAILTOR- NO 10 CCIL

I-1SS tLMJ

Fig. A.1-lnotograp. installation, Janet, Mike s1.0-

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RACK PANE 12ý8V - CTATR-M' 71 2 VMA NOIO-c oIST i24V i OICNAT

12-24- 28V '28V -S58MI IN Ojljý

2- VM NO 2

2 PO 2 POE --- M2 WýINOOW

128V ON-I4-I I28V -CNTTR

8 -46V 1V CONTACTS N OL4V -5S +58S

CHARGER 9 5S+8

CAM CNTACT _24V 0-C CAM24V NO STI 90S TIMER

24v 0-C COTATAMST2 ~ 300M TýIMER

0+60S 1L MOTOR

2VCAM CONTACTNC LTf

4305 +30M.

02V 0C CONTACTOR ECNJ28V NO 3 CONTACTS

+9m +26MEK CINEI

C 2 1IAM 7CONTACT 0- C COýNTACTORI2BV NO LT2 - NCO 3 COIL

_tgM *'261M +9M +26m

Fig. A .2 -Photographic installation, Yvonne, Mike shot.

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428V T28 J- 24VATO MICCNAC24 VM NO8 NO CONTACTSCTS2

52 -S +58S _ M- WINDOW -S+8

2 POLE M--- ,2-WIND'O W-F2 MN2ETY SW

428V ON-I4-t 128V 0-C CONTACTORI128V CONTACTS NOICI 4 AM CONTACT4V _S +5S N I CIL 2V CNO ST3-55+58 *.5S +58S -3S +58S

r- CONTACTO 1SO -I1- COILIV -5S 5++88

FCAM CON' ACT, 24V 0-cC CAM24VL NO ST I 9OS TIMER

-3S +85S 24V] MOTOR

24V CAM CONTAC 0- AMNO ST2 ___ 30.1 TIMER0+460S MOTOR!L

2g4V CAM CONTACTNO LTI

+30r +30M

I2V0C CONTACTOR ECN

428V CAM CONTACT 0i-C- CONTACTOR1NO LT2 -1 NO 3 COIL

+9i-M +26M j _+9M +26M_

Fig. A.2 -Photographic installation,, Yvonne, Mike shot.

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PANEL E* R- ACK PANEL CM CONTACT3N 200 1 3 a 4W - SAEY24V/0-C NO ST4

T1N 5v01/ , SIC OIST_ -7S .45STON

SAFETY SWITCHU SE AS JUNLTION A-C CONTACTORS NO 7,Z,9,4O 11CACOTACTBOX0 OLY FOR CONTACTS NO S5524V 0-NC 2 NO 2 -155 .2S 0 -7S 445S

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01 T -i5M +455 PANEL --- 1

A-C CONTACTOS 5 1151 -v M1 ON-Il-3NO 3 CONTACTS tCON-ACTS

El -O F37S f75S'

A-C CONTACTOR CAM CONTACT1

NO 'CONTACTS 200 0~N ST6-lAS +45S PAE 40 +7C5

M11 CA" CONTACTNO AT

+5OS .' 30SM2

POWER SYSTEM

_i5M FILAMENTS

100- 1/M j ~1 53 R

NO Ii CORL

II 612345611f

A-C COTACTOSFMI 4

0!v 1 0CAM CONTACT A-C CONTACTOR A-C CONTACTOr -4 3 200 2 2100NO0 ATý2S 5 N CONTACTS NO 2 COIL ,-rO3MG-034 V 4

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ICION I

CAM CONTACT A-C CONTACTOR A-C CONTACTOR SI MI

-7S +5S -455Ss+AS -15S +5S_ P

CAM CNTACTA-C CIINTACTOSNO ST8NO 6 COIL A-C CONTACTO

-SOS~l2A+90SS +125S NO OR TAT-45 N. +45SPANEL "C

A-C~~~~ ~ COTCO A-TOTAASCIT 8NO 2 OCON TACTSNO7CI A-C CONTACiTfl-lAS +25-IS -O NO 6CONTACTS~

+ ,OS +-lOSS

A-C CON TACTONO COIL-5S 42S

A-C CONTACTORNO 9 COIL-15S 2SA

LA-C CONTACTORL NO 10 COIL

-15S .2S

Fig. A.3- Photographic installation, Elmer tower Mike and King shots.

63

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TY

CONACTrS PANEL , CAM CONTACT c0_

-?S.45

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200- VIAAFILAMENTS

4F'124506 423456

A-C CONTACTOR FMIl FMUSMNO5

ACT A-C CONTACTOR A-tOTATR2 200- 2 I 2 '00O-2 NO 2CONTACTS NOCOL03 VM 3 03 VIA

S-15S 42S oIA+2 4 40 04

TS S M2Is

S

ACT F - OTCO -C COTATONO 30 N N COIL

S 5S+5S-15S+55PULSE SYSTEM

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-4S45

ACT fT~ CONTA.1CTOR ________ _________8 ~~~NOA C OILCOATO

I 0 I45 A-C CONTCTR OPE' NO 5 CONTACTS CONTACTSN

PANEL C 000+4SH _8ONAT

CTOR A-C CO'NTACTOR I 4S 78 MOTORACTS ISAL A AC CONTACTOR

SNO0A CONTACTS CNTACTOSE

I8 S AC055A-C (ONTACTOR

NO 8 OIL

-15S +2SDOOR SYSTEM

A-i.LIIIC

-I5S +2S

NO IC COIL

Fig. A. 3-Photographic installation, Elmer tower, Mike and King snsots.

63

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RACK PANEL 0-C COTCO 0~ V 0-MNLOI -CCMON-Il-2 RACK 0

ANIEL

lABO-Cu -~s A~ 00- VMOI HOR TIERCONTACTS 24V 0-C

01ST 5 AS*sE OO IS +'S 01S TK -I5S +5S

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SAFETY SW M-5 I SS M - S . AEYSK -5S +5S -7S +755

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+S1.30S ,30. HRECHARGER M -IS lA -2S IAIS * 2 5IISS 21 f ONLY

CONTACTS N4COLLONC TIME No LT "ARDrC Ir.11r SLN SUPPLY

CONACS N S COIL CDM CONACM IS +SE M -55 -OM

-E1 S +SS K 15+5S

ý.'TAC F 7C RPA N

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IM NO I- D CMDN-II-2 RACPNESOTTMRCONTACTS 24,' 0-C

NO CAMCON'TAACTTF

SAFETYS

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L A- CONACTO NO MIA-C CONTACTOR NO 5 24V RC AERCPAECOTCSCONTACTS RAC PaNEL O

2 VM NO5 +9 M-15S+.56 M. 30S 12V DISTDISTK- 5S+ 55S WIDOWK-IS5 S +29 M

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CAM CONýTACýTq NO 4I- O TA T R NU-S+8. 30 Ci

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RACK PAN"L 0-C CONTACTOR MI - ~ VM - -- C-0 CONTACIORL

2,2 NOICONTACTS NO V 12I SNa TIME O_ COTAT

.CC CDNTCTT 502 COIL

OCDSS.4MIWNDOWCI 5lO .4$ST NTST

S AF I S8-16VV~~0- CONTACTACORO -~5 SIGNAL 2 212

BATTERIES ~ ~ ~ N 4 COILTCS O3 TERE.41-15 M3 WNDO

15 V NOOCONTACTS

O N-CO ATO MR - A -C0TCO 4BATRE OCONTACTS 01TIENO3C TAS

TO5 .4S OORNO 15V+5

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APPENDIX B

FILM COMPOSITION AND DISPOSITION

The various films from this operation were assembled by subject matter into reels up to400 ft in length. Composition of these reels is shown in detail in Tables B.1 and B.2. Projec-tion prints were made from all reels, and copies were issued as follows: three copies, J-Divi-sion, LASL; two copies, Chief, Armed Forces Special Weapons Project, Washington, D. C.; twocopies, EG&G, Boston; one copy, EG&G, Las Vegas. One additional copy of the King rocket reelwas also sent to NOL, Washington, D. C.

Fine-grain master positive copies and prints .f the Ivy records were sent to the Air ForceLookout Mountain Laboratory to make tinted Kodachrome master footage for the Ivy documen-tary.

67

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Table B.1-MIKE RELEASE-PRINT ASSEMBLIES

Focallength Distance

Perforation Nominal of lens, Camera from zero,Reel No. frames/sec mm station miles Direction

Fireball 16,125 100 152 EE-J01 22 SE16,109 Z5000 102 J-303 3.7 E16,108 3000 102 J-303 3.7 E16,107 3000 102 J-303 3.7 E16,111 3000 25 J-303 3.7 E16,110 3000 25 J-303 3.7 E16,103 3000 102 EE-302 22 SE16,101 3000 102 EE-302 22 SE16,102 3000 102 EE-302 22 SE

1,- 00G 102 EE-302 22 SE19,112 1000 102 Ship -30

Mass motion 16,171 70 100 U-306 10.1 E16,172 70 152 U-306 10.1 E16,173 70 152 U-306 10.1 E16,174 70 152 U-306 10.1 E16,175 70 152 U-306 10.1 E16,176 70 75 J-303 3.7 E16,178 70 75 J-303 3.7 E16,179 70 75 J-303 3.7 E16,180 70 152 U-306 10.1 E16,181 70 152 U-306 10.1 E16,182 70 152 U-306 10.1 E16,184 70 152 Y-307 13.2 SE

Cloud stem 16,125 100 152 EE-301 22 SE16,119 /2 18.5 EE-308 22 SE

Timing 16,117 2-8 15 Shiprecord, television 16,118 2-8 15 Ship

Water-wave motion 16,114 12 25 U-306 10.1 E16,115 12 25 Y-307 13.2 E16,116 12 25 EE-308 22 SE

Table B.2--KING RELEASE-PRINT ASSEMBLIES

Focallength Distance

Perforation Nominal of lens, Camera from zero,Reel No. frames/sec mm station miles Direction

Fireball 16,201 3000 102 EE-302 10.4 S16,204 3000 102 EE-302 10.4 S16,205 3000 102 EE-302 10.4 S

Mass motion 16,276 100 152 U-303 4 N16,277 100 152 U-306 4 N16,278 100 152 U-306 4 N16,279 100 152 U-306 4 N16,294 600 102 Y-307 1.5 S

Shock velocity (rockets) 16,293 100 102 U-306 4 N16,291 100 35 U-306 4

68

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APPENDIX C

METEOROLOGICAL DATA

Table C.1 -METEOROLOGICAL CONDITIONS, OPERATION IVY

Air

Pressure, Temperature, RC lelative density,Shot Date Local time in. Hg Dry bulb Wet bulb humidity, % g/liter

Mike 11/1/52 0714:59.4 ± 0.2 sec 29.79 29.4 24.2 64 1.118*King 11/16/52 1130:00 • 2 sec 29.84 29.4 26.6 80 1.109t

*At ce3nter of gravity of fireball.

tAt burst height.

69-70

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APPENDJX D

CAMERA DATA SHEETS

71-72

SECA ET- RESTRICTED DATA

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EDGERTON, GERMESHAIJSEN a GRIER, INC. GAMERA DATA SHEET

PEA R LR V~ WE R TEST~4ZdDAT E Ah-kka STA . -UP-2LREMARKS 8 NOTES CAMERA TIME -- FNS4

S'~v FR45EC. NO. SERIAL IMAG. OPER. IFOC. LGH.~ SERIAL

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EDGERTON, GERMESHAUSEN 8 GRIERJINC. CAMERA DATA SHEET

p' xy E t.TEST I~QŽLty- DATEuf'ijazSTA. 0,U

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EDGERTON, GCtRMESHAUSEN a GRIER, INC. CAMERA DATA SHEET

TEST1lf-d DAVE ,-/-5.. STA. ,Lt_3 Vor

REMARKS & NOTES CAMERA TIME LENS" •/.k, o, &mjgFR.lSEC. SO. SERIAL MA. OPER. FO. Oc.L. SERIAL

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EDGERTON,GERMESHAUSEN a GRIERJINC. CAMERA DATA SHEETRy 6-ND.TEST W'vY-M DATE LLLŽ3~STA.30AIW

___ ___ ___ __ 7-1'-V ,-P *4 .3to..ZPERF. EMULSIFILTERS JAPER. AIMING POWER TIMING MARKERS, SERIALSIRACK ýýAM

CODE IND lCOLOR SET. ONRIZOFFRTFM.______ ON OFF VLZEROPO0.

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EDGERTON, GERMESHAUSEN a GRIER, INC. CAMERA DATA SHEETTEST.X.;L- DATE__ STA. 103

REMARKS 8 NOTES GAMERA ___TIME LENS- E N . E IA L A G. O R . FO . LG H . S

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EDGERTON, GF-RMESHAUSENaBGRIERINC. CAMERA DATA SHEET

E~vc--,olT E STryp&m D A TE LAS TA. AVL

PERF. EMULS FILTERS APER. AIMING POWER -TIMING IMARKERS,SERIALSIRACK CAM

CODE ___N7 COLOR' SET. OI ET ON OFF FM. VEL IZERO POS. NO.

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EDGERTON, GERMESHAUSEN a GRIER, INC. CAMERA DATA SHEETRoJ-oA TESTZv./. DATE 11-1-5Z STA. ZQ4,W

REMARKS a NOTES CAMERA TIME LENS

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EDGERTON,GERMESNAUSEN 3 GRIERINC. CAMERA DATA SHEETTEST _.IvtidýATE A1~4,47 STA.

PERF. EMULS FILTE",RS APER. AIMING POWER TI1M ING MARKERS.SERIALS RACK CAM

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EDGERTON, GERMESHAUSEN B GRIER, INC. CAMERA DATA SHEET

RoNO E r TEST vy_-. , DATE 1-- 5-'s' STA. $07

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Ev FR.JSEC. NO. SERIAL MAG. OPER. FOG.LGH. SERIAL

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EDGERTON,GERMESHAUSEN a GRIERINC. CAMERA DATA SHEET

R•LNIr TESTZVXAIIK DATE //-/-S-STA. 3.07

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EDGERTON, GERMESHAUSEN a GRIER, INC. CAMERA DATA SHEETTESTly--A DATE-nIiI"2 STA.Mc.

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EDGERTON, GERMESHAUSEN a GRIERINC. CAMERA DATA SHEET-t 5 TZ5 TEST14ny -?fhJDATEý ",S;L STA. E-s/a S

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EDGERTON, GERMESHAUSEN B GRIER, INC. CAMERA DATA SHEET

REMARKS 8 NOTES C GAMERA TEST!IME | LENS

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EDGERTON, GERMESHAUSEN a GRIERJlNC. CAMERA DATA SHEET

CUeRT/S5 TEST l X DATE k STA. L&6L

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0"GERTON, GERMESHAUSEN a GRIER, INC. CAMERA DATA SHEET

~,P~I~FrTES1IýL- DA-(F- iJ,/6L;STA.4eA16."REMARKS 8 PNOTES CAMERA TIME LENS

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EDGERTON, GERMESHAUSEN a GRIER, INC. CAMERA DATA SHEETP~q~yroERTEST~vy-Kd DATE a-6 - STA. 30

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EDGERTON,GERMESHAUSEN a GRIERJINC. CAMERA DATA SHEET

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EDGERTON, GERMESHAUSEN & GRIER, INC. CAMERA DATA SHEETTESTIlq--X DATE 1-16 STA. .302of_30,PA4RRY &IVD.

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EDGERTON, GERMESHAUSEN 8 GRIEP. INC. CAMERA DATA SHEET

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