Weapons-Test Connection by Roger C
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Bob Farquhar
1 2 Created by Bob Farquhar For and dedicated to my grandchildren, their children, and all humanity. This is Copyright material 3 Table of Contents Preface 4 Conclusions 6 Gadget 8 Making Bombs Tick 15 ‘Little Boy’ 25 ‘Fat Man’ 40 Effectiveness 49 Death By Radiation 52 Crossroads 55 Atomic Bomb Targets 66 Acheson–Lilienthal Report & Baruch Plan 68 The Tests 71 Guinea Pigs 92 Atomic Animals 96 Downwinders 100 The H-Bomb 109 Nukes in Space 119 Going Underground 124 Leaks and Vents 132 Turning Swords Into Plowshares 135 Nuclear Detonations by Other Countries 147 Cessation of Testing 159 Building Bombs 161 Delivering Bombs 178 Strategic Bombers 181 Nuclear Capable Tactical Aircraft 188 Missiles and MIRV’s 193 Naval Delivery 211 Stand-Off & Cruise Missiles 219 U.S. Nuclear Arsenal 229 Enduring Stockpile 246 Nuclear Treaties 251 Duck and Cover 255 Let’s Nuke Des Moines! 265 Conclusion 270 Lest We Forget 274 The Beginning or The End? 280 Update: 7/1/12 Copyright © 2012 rbf 4 Preface 5 Hey there, I’m Ralph. That’s my dog Spot over there. Welcome to the not-so-wonderful world of nuclear weaponry. This book is a journey from 1945 when the first atomic bomb was detonated in the New Mexico desert to where we are today. It’s an interesting and sometimes bizarre journey. It can also be horribly frightening. Today, there are enough nuclear weapons to destroy the civilized world several times over. Over 23,000. “Enough to make the rubble bounce,” Winston Churchill said. The United States alone has over 10,000 warheads in what’s called the ‘enduring stockpile.’ In my time, we took care of things Mano-a-Mano. -
Jacques Tiziou Space Collection
Jacques Tiziou Space Collection Isaac Middleton and Melissa A. N. Keiser 2019 National Air and Space Museum Archives 14390 Air & Space Museum Parkway Chantilly, VA 20151 [email protected] https://airandspace.si.edu/archives Table of Contents Collection Overview ........................................................................................................ 1 Administrative Information .............................................................................................. 1 Biographical / Historical.................................................................................................... 1 Scope and Contents........................................................................................................ 2 Arrangement..................................................................................................................... 2 Names and Subjects ...................................................................................................... 2 Container Listing ............................................................................................................. 4 Series : Files, (bulk 1960-2011)............................................................................... 4 Series : Photography, (bulk 1960-2011)................................................................. 25 Jacques Tiziou Space Collection NASM.2018.0078 Collection Overview Repository: National Air and Space Museum Archives Title: Jacques Tiziou Space Collection Identifier: NASM.2018.0078 Date: (bulk 1960s through -
National Reconnaissance Office Review and Redaction Guide
NRO Approved for Release 16 Dec 2010 —Tep-nm.T7ymqtmthitmemf- (u) National Reconnaissance Office Review and Redaction Guide For Automatic Declassification Of 25-Year-Old Information Version 1.0 2008 Edition Approved: Scott F. Large Director DECL ON: 25x1, 20590201 DRV FROM: NRO Classification Guide 6.0, 20 May 2005 NRO Approved for Release 16 Dec 2010 (U) Table of Contents (U) Preface (U) Background 1 (U) General Methodology 2 (U) File Series Exemptions 4 (U) Continued Exemption from Declassification 4 1. (U) Reveal Information that Involves the Application of Intelligence Sources and Methods (25X1) 6 1.1 (U) Document Administration 7 1.2 (U) About the National Reconnaissance Program (NRP) 10 1.2.1 (U) Fact of Satellite Reconnaissance 10 1.2.2 (U) National Reconnaissance Program Information 12 1.2.3 (U) Organizational Relationships 16 1.2.3.1. (U) SAF/SS 16 1.2.3.2. (U) SAF/SP (Program A) 18 1.2.3.3. (U) CIA (Program B) 18 1.2.3.4. (U) Navy (Program C) 19 1.2.3.5. (U) CIA/Air Force (Program D) 19 1.2.3.6. (U) Defense Recon Support Program (DRSP/DSRP) 19 1.3 (U) Satellite Imagery (IMINT) Systems 21 1.3.1 (U) Imagery System Information 21 1.3.2 (U) Non-Operational IMINT Systems 25 1.3.3 (U) Current and Future IMINT Operational Systems 32 1.3.4 (U) Meteorological Forecasting 33 1.3.5 (U) IMINT System Ground Operations 34 1.4 (U) Signals Intelligence (SIGINT) Systems 36 1.4.1 (U) Signals Intelligence System Information 36 1.4.2 (U) Non-Operational SIGINT Systems 38 1.4.3 (U) Current and Future SIGINT Operational Systems 40 1.4.4 (U) SIGINT -
Records of Prime Contracts Awarded by the Military Services And
""" "II" n "'1"1""" National Archives and Records Adlninistration 8601 Adelphi Road College Park, Maryland 2fJUO-6tJOl List ofDcicumentation Military Prime CQntractFile. 1966-1975 Records of the Office ofthe Secretary ofDefense, Record Group 330 Accession Number: NN1-330-79-003 I. Basic Documentation 1. List ofDocumentation 1 2. tis! ofProourement Manuals (prepared 1995) 1 3. User Note 1 1 4. Abstract (prepared 1988) 1 5. rntroduction (prepared 1988) 2 6. NARA prepared record layout (April 200 1) :3 7. Valjdatl'on Statement (prepared 1988) 2 8. User Note 2 1 9. Agency prepared record layouts (prepared 1970) 3 10. UserNote3 1 11. DD Form 350J i 97 t (source for MPCf) 1 12. Agency description ofDD Form 350 . 1 13. Agency description of ><FlXS" data variable t II. Additional Documentation L NARA Magnetic Tape Record Inventory (January 19(2) 3 2. NARAMagnetic Tape Record lnllentoty (February 1972) 3 3. DcpaIimcnt ofDefense Publil,:aiions 4. MPCF Procurement Coding Manual. FY 1966 59 5. MPCF Procurement Codlng Manual. FY 1967 65 6. MPCF Procurement Coding Manual, FY 1968 68 7. MPCF Procurement Coding Manual, FY 1969 73 8. MPCF Procurement Coding Manual, FY 1970 78 9, MPCF Procurement Coding Manual, FY 1971 81 10. MPCf Procurement Coding Manual, FY 1972 89 11. MPCF Procurement Coding Manual, FY 1913 101 12. MPCF Procurement Coding Manual, FY 1974 79 13, MPCF Procurement Coding Manual, FY 1975 80 m. Processing Materials 1. AERie Verification Reports 2. NARA Sample Dumps (prepared 1988) 3. Agency SampleDurnps (1966-1975) William P. Fischer April 22. 2002 NARA Reference Copy Page # 1 Me. -
1. State of the Magnetosphere
VOL. 78, NO. 16 3OURNAL OF GEOPHYSICAL RESEARCH 3UNE 1, 1973 SatelliteStudies of MagnetosphericSubstorms on August15, 1968 1. Stateof the Magnetosphere R. L. M CPHERRON Department o] Planetary and SpaceScience and Institute o] Geophysicsand Planetary Physics University o] California, Los Angeles,California 90024 The sequenceof eventsoccurring throughou.t the magnetosphereduring a substormhas not been precisely determined. This paper introduces a collection.of papers that attempts to establish this sequencefor two substormson August 15, 1968. Data from a wide variety of sourcesare used, the major emphasisbeing changesin the magnetic field. In this paper we use ground magnetograms to determine the onset times of two substorms that occurred while the Ogo 5 satellite was inbound on the midnight meridian through the cusp region of the geomagnetictail (the region of rapid changefrom taillike to dipolar field). We concludethat at least two worldwide substormexpansions were precededby growth phases.Probable begin- nings of these phaseswere at 0330 and 0640 UT. However, the onset of the former growth phase was partially obscuredby the effects of a preceding expansionphase around 0220 and a possible localized event in the auroral zone near 0320 UT. The onsets of the cor- respondingexpansion phases were 0430 and 0714 UT. Further support for these determina- tions is provided by data discussedin the subsequentnotes. The precise sequenceof events that occurs Ogo 5 in the near tail, and ATS I at syn- during a magnetosphericsubstorm has not been chronousorbit. Solar wind plasma parameters established.Among the reasons for this are were measured by Vela 4A. Magnetospheric lack of consistencyin the definition of sub- convection is inferred from a combination of storm onset and the wide variability of suc- plasmapauseobservations on Ogo 4 and 5 in cessivesubstorms. -
The 22 September 1979 Vela Incident—Part II: Radionu- Clide and Hydroacoustic Evidence for a Nuclear Explosion”
SCIENCE & GLOBAL SECURITY ,VOL.,NO.,– https://doi.org/./.. The September Vela Incident: The Detected Double-Flash Christopher M. Wrighta and Lars-Erik De Geer b aUNSW Canberra, School of Physical, Environmental and Mathematical Sciences, Research Group on Science & Security, The Australian Defence Force Academy, Canberra BC, Australia; b(Retired) FOI, Swedish Defense Research Agency, and the Preparatory Commission for the Comprehensive Nuclear-Test-Ban Treaty Organisation, Flädervägen , Upplands Väsby, Sweden ABSTRACT ARTICLE HISTORY On 22 September 1979 two optical sensors on U.S. satellite Vela Received March 6911 detected a double-flash of light that appeared characteristic Accepted October of an atmospheric nuclear explosion conducted over the south- ern Atlantic or Indian Ocean. It became known as the Vela Inci- dent, Event 747, or Alert 747. An anomaly between the amplitude of the two signals during the second pulse led a U.S. govern- ment expert panel established to assess the event to conclude in mid-1980 that a more likely explanation was the impact of a small meteoroid on the satellite, the debris from which reflected sunlight into the sensors’ field of view. No model was presented to support the contention, and a similar anomaly—known as background modulation—was a given for the second pulse of all confirmed explosions detected by Vela, though beginning later. Nonetheless, this event has remained the subject of intense debate. This article reviews the evidence and presents an updated analysis of the original Vela signal based on recently declassi- fied literature and on modern knowledge of interplanetary dust and hyper velocity impact. Given the geometry of the satellite, and that the bulk of the surface comprised solar panels, much of the debris from any collision would be carried away from the sensors’ field of view. -
Polychromatic View of Intergalactic Star Formation in NGC 5291
A&A 467, 93–106 (2007) Astronomy DOI: 10.1051/0004-6361:20066692 & c ESO 2007 Astrophysics Polychromatic view of intergalactic star formation in NGC 5291 M. Boquien1,2, P.-A. Duc1, J. Braine3, E. Brinks4, U. Lisenfeld5, and V. Charmandaris6,7,8 1 Laboratoire AIM, CEA, CNRS et Université Paris Diderot 2 CEA-Saclay, DSM/DAPNIA/Service d’Astrophysique, 91191 Gif-sur-Yvette Cedex, France e-mail: [email protected] 3 Observatoire de Bordeaux, UMR 5804, CNRS/INSU, BP 89, 33270 Floirac, France 4 Centre for Astrophysics Research, University of Hertfordshire, College Lane, Hatfield AL10 9AB, UK 5 Dept. de Física Teórica y del Cosmos, Universidad de Granada, Granada, Spain 6 Department of Physics, University of Crete, 71003 Heraklion, Greece 7 IESL/Foundation for Research and Technology, Hellas, 71110 Heraklion, Greece 8 Chercheur Associé, Observatoire de Paris, 75014 Paris, France Received 3 November 2006 / Accepted 18 February 2007 ABSTRACT Context. Star formation (SF) takes place in unusual places such as way out in the intergalactic medium out of material expelled from parent galaxies. Aims. Whether SF proceeds in this specific environment in a similar way than in galactic disks is the question we wish to answer. Particularly, we address the reliability of ultraviolet, Hα and mid-infrared as tracers of SF in the intergalactic medium. Methods. We have carried out a multiwavelength analysis of the interacting system NGC 5291, which is remarkable for its extended HI ring hosting numerous intergalactic HII regions. We combined new ultraviolet (GALEX) observations with archival Hα,8µm (Spitzer Space Telescope) and HI (VLA B-array) images of the system. -
Eyes for Gamma Rays” Though the Major Peaks Suggest a Periodic- Whether These Are Truly Gamma-Ray Bursts for a Description of This System)
sion of regularity and slow evolution in the They suggested that examination of the Vela exe-atmospheric nuclear detonation. Surpris- universe persisted into the 1960s. data might disclose evidence of bursts of ingly, however, the survey soon revealed that The feeling that transient cosmic events gamma rays at times close to the appearance the gamma-ray instruments on widely sepa- were rare was certainly prevalent in 1959 of supernovae. Such searches were con- rated satellites had sometimes responded when summit meetings were being held be- ducted; however, no distinctive signals were almost identically. Some of these events were tween England, the United States, and found. attributable to solar flare activity. However, Russia to discuss a nuclear test-ban treaty. On the other hand, there was evidence of one particularly distinctive event was dis- One key issue was the ability to detect treaty variability that had been ignored. For exam- covered for which a solar origin seemed violations unambiguously. A leading ple, the earliest x-ray data from small rocket inconsistent. Fortunately, the characteristics proposal for the detection of exo-at- probes and from satellites were often found of this event did not at all resemble those of a mospheric nuclear explosions was the use of to disagree significantly. The quality of the nuclear detonation, and thus the event did satellites with instruments that included de- data, rather than actual variations in the not create concern of a possible test-ban tectors sensitive to the gamma rays emitted sources, was suspected as the reason for treaty violation. by the explosion as well as those emitted these discrepancies. -
Seismographic Study of Mid-Continental Primary Wave Travel Times
A SEISHOGRAPHIC STUDY GOP MID^OHTBENTAL PRIMARY WAVE TRAVEL TIMES by JON FERRELL HOLIES B, S.f Kansas State University, l?6l A Tr^SLS submitted in partial I'ulfillment of the requirements for the degree MASTER OF SCIENCE Department of Geology and Geography KANSAS STATE UNIVERSITY Manhattan, Kansas 196h Approved byt u Major Professor LD WIS TABLE OF CONTENTS INTRODUCTION 1 PROJECT VELA UNIFORM 1 SAINT LOUIS UNIVERSITY SPONSORSHIP k The Role and Location of the Manhattan Station 6 MANHATTAN SEISMOGRAPH STATION 7 Pnysical Plant 7 Operation and Theory 10 SEISMOGRAPHIC STUDY OF MID-CONTINENTAL PRIMARY WAVE TRAVEL TIMES .. 19 Characteristics of Primary Waves 19 Calculations 23 Travel Tines 26 Summary 28 Conclusion APPENDIX I 38 REFERENCES ^ ACKNaYIEDCBOTS I would lilce to express my appreciation for the aid given to me by- Father William Stauder, S.J. in developing the outline of this thesis and his suggestions in the preparation of the text. I am also indebted to Dr. J.R. Chelikowsky for his assistance and guidance with the work on the thesis and in the operation of the seismograph station throughout the past year. • INTRODUCTION A seismograph station was established at Kansas State University by St. Louis University in the fall of 1961, A research assistantship -was granted at Kansas State to initiate seismic studies in addition to operation of the station for St. Louis. The purpose was to create a basic seismic program in the event that the Kansas State Geology Depart- ment takes over full operation of the station. The text of this thesis is divided into two areas, (1) a discussion of the Manhattan Station's development and operation, and (2) basic research on travel times of primary waves in the mict-continent. -
Desind Finding
NATIONAL AIR AND SPACE ARCHIVES Herbert Stephen Desind Collection Accession No. 1997-0014 NASM 9A00657 National Air and Space Museum Smithsonian Institution Washington, DC Brian D. Nicklas © Smithsonian Institution, 2003 NASM Archives Desind Collection 1997-0014 Herbert Stephen Desind Collection 109 Cubic Feet, 305 Boxes Biographical Note Herbert Stephen Desind was a Washington, DC area native born on January 15, 1945, raised in Silver Spring, Maryland and educated at the University of Maryland. He obtained his BA degree in Communications at Maryland in 1967, and began working in the local public schools as a science teacher. At the time of his death, in October 1992, he was a high school teacher and a freelance writer/lecturer on spaceflight. Desind also was an avid model rocketeer, specializing in using the Estes Cineroc, a model rocket with an 8mm movie camera mounted in the nose. To many members of the National Association of Rocketry (NAR), he was known as “Mr. Cineroc.” His extensive requests worldwide for information and photographs of rocketry programs even led to a visit from FBI agents who asked him about the nature of his activities. Mr. Desind used the collection to support his writings in NAR publications, and his building scale model rockets for NAR competitions. Desind also used the material in the classroom, and in promoting model rocket clubs to foster an interest in spaceflight among his students. Desind entered the NASA Teacher in Space program in 1985, but it is not clear how far along his submission rose in the selection process. He was not a semi-finalist, although he had a strong application. -
GASP XXXIII. the Ability of Spatially Resolved Data to Distinguish Among the Different Physical Mechanisms Affecting Galaxies in Low-Density Environments
Draft version April 7, 2021 Typeset using LATEX twocolumn style in AASTeX63 GASP XXXIII. The ability of spatially resolved data to distinguish among the different physical mechanisms affecting galaxies in low-density environments Benedetta Vulcani ,1 Bianca M. Poggianti,1 Alessia Moretti,1 Andrea Franchetto,2, 1 Cecilia Bacchini,1 Sean McGee,3 Yara L. Jaffe,´ 4 Matilde Mingozzi,1, 5 Ariel Werle,1 Neven Tomiciˇ c,´ 1 Jacopo Fritz,6 Daniela Bettoni,1 Anna Wolter,7 and Marco Gullieuszik1 1INAF- Osservatorio astronomico di Padova, Vicolo Osservatorio 5, 35122 Padova, Italy 2Dipartimento di Fisica & Astronomia \Galileo Galilei", Universit`adi Padova, vicolo Osservatorio 3, 35122, Padova, Italy 3University of Birmingham School of Physics and Astronomy, Edgbaston, Birmingham B15 2TT, England 4Instituto de F´ısica y Astronom´ıa,Universidad de Valpara´ıso,Avda. Gran Breta~na1111 Valpara´ıso,Chile 5Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 6Instituto de Radioastronom´ıay Astrof´ısica, UNAM, Campus Morelia, A.P. 3-72, C.P. 58089, Mexico 7INAF- Osservatorio Astronomico di Brera, via Brera 28, I-20121 Milano, Italy (Received July 10, 2020; Revised July 10, 2020; Accepted April 7, 2021) Submitted to ApJ ABSTRACT Galaxies inhabit a wide range of environments and therefore are affected by different physical mech- anisms. Spatially resolved maps combined with the knowledge of the hosting environment are very powerful to classify galaxies by physical process. In the context of the GAs Stripping Phenomena in galaxies (GASP), we present a study of 27 non-cluster galaxies: 24 of them were selected for showing asymmetries and disturbances in the optical morphology, suggestive of gas stripping, three of them are passive galaxies and were included to characterize the final stages of galaxy evolution. -
Intervening Material in Sight-Lines Towards Grbs and Qsos
Programa de Doctorado en F´ısica y Matem´aticas Universidad de Granada Cosmic Lighthouses at High Redshift: Intervening material in sight-lines towards GRBs and QSOs Rub´en S´anchez Ram´ırez Thesis submitted for the degree of Doctor of Philosophy 10 June 2016 Supervisors: Prof. Javier Gorosabel Urkia, Dr. Antonio de Ugarte Postigo, and Prof. Alberto J. Castro Tirado Instituto de Astrof´ısica de Andaluc´ıa Consejo Superior de Investigaciones Cient´ıficas Para todos aquellos que caminaron a mi lado, a´unsin yo mismo entender hacia d´ondeme dirig´ıa... ii In Memoriam Javier Gorosabel Urquia (1969 - 2015) “El polvo de las estrellas se convirti´oun dia en germen de vida. Y de ´elsurgimos nosotros en algun momento. Y asi vivimos, creando y recreando nuestro ambito. Sin descanso. Trabajando pervivimos. Y a esa dura cadena estamos todos atados.” — Izarren Hautsa, Mikel Laboa “La vida son estos momentos que luego se te olvidan”. Esa fue la conclusi´on a la que lleg´oJavier al final de uno de esos fant´asticos d´ıas intensos y maratonianos a los que me ten´ıa acostumbrado. Vi´endolo ahora con perspectiva estaba en lo cierto, porque por m´as que me esfuerce en recordar y explicar lo que era el d´ıa a d´ıa con ´el, no puedo transmitir con justicia lo que realmente fue. La reconstrucci´on de esos momentos es inevitablemente incompleta. Contaros c´omo era Javier como jefe es muy sencillo: ´el nunca se comport´ocomo un jefe conmigo. Nunca orden´o. Siempre me dec´ıa, lleno de orgullo, que no le hac´ıa ni caso.