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Technical Note
NASA TN D-1493 O5 C,/ 1-4 I Q LOAJN' ? < TECHNICAL NOTE D-1493 ENVIRONMENTAL PROBLEMS OF SPACE FLIGHT STRUCTURES H. METEOROID HAZARD Prepared by John R. Davidson and Paul E. Sandorff in collaboration with the NASA Research Advisory Committee on Missile and Space Vehicle Structures Langley Research Center Langley Station, Hampton, Va. NATIONAL AERONAUTICS AND SPACE ADMINISTRATION WASHINGTON January 1963 TECH LIBRARY KAFB, NM Illllllll TABLE OF CONTENTS 0153^57 Page PREFACE li MEMBERS OF THE NASA RESEARCH ADVISORY COMMITTEE ON MISSILE AND SPACE VEHICLE STRUCTURES in SUMMARY 1 INTRODUCTION 1 SYMBOLS -. 2 METEOROID ENVIRONMENT ^ Asteroidal Particles ; . k Cometary Particles 5 Tektites 8 Pertubation Forces 9 Observations of Meteors From the Earth 10 Satellites and Space Probes 15 Research in Progress 18 INTERACTION BETWEEN METEOROID ENVIRONMENT AND STRUCTURE 19 Historical Aspects of the Plate Perforation Problem 19 Physical Description of High-Speed Impact Phenomena 20 Modern Theories of Penetration 22 Experimental Data .__ 26 PROTECTION METHODS 30 Types of Structural Damage 30 Application of Meteoroid Flux Data and Impact Data to Design Problems 30 RESEARCH IN PROGRESS 36 Ground Research 36 Flight Test Research 36 RECOMMENDED METEOROID RESEARCH PROGRAM 36 REFERENCES kO BIBLIOGRAPHY 1*7 TABLES 49 FIGURES 61 PREFACE The exploration, study, and definition of the environmental conditions which exist in space beyond the earth's atmosphere form an essential part of the current space-age effort. The development of this science is of especial interest to the vehicle structures designer, who must make decisions today that will establish the capability and efficiency of the space hardware in use 5 °r 10 years hence. -
Viscosity from Newton to Modern Non-Equilibrium Statistical Mechanics
Viscosity from Newton to Modern Non-equilibrium Statistical Mechanics S´ebastien Viscardy Belgian Institute for Space Aeronomy, 3, Avenue Circulaire, B-1180 Brussels, Belgium Abstract In the second half of the 19th century, the kinetic theory of gases has probably raised one of the most impassioned de- bates in the history of science. The so-called reversibility paradox around which intense polemics occurred reveals the apparent incompatibility between the microscopic and macroscopic levels. While classical mechanics describes the motionof bodies such as atoms and moleculesby means of time reversible equations, thermodynamics emphasizes the irreversible character of macroscopic phenomena such as viscosity. Aiming at reconciling both levels of description, Boltzmann proposed a probabilistic explanation. Nevertheless, such an interpretation has not totally convinced gen- erations of physicists, so that this question has constantly animated the scientific community since his seminal work. In this context, an important breakthrough in dynamical systems theory has shown that the hypothesis of microscopic chaos played a key role and provided a dynamical interpretation of the emergence of irreversibility. Using viscosity as a leading concept, we sketch the historical development of the concepts related to this fundamental issue up to recent advances. Following the analysis of the Liouville equation introducing the concept of Pollicott-Ruelle resonances, two successful approaches — the escape-rate formalism and the hydrodynamic-mode method — establish remarkable relationships between transport processes and chaotic properties of the underlying Hamiltonian dynamics. Keywords: statistical mechanics, viscosity, reversibility paradox, chaos, dynamical systems theory Contents 1 Introduction 2 2 Irreversibility 3 2.1 Mechanics. Energyconservationand reversibility . ........................ 3 2.2 Thermodynamics. -
Slope - Geologic Age Relationships in Complex Lunar Craters C
49th Lunar and Planetary Science Conference 2018 (LPI Contrib. No. 2083) 2399.pdf SLOPE - GEOLOGIC AGE RELATIONSHIPS IN COMPLEX LUNAR CRATERS C. Rojas1, P. Mahanti1, M. S. Robinson1, LROC Team1, 1LROC Science Operation Center, School of Earth and Space Exploration, Arizona State University, Tempe, Arizona ([email protected]) Table 1: List of complex craters. *Copernican craters Introduction: Impact events leading to formation Crater D (km) Model Age (Ga) Lon Lat of basins and large craters dominate the early history Moore F* 24 0.041∓0.012 [8] 37.30 185.0 of the Moon [1] leading to kilometer scale topographic Wiener F* 30 0.017∓0.002 149.9740.90 variations on the lunar surface, with smaller crater [2], Klute W* 31 0.090∓0.007 216.7037.98 progressively introducing higher frequency topography. Necho* 37 0.080∓0.024 [8] 123.3 –5.3 Crater wall slopes represent most of the overall topo- Aristarchus* 40 0.175∓0.0095 312.5 23.7 graphic variation since many locations on the Moon are Jackson* 71 0.147∓0.038 [9] 196.7 22.1 craters. While impact events lead to the formation of McLaughlin 75 3.7∓0.1 [10] 267.1747.01 steep slopes [3], they are also primarily responsible for Pitiscus 80 3.8∓0.1 [10] 30.57 -50.61 landform degradation [4]. During crater formation, tar- Al-Biruni 80 3.8∓0.1 [10] 92.62 18.09 get properties and processes controlling structural sta- La Pérouse 80 3.6∓0.1 [10] -10.66 76.18 bility limit maximum slopes [4]. -
Modeling and Mapping of the Structural Deformation of Large Impact Craters on the Moon and Mercury
MODELING AND MAPPING OF THE STRUCTURAL DEFORMATION OF LARGE IMPACT CRATERS ON THE MOON AND MERCURY by JEFFREY A. BALCERSKI Submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy Department of Earth, Environmental, and Planetary Sciences CASE WESTERN RESERVE UNIVERSITY August, 2015 CASE WESTERN RESERVE UNIVERSITY SCHOOL OF GRADUATE STUDIES We hereby approve the thesis/dissertation of Jeffrey A. Balcerski candidate for the degree of Doctor of Philosophy Committee Chair Steven A. Hauck, II James A. Van Orman Ralph P. Harvey Xiong Yu June 1, 2015 *we also certify that written approval has been obtained for any proprietary material contained therein ~ i ~ Dedicated to Marie, for her love, strength, and faith ~ ii ~ Table of Contents 1. Introduction ............................................................................................................1 2. Tilted Crater Floors as Records of Mercury’s Surface Deformation .....................4 2.1 Introduction ..............................................................................................5 2.2 Craters and Global Tilt Meters ................................................................8 2.3 Measurement Process...............................................................................12 2.3.1 Visual Pre-selection of Candidate Craters ................................13 2.3.2 Inspection and Inclusion/Exclusion of Altimetric Profiles .......14 2.3.3 Trend Fitting of Crater Floor Topography ................................16 2.4 Northern -
Ages of Large Lunar Impact Craters and Implications for Bombardment During the Moon’S Middle Age ⇑ Michelle R
Icarus 225 (2013) 325–341 Contents lists available at SciVerse ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Ages of large lunar impact craters and implications for bombardment during the Moon’s middle age ⇑ Michelle R. Kirchoff , Clark R. Chapman, Simone Marchi, Kristen M. Curtis, Brian Enke, William F. Bottke Southwest Research Institute, 1050 Walnut Street, Suite 300, Boulder, CO 80302, United States article info abstract Article history: Standard lunar chronologies, based on combining lunar sample radiometric ages with impact crater den- Received 20 October 2012 sities of inferred associated units, have lately been questioned about the robustness of their interpreta- Revised 28 February 2013 tions of the temporal dependance of the lunar impact flux. In particular, there has been increasing focus Accepted 10 March 2013 on the ‘‘middle age’’ of lunar bombardment, from the end of the Late Heavy Bombardment (3.8 Ga) until Available online 1 April 2013 comparatively recent times (1 Ga). To gain a better understanding of impact flux in this time period, we determined and analyzed the cratering ages of selected terrains on the Moon. We required distinct ter- Keywords: rains with random locations and areas large enough to achieve good statistics for the small, superposed Moon, Surface crater size–frequency distributions to be compiled. Therefore, we selected 40 lunar craters with diameter Cratering Impact processes 90 km and determined the model ages of their floors by measuring the density of superposed craters using the Lunar Reconnaissance Orbiter Wide Angle Camera mosaic. Absolute model ages were computed using the Model Production Function of Marchi et al. -
GRAIL Gravity Observations of the Transition from Complex Crater to Peak-Ring Basin on the Moon: Implications for Crustal Structure and Impact Basin Formation
Icarus 292 (2017) 54–73 Contents lists available at ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus GRAIL gravity observations of the transition from complex crater to peak-ring basin on the Moon: Implications for crustal structure and impact basin formation ∗ David M.H. Baker a,b, , James W. Head a, Roger J. Phillips c, Gregory A. Neumann b, Carver J. Bierson d, David E. Smith e, Maria T. Zuber e a Department of Geological Sciences, Brown University, Providence, RI 02912, USA b NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA c Department of Earth and Planetary Sciences and McDonnell Center for the Space Sciences, Washington University, St. Louis, MO 63130, USA d Department of Earth and Planetary Sciences, University of California, Santa Cruz, CA 95064, USA e Department of Earth, Atmospheric and Planetary Sciences, MIT, Cambridge, MA 02139, USA a r t i c l e i n f o a b s t r a c t Article history: High-resolution gravity data from the Gravity Recovery and Interior Laboratory (GRAIL) mission provide Received 14 September 2016 the opportunity to analyze the detailed gravity and crustal structure of impact features in the morpho- Revised 1 March 2017 logical transition from complex craters to peak-ring basins on the Moon. We calculate average radial Accepted 21 March 2017 profiles of free-air anomalies and Bouguer anomalies for peak-ring basins, protobasins, and the largest Available online 22 March 2017 complex craters. Complex craters and protobasins have free-air anomalies that are positively correlated with surface topography, unlike the prominent lunar mascons (positive free-air anomalies in areas of low elevation) associated with large basins. -
Modelling the Liquid-Water Vein System Within Polar Ice Sheets As a Potential Microbial Habitat
Earth and Planetary Science Letters 333–334 (2012) 238–249 Contents lists available at SciVerse ScienceDirect Earth and Planetary Science Letters journal homepage: www.elsevier.com/locate/epsl Modelling the liquid-water vein system within polar ice sheets as a potential microbial habitat K.G. Srikanta Dani a,1, Heidy M. Mader a,n, Eric W. Wolff b, Jemma L. Wadham c a School of Earth Sciences, University of Bristol, Wills Memorial Building, Queen’s Road, Bristol BS8 1RJ, UK b British Antarctic Survey, High Cross, Madingley Road, Cambridge CB3 0ET, UK c School of Geographical Sciences, University of Bristol, University Road, Bristol BS8 1SS, UK article info abstract Article history: Based on the fundamental and distinctive physical properties of polycrystalline ice Ih, the chemical and Received 12 October 2011 temperature profiles within the polar ice sheets, and the observed selective partitioning of bacteria into Received in revised form liquid water filled veins in the ice, we consider the possibility that microbial life could survive and be 21 March 2012 sustained within glacial systems. Here, we present a set of modelled vertical profiles of vein diameter, Accepted 6 April 2012 vein chemical concentration, and vein water volume variability across a range of polar ice sheets using Editor: G. Henderson Available online 22 May 2012 their ice core chemical profiles. A sensitivity analysis of VeinsInIce1.0, the numerical model used in this study shows that the ice grain size and the local borehole temperature are the most significant factors Keywords: that influence the intergranular liquid vein size and the amount of freeze-concentrated impurities polar ice cores partitioned into the veins respectively. -
Science Concept 3: Key Planetary
Science Concept 6: The Moon is an Accessible Laboratory for Studying the Impact Process on Planetary Scales Science Concept 6: The Moon is an accessible laboratory for studying the impact process on planetary scales Science Goals: a. Characterize the existence and extent of melt sheet differentiation. b. Determine the structure of multi-ring impact basins. c. Quantify the effects of planetary characteristics (composition, density, impact velocities) on crater formation and morphology. d. Measure the extent of lateral and vertical mixing of local and ejecta material. INTRODUCTION Impact cratering is a fundamental geological process which is ubiquitous throughout the Solar System. Impacts have been linked with the formation of bodies (e.g. the Moon; Hartmann and Davis, 1975), terrestrial mass extinctions (e.g. the Cretaceous-Tertiary boundary extinction; Alvarez et al., 1980), and even proposed as a transfer mechanism for life between planetary bodies (Chyba et al., 1994). However, the importance of impacts and impact cratering has only been realized within the last 50 or so years. Here we briefly introduce the topic of impact cratering. The main crater types and their features are outlined as well as their formation mechanisms. Scaling laws, which attempt to link impacts at a variety of scales, are also introduced. Finally, we note the lack of extraterrestrial crater samples and how Science Concept 6 addresses this. Crater Types There are three distinct crater types: simple craters, complex craters, and multi-ring basins (Fig. 6.1). The type of crater produced in an impact is dependent upon the size, density, and speed of the impactor, as well as the strength and gravitational field of the target. -
13. Martian Cratering and Implications for the Chronostratigraphy
13. Martian Cratering and Implications for the Chronostratigraphy The record of large impact basins on differ- ent planetary bodies allows us to compare the characteristics of the heavy bombardment pe- riod and the end of planetary formation. Both the cratering record itself and the age distri- bution of the impact basins represent the pe- riod of highest impactor flux, decaying rapidly within the first half billion years of our solar system. In order to test the plausibility of the Martian chronology model (see Chapter 5), the ages of the large Martian impact basins, using the derived Martian production function, were determined and compared to lunar basin ages. For the Moon, the large basins were produced no later than about 3.8 to 3.9 Ga ago and a similar situation should exist for Mars, follow- ing the marker horizon idea (Wetherill, 1975). This idea is based on the assumption that solar system bodies have undergone a similar evo- lution since planetary formation. In the cra- Figure 13.1.: The crater size frequency distribu- tering record on any solid surface body, which tion measured for one of the oldest regions on Mars: has representative large old surface units, this Noachis Terra (map nomenclature: unit Npl1). first period of heavy bombardment is present in the general crater size–frequency distribution as well as the large basin record itself. According to our investigation, the oldest surface areas on than the visible highland surface, where crater Mars, roughly the Martian southern highlands, count ages are based on craters clearly recog- e. g. Noachis Terra, were formed between 4.0 nized by their morphology. -
Arxiv:1205.3312V3 [Physics.Gen-Ph] 4 Sep 2012
A beacon of new physics: the Pioneer anomaly modelled as a path based speed loss driven by the externalisation of aggregate non-inertial QM energy Paul G. ten Boom School of Physics, University of New South Wales, Sydney NSW 2052, Australia Email: [email protected], [email protected] Abstract: This treatise outlines how a non-systematic based Pioneer anomaly, with its implied violation (re: ‘low’ mass bodies only) of both general relativity’s weak equivalence principle and the Newtonian inverse-square law, can be successfully modelled. These theoretical hurdles and various awkward observational constraints, such as the low value of Pioneer 11’s anomaly pre-Saturn encounter, have (to date) not been convincingly modelled. Notwithstanding the recent trend to embrace a non-constant Sun/Earth-directed heat based explanation of this anomalous deceleration, the actual: nature, direction, and temporal and spatial variation of the Pioneer anomaly remain an open arena of research. Working backwards from the observational evidence, and rethinking: time, mass, quantum entanglement and non-locality, we hypothesise a mechanism involving a quantum mechanical energy source and a new type of ‘gravitational’ field; neither of which lie within general relativity’s domain of formulation/application. By way of a systemic conservation of energy principle, an internally inexpressible (aggregate) non-inertial energy discrepancy/uncertainty — involving a myriad of quantum (lunar/third-body residing) atomic and molecular systems moving in analog curved spacetime — is (non-locally) re-expressed externally as a (rotating) non-Euclidean spatial geometry perturbation. At a moving body each “rotating space-warp” induces sinusoidal proper acceleration and speed perturbations, as well as a path-based constant (per cycle) rate of speed shortfall relative to predictions that omit the additional effect. -
Statistical Study of Rock Drilling by Hypervelocity Jets from Explosive Shaped Charges
Scholars' Mine Doctoral Dissertations Student Theses and Dissertations 1971 Statistical study of rock drilling by hypervelocity jets from explosive shaped charges John William Brown Follow this and additional works at: https://scholarsmine.mst.edu/doctoral_dissertations Part of the Mining Engineering Commons Department: Mining Engineering Recommended Citation Brown, John William, "Statistical study of rock drilling by hypervelocity jets from explosive shaped charges" (1971). Doctoral Dissertations. 1850. https://scholarsmine.mst.edu/doctoral_dissertations/1850 This thesis is brought to you by Scholars' Mine, a service of the Missouri S&T Library and Learning Resources. This work is protected by U. S. Copyright Law. Unauthorized use including reproduction for redistribution requires the permission of the copyright holder. For more information, please contact [email protected]. STATISTICAL STUDY OF ROCK DRILLING BY HYPERVELOCITY JETS FROM EXPLOSIVE SHAPED CHARGES by JOHN WILLIAM BROWN, 19 42- A DISSERTATION Presented to the Faculty of the Graduate School of the UNIVERSITY OF MISSOURI-ROLLA In Partial Fulfillment of the Requirements for the Degree DOCTOR OF PHILOSOPHY in T2608 164 pages MINING ENGINEERING c.l 1971 &~£~ £i?L;;~~ 202886 @ 1972 JOHM WILLIAM BROWN ALL RIGHI'S RESERVED iii STATISTICAL STUDY OF ROCK DRILLING BY HYPERVELOCITY JETS FROM EXPLOSIVE SHAPED CHARGES ABSTRACT The drilling effect in rock of hypervelocity jets from explosive shaped charges was investigated experimentally to supplement a rapid excavation concept. The effects of the design factors of the charge and the mechanical properties of eight rock types were studied. Experiments were both designed and analyzed upon statistical principles. A full factorial experimental design was used for each of seven rock types. -
The George Wright Forum
national park units A new method for setting preservation priorities Science vs. political interference in system planning What's a name worth? — The Yosemite trademark fight Why public financing is critical to parks Needed: Reliable funding for bison management Countering "ecomodernism" The George Wright Forum The GWS Journal of Parks, Protected Areas & Cultural Sites volume 33 number 1 • 2016 Mission The George Wright Society promotes protected area stewardship by bring ing practitioners together to share their expertise. Our Goal The Society strives to be the premier organization connecting people, plac es, knowledge, and ideas to foster excellence in natural and cultural resource management, research, protection, and interpretation in parks and equivalent reserves. Board of Directors Nathalie Gagnon, President • Ottawa, Ontario Jerry M. Mitchell, Vice President • Littleton, Colorado David J. Parsons, Secretary • Florence, Montana Ryan Sharp, Treasurer • Manhattan, Kansas Zarnaaz Bashir • Ashburn, Virginia David Graber • Three Rivers, California Barrett Kennedy • Baton Rouge, Louisiana Armando Quintero • San Rafael, California Chris Spence • Mill Valley, California Lynn Wilson • Cobble Hill, British Columbia Graduate Student Liaison to the Board Gina Depper • Clemson, South Carolina Executive Office David Harmon, Executive Director/ Co-editor, The George Wright Forum Emily Dekker-Fiala, Conference Coordinator Rebecca Conard, Co-editor, The George Wright Forum P. O. Box 65 • Hancock, Michigan 49930-0065 USA 1-906-487-9722 • [email protected] • www.georgewright.org O 2016 The George Wright Society. All rights reserved (No copyright is claimed for previously published material reprinted herein.) ISSN 0732-4715. Editorial and manuscript submission guidelines may be found at www.georgewright.org/forum. Text paper is made of 50% recycled fi bers.