Pife-Pic: Parallel Immersed-Finite-Element Particle-In-Cell for 3-D Kinetic Simulations of Plasma-Material Interactions∗
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Lunar Impact Basins Revealed by Gravity Recovery and Interior
Lunar impact basins revealed by Gravity Recovery and Interior Laboratory measurements Gregory Neumann, Maria Zuber, Mark Wieczorek, James Head, David Baker, Sean Solomon, David Smith, Frank Lemoine, Erwan Mazarico, Terence Sabaka, et al. To cite this version: Gregory Neumann, Maria Zuber, Mark Wieczorek, James Head, David Baker, et al.. Lunar im- pact basins revealed by Gravity Recovery and Interior Laboratory measurements. Science Advances , American Association for the Advancement of Science (AAAS), 2015, 1 (9), pp.e1500852. 10.1126/sci- adv.1500852. hal-02458613 HAL Id: hal-02458613 https://hal.archives-ouvertes.fr/hal-02458613 Submitted on 26 Jun 2020 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. RESEARCH ARTICLE PLANETARY SCIENCE 2015 © The Authors, some rights reserved; exclusive licensee American Association for the Advancement of Science. Distributed Lunar impact basins revealed by Gravity under a Creative Commons Attribution NonCommercial License 4.0 (CC BY-NC). Recovery and Interior Laboratory measurements 10.1126/sciadv.1500852 Gregory A. Neumann,1* Maria T. Zuber,2 Mark A. Wieczorek,3 James W. Head,4 David M. H. Baker,4 Sean C. Solomon,5,6 David E. Smith,2 Frank G. -
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. -
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. -
University of Arkansas School of Architecture.” Annual Conference of the Society of Architectural Historians Savannah, Georgia, April 28, 2006
UNIVERSITY OF ARKANSAS FAYETTEVILLE, ARKANSAS PUBLICATIONS AND PRESENTATIONS July 1, 2005-June 30, 2006 Table of Contents Bumpers College of Agricultural, Food and Life Sciences Page 3 School of Architecture Page 145 Fulbright College of Arts and Sciences Page 156 Walton College of Business Page 273 Deleted: 5 College of Education and Health Professions Page 297 Deleted: 300 College of Engineering Page 322 Deleted: 5 School of Law Page 392 Deleted: 7 2 Dale Bumpers College of Agricultural, Food and Life Sciences Books Biological and Agricultural Engineering Sabatier, P., Focht, W., Lubell, M., Trachtenberg, Z., Vedlitz, A., and Matlock, M.. Swimming Upstream: Collaborative Approaches to Watershed Management. Publisher: MIT Press – ISBN # 0-262-19520-8; March 2005. Crop, Soil and Environmental Sciences Norman, R.J., J.-F. Meullenet, K.A.K. Moldenhauer (eds.). 2005. B.R. Wells Rice Research Studies 2004. Univ. of Ark., Agr. Exp. Stn. Res. Ser. 529. 441 pages. Roberts, C.A., C.P. West, and D.E. Spiers (eds). 2005. Neotyphodium in Cool-Season Grasses. Blackwell Publishing Professional. Ames, IA. 395 pages. Entomology Horton, D. and D.T. Johnson. 2005. Southeastern peach grower’s handbook. The University of Georgia College of Agricultural and Environmental Sciences Cooperative Extension Service Bull. 1171. McLeod, P.J., M.E. Pontaroli, J.C. Correll, F. Copa, H. Serrate and R. Unterladstaetter. 2005. Identificacion y Manejo de Insectos en Hortalizas en Bolivia (Identification and Management of Insects in Vegetable sin Bolivia). Sirena Press, Santa Cruz, Bolivia, 162 pp. Horticulture Hensley, D.L. 2005. Professional Landscape Management 2nd edition. Stipes Publishing. Champaign, IL, 342 p. -
Signal Processing: a Mathematical Approach, Second Edition
Mathematics MONOGRAPHS AND RESEARCH NOTES IN MATHEMATICS MONOGRAPHS AND RESEARCH NOTES IN MATHEMATICS Second Edition Second Signal Processing: A Mathematical Approach is designed to show how many of the mathematical tools the reader knows can be used to understand and employ signal processing techniques in an applied environment. Assuming an advanced undergraduate- or graduate- level understanding of mathematics—including familiarity with Fouri- er series, matrices, probability, and statistics—this Second Edition: Signal Processing , Contains new chapters on convolution and the vector DFT, Processing Signal plane-wave propagation, and the BLUE and Kalman lters A Mathematical Approach , Expands the material on Fourier analysis to three new chapters to provide additional background information Second Edition , Presents real-world examples of applications that demonstrate how mathematics is used in remote sensing Featuring problems for use in the classroom or practice, Signal Processing: A Mathematical Approach, Second Edition covers topics such as Fourier series and transforms in one and several vari- ables; applications to acoustic and electro-magnetic propagation models, transmission and emission tomography, and image recon- struction; sampling and the limited data problem; matrix methods, singular value decomposition, and data compression; optimization techniques in signal and image reconstruction from projections; autocorrelations and power spectra; high-resolution methods; de- tection and optimal ltering; and eigenvector-based methods for array processing and statistical ltering, time-frequency analysis, and wavelets. Charles L. Byrne “A PDF version of this book is available for free in Open Byrne Access at www.taylorfrancis.com. It has been made available under a Creative Commons Attribution-Non Commercial-No Derivatives 4.0 license.” Signal Processing A Mathematical Approach Second Edition MONOGRAPHS AND RESEARCH NOTES IN MATHEMATICS Series Editors John A. -
Constraining the Evolutionary History of the Moon and the Inner Solar System: a Case for New Returned Lunar Samples
Constraining the Evolutionary History of the Moon and the Inner Solar System: A Case for New Returned Lunar Samples The MIT Faculty has made this article openly available. Please share how this access benefits you. Your story matters. Citation Tartèse, Romain, et al. "Constraining the Evolutionary History of the Moon and the Inner Solar System: A Case for New Returned Lunar Samples." Space Science Reviews, 215 (December 2019): 54. © 2019, The Author(s). As Published http://dx.doi.org/10.1007/s11214-019-0622-x Publisher Springer Science and Business Media LLC Version Final published version Citable link https://hdl.handle.net/1721.1/125329 Terms of Use Creative Commons Attribution 4.0 International license Detailed Terms https://creativecommons.org/licenses/by/4.0/ Space Sci Rev (2019) 215:54 https://doi.org/10.1007/s11214-019-0622-x Constraining the Evolutionary History of the Moon and the Inner Solar System: A Case for New Returned Lunar Samples Romain Tartèse1 · Mahesh Anand2,3 · Jérôme Gattacceca4 · Katherine H. Joy1 · James I. Mortimer2 · John F. Pernet-Fisher1 · Sara Russell3 · Joshua F. Snape5 · Benjamin P. Weiss6 Received: 23 August 2019 / Accepted: 25 November 2019 / Published online: 2 December 2019 © The Author(s) 2019 Abstract The Moon is the only planetary body other than the Earth for which samples have been collected in situ by humans and robotic missions and returned to Earth. Scien- tific investigations of the first lunar samples returned by the Apollo 11 astronauts 50 years ago transformed the way we think most planetary bodies form and evolve. Identification of anorthositic clasts in Apollo 11 samples led to the formulation of the magma ocean concept, and by extension the idea that the Moon experienced large-scale melting and differentiation. -
NASA Scientific and Technical Aerospace Reports
NASA STI Program ... in Profile Since its founding, NASA has been dedicated • CONFERENCE PUBLICATION. to the advancement of aeronautics and space Collected papers from scientific and science. The NASA scientific and technical technical conferences, symposia, information (STI) program plays a key part in seminars, or other meetings sponsored helping NASA maintain this important role. or co-sponsored by NASA. The NASA STI program operates under the • SPECIAL PUBLICATION. Scientific, auspices of the Agency Chief Information technical, or historical information from Officer. It collects, organizes, provides for NASA programs, projects, and missions, archiving, and disseminates NASA’s STI. The often concerned with subjects having NASA STI program provides access to the substantial public interest. NASA Aeronautics and Space Database and its public interface, the NASA Technical Report • TECHNICAL TRANSLATION. Server, thus providing one of the largest English-language translations of foreign collections of aeronautical and space science scientific and technical material pertinent to STI in the world. Results are published in both NASA’s mission. non-NASA channels and by NASA in the NASA STI Report Series, which includes the Specialized services also include organizing following report types: and publishing research results, distributing specialized research announcements and feeds, • TECHNICAL PUBLICATION. Reports of providing help desk and personal search completed research or a major significant support, and enabling data exchange services. phase of research that present the results of NASA Programs and include extensive data For more information about the NASA STI or theoretical analysis. Includes compila- program, see the following: tions of significant scientific and technical data and information deemed to be of • Access the NASA STI program home page continuing reference value. -
10Th International Conference and School on Plasma Physics and Controlled Fusion
UA0500657 10th International Conference and School on Plasma Physics and Controlled Fusion Alushta (Crimea), Ukraine, September 13-18, 2004 i Alushta Ukraine Organized by National Science Center 'Kharkov Institute of Physics and Technology 10th International Conference and School on Plasma Physics and Controlled Fusion Alushta (Crimea), Ukraine, September 13-18, 2004 BOOK OF ABSTRACTS Alushta Ukraine Organized by National Science Center 'Kharkov Institute of Physics and Technology' International Advisory Committee: C.Alejaldre - CIEMAT, Spain M.I.Pergament-TRINITI, Russia V.Astashynski - 1MAF of Belarus MJ.Sadowski - SINS, Poland Acad. of Sci. V.P.Smirnov - RRC "Kurchatov I.G.Brown - LBNL, USA Inst.", Russia T.Dolan - INEEL, USA P.E.Stott - CEA, Cadarache, France Ya.B.Fainberg-NSC KIPT, Ukraine F.Wagner - IPP, Germany A.Hassanein - ANL, USA K. Yamazaki - NIFS, Japan L.M.Kovrizhnykh -GPI of RAS, Russia K.A.Yushchenko - Paton Inst. of E.P.Kruglyakov - INF, Russia Welding, NAS of Ukraine V.I.Lapshin - NSC KIPT, Ukraine A.G.Zagorodny - Bogolyubov Inst. J.Lyon - ORNL, USA for Theoretic Phys., NAS of Ukraine Program Committee: V.I.Lapshin (IPP NSC KIPT) - Chairman K.N.Stepanov (IPP NSC KIPT) - Vice Chairman I.E.Garkusha (IPP NSC KIPT) - Scientific Secretary N.A.Azarenkov (Karazin National Univ., Kharkov) Yu.I.Chutov (T.Shevchenko National Univ., Kiev) T.A.Davydova (INR of NAS of Ukraine, Kiev) G.S.Kirichenko (INR of NAS of Ukraine, Kiev) I.N.Qnishchenko (IPENMA NSC KIPT) O.S.Pavlichenko (IPP NSC KIPT) O.B.Shpenyk (IEP of NAS of Ukraine, Uzhgorod) I.A.SoIoshenko (IP of NAS of Ukraine, Kiev) V.S.Taran (IPP NSC KIPT) V.I.Tereshin (IPP NSC KIPT) V.T.Tolok (Karazin National Univ., Kharkov) V.S.Voitsenya (IPP NSC KIPT) E.D.Volkov (IPP NSC KIPT) A.M.Yegorov (IPENMA NSC KIPT) I.I.Zalyubovski (Karazin National Univ., Kharkov) K.A.Yushchenko (Paton Inst. -
Crustal Porosity Reveals the Bombardment History of the Moon Authors: Ya Huei Huang1*, Jason M
Crustal porosity reveals the bombardment history of the Moon Ya Huei Huang ( [email protected] ) Massachusetts Institute of Technology Jason Soderblom Massachusetts Institute of Technology https://orcid.org/0000-0003-3715-6407 David Minton Purdue University Masatoshi Hirabayashi Auburn University https://orcid.org/0000-0002-1821-5689 Jay Melosh Purdue University https://orcid.org/0000-0003-1881-1496 Article Keywords: Planetary Bombardment, Solar System Formation and Evolution, Porosity Modication, Siderophile Delivery Posted Date: January 6th, 2021 DOI: https://doi.org/10.21203/rs.3.rs-98852/v1 License: This work is licensed under a Creative Commons Attribution 4.0 International License. Read Full License Title: Crustal porosity reveals the bombardment history of the Moon Authors: Ya Huei Huang1*, Jason M. Soderblom1, David A. Minton2, Masatoshi Hirabayashi3, H. Jay Melosh2. Affiliations: 1Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, Massachusetts USA 02139. 2Department of Earth, Atmospheric, and Planetary Sciences, Purdue University, West Lafayette, Indiana USA 47907. 3Department of Aerospace Engineering, Auburn University, Auburn, Alabama USA 36849. *To whom correspondence should be addressed. E-mail: [email protected] 1 Planetary bombardment histories provide critical information regarding the formation and 2 evolution of the Solar System and of the planets within it. These records evidence transient 3 instabilities in the Solar System’s orbital evolution1, giant impacts such as the Moon-forming 4 impact2, and material redistribution. Such records provide insight into planetary evolution, 5 including the deposition of energy, delivery of materials, and crustal processing, specifically 6 the modification of porosity. Bombardment histories are traditionally constrained from the 7 surface expression of impacts — these records, however, are degraded by various geologic 8 processes. -
Science Concept 3: Key Planetary Processes Are Manifested in the Diversity of Lunar Crustal Rocks
Science Concept 3: Key Planetary Processes are Manifested in the Diversity of Lunar Crustal Rocks Science Concept 3: Key planetary processes are manifested in the diversity of crustal rocks Science Goals: a. Determine the extent and composition of the primary feldspathic crust, KREEP layer, and other products of differentiation. b. Inventory the variety, age, distribution, and origin of lunar rock types. c. Determine the composition of the lower crust and bulk Moon. d. Quantify the local and regional complexity of the current lunar crust. e. Determine the vertical extent and structure of the megaregolith. INTRODUCTION Formation and Evolution of the Moon The Moon is a unique environment, preserving crucial information about the early history and later evolution of the solar system. The lack of major surficial tectonic processes within the past few billion years or so, as well as the lack of significant quantities of surface water, have allowed for excellent preservation of the lithologies and geomorphological features that formed during the major planetary formation events. Fundamental discoveries during the Apollo program showed that the Moon is made up of a variety of volcanic and impact rock types that exhibit a particular range of chemical and mineralogical compositions. The key planetary processes conveyed by this diversity include planetary differentiation, volcanism, and impact cratering. Analysis of Apollo, Luna, and lunar meteoritic samples, as well as orbital data from a series of lunar exploration missions, generated geophysical models that strove to tell the story of the Moon. However, such models are restricted in the sense that they are based on information gathered from the samples that have so far been acquired. -
Density and Porosity of the Upper Lunar Crust from Combined Analysis of Gravity and Topography Data – Evaluation of the Interior Structure of Impact Basins
Titelblatt Density and porosity of the upper lunar crust from combined analysis of gravity and topography data – Evaluation of the interior structure of impact basins vorgelegt von M.Sc. Daniel Wahl ORCID: 0000-0003-4884-6630 von der Fakultät VI – Planen, Bauen, Umwelt der Technischen Universität Berlin zur Erlangung des akademischen Grades Doktor der Ingenieurwissenschaften - Dr.-Ing. - genehmigte Dissertation Promotionsausschuss: Vorsitzender: Prof. Dr. Frank Flechtner Gutachter: Prof. Dr. Jürgen Oberst Gutachter: Prof. Dr. Doris Breuer Gutachter: Prof. Dr. Ulrich Hansen Tag der wissenschaftlichen Aussprache: 18. Dezember 2020 Berlin 2021 PhD Thesis Density and porosity of the upper lunar crust from combined analysis of gravity and topography data – Evaluation of the interior structure of impact basins Supervised by Prof. Dr. phil. nat. Jürgen Oberst Released by M.Sc. Daniel Wahl Berlin 2021 Density and porosity of the upper lunar crust from combined analysis of gravity and topography data – Evaluation of the interior structure of impact basins Daniel Wahl This research was funded by the Deutsche Forschungsgemeinschaft (DFG), grant SFB TRR-170-1 TP A4 – Late Accretion onto Terrestrial Planets. The project was realized at the Chair of Planetary Geodesy, Institute of Geodesy and Geoinformation Science, Technische Universität Berlin, Germany. i Acknowledgement First, I would like to express my gratitude to Jürgen Oberst, who offered me the great opportunity to do my PhD in the most exciting field of lunar research at his department of Planetary Geodesy at Technische Universität Berlin. Thank you for providing excellent support throughout the entire doctorate and spending so much time discussing my work. Thank you for sending me around the world to inspiring conferences and workshops, where I had the chance to present and discuss my findings with experts from different scientific fields. -
The Composition of the Lunar Crust: an In-Depth Remote Sensing View
THE COMPOSITION OF THE LUNAR CRUST: AN IN-DEPTH REMOTE SENSING VIEW A DISSERTATION SUBMITTED TO THE GRADUATE DIVISION OF THE UNIVERSITY OF HAWAIʻI AT MĀNOA IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF DOCTOR OF PHILOSOPHY IN GEOLOGY AND GEOPHYSICS August 2016 By Myriam Lemelin Dissertation Committee: Paul G. Lucey, Chairperson G. Jeffrey Taylor Jeffrey J. Gillis-Davis Peter Englert Karen Meech Keywords: Moon; Remote sensing; Spectroscopy; Lunar crust; Central peak; Basin ring ii ACKNOWLEDGEMENTS Five years ago I was working at the Lunar and Planetary Institute with amazing colleagues such as Carolyn Eve, David Blair, Kirby Runyon, Stephanie Quintana and Sarah Crites. We were discussing our future on our way back home from work, stopping to see the alligators and armadillos on the way, and they asked me what I wanted do next. If I could do anything, what would it be? I wanted to do a PhD in Hawaii with Paul Lucey. I feel very privileged that it happened, as it has been such a marking moment in my life, both from a science and a personnel perspective. I want to thank many people who contributed in making this experience incredible. I want to thank my advisor, Paul Lucey, for his endless creative ideas, his impressive knowledge and for allowing me to take part in many science meetings and conferences where I learned so much about various aspects of planetary sciences, and where I met numerous space enthusiast scientists. I want to thank my dissertation committee members, Jeff Taylor, Jeff Gillis-Davis, Peter Englert, and Karen Meech for their suggestions and comments.