Monday Morning, October 19, 2015 Atom Probe Tomography Focus Topic Complex Device Such As Solar Cells and Batteries Is the Need of the Hour
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UC Irvine UC Irvine Previously Published Works
UC Irvine UC Irvine Previously Published Works Title Astrophysics in 2006 Permalink https://escholarship.org/uc/item/5760h9v8 Journal Space Science Reviews, 132(1) ISSN 0038-6308 Authors Trimble, V Aschwanden, MJ Hansen, CJ Publication Date 2007-09-01 DOI 10.1007/s11214-007-9224-0 License https://creativecommons.org/licenses/by/4.0/ 4.0 Peer reviewed eScholarship.org Powered by the California Digital Library University of California Space Sci Rev (2007) 132: 1–182 DOI 10.1007/s11214-007-9224-0 Astrophysics in 2006 Virginia Trimble · Markus J. Aschwanden · Carl J. Hansen Received: 11 May 2007 / Accepted: 24 May 2007 / Published online: 23 October 2007 © Springer Science+Business Media B.V. 2007 Abstract The fastest pulsar and the slowest nova; the oldest galaxies and the youngest stars; the weirdest life forms and the commonest dwarfs; the highest energy particles and the lowest energy photons. These were some of the extremes of Astrophysics 2006. We attempt also to bring you updates on things of which there is currently only one (habitable planets, the Sun, and the Universe) and others of which there are always many, like meteors and molecules, black holes and binaries. Keywords Cosmology: general · Galaxies: general · ISM: general · Stars: general · Sun: general · Planets and satellites: general · Astrobiology · Star clusters · Binary stars · Clusters of galaxies · Gamma-ray bursts · Milky Way · Earth · Active galaxies · Supernovae 1 Introduction Astrophysics in 2006 modifies a long tradition by moving to a new journal, which you hold in your (real or virtual) hands. The fifteen previous articles in the series are referenced oc- casionally as Ap91 to Ap05 below and appeared in volumes 104–118 of Publications of V. -
Salubrious Living
Salubrious Living 00. Salubrious Living - Introduction 01. The Search for Youth 02. The Myth of Medical Progress 03. The Hygienic System 04. The Nature of Disease 05. The Foods of Civilization 06. The Foods of Primitive Man 07. Don't Cook Your Foods 08. The Fruitarian Diet 09. How to Plan Your Meals 10. The Best Sources of Minerals and Vitamins 11. Soil and Food 12. Nature's Supreme Healing Agency 13. The Value of Heliotherapy 14. Building Strength and Health Through Exercise 15. Some Common Ailments 16. Why Lose Your Teeth? 17. Better Vision Without Glasses 18. Building Strong Feet 19. Keep Your Hair 20. The Needs of Infants and Growing Children 21. To Build Beauty You Must Build Health 22. Eugenics and the Survival of the White Race Author: Ben Klassen Format: Paperback Creativity Book Publisher Pub. Date: 1982 Food Chart Copyright © 2003 by World Church of Creativity Salubrious Living - Introduction The term "Salubrious Living" is a nomenclature I have coined as part and parcel of a very important facet of our religious creed and program set forth by the CHURCH OF THE CREATOR. The word "salubrious" comes from the Latin word "salubris" meaning "healthy; wholesome; sound; useful; vigorous". Webster's dictionary defines the English derivative "salubrious" as: 1. favorable to, or promoting health or well being; invigorating; 2. spiritually wholesome; conducive to good results". It is in this context of fully promoting the health and well being of the White Race that we use this term in its true literal meaning. We of the CHURCH OF THE CREATOR want to differentiate this term from "Natural Hygiene popularly used for many decades by health practitioners devoted to this worthy art and science. -
The Composition of the Lunar Crust: Radiative Transfer Modeling and Analysis of Lunar Visible and Near-Infrared Spectra
THE COMPOSITION OF THE LUNAR CRUST: RADIATIVE TRANSFER MODELING AND ANALYSIS OF LUNAR VISIBLE AND NEAR-INFRARED SPECTRA A DISSERTATION SUBMITTED TO THE GRADUATE DIVISION OF THE UNIVERSITY OF HAWAI‘I IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF DOCTOR OF PHILOSOPHY IN GEOLOGY AND GEOPHYSICS DECEMBER 2009 By Joshua T.S. Cahill Dissertation Committee: Paul G. Lucey, Chairperson G. Jeffrey Taylor Patricia Fryer Jeffrey J. Gillis-Davis Trevor Sorensen Student: Joshua T.S. Cahill Student ID#: 1565-1460 Field: Geology and Geophysics Graduation date: December 2009 Title: The Composition of the Lunar Crust: Radiative Transfer Modeling and Analysis of Lunar Visible and Near-Infrared Spectra We certify that we have read this dissertation and that, in our opinion, it is satisfactory in scope and quality as a dissertation for the degree of Doctor of Philosophy in Geology and Geophysics. Dissertation Committee: Names Signatures Paul G. Lucey, Chairperson ____________________________ G. Jeffrey Taylor ____________________________ Jeffrey J. Gillis-Davis ____________________________ Patricia Fryer ____________________________ Trevor Sorensen ____________________________ ACKNOWLEDGEMENTS I must first express my love and appreciation to my family. Thank you to my wife Karen for providing love, support, and perspective. And to our little girl Maggie who only recently became part of our family and has already provided priceless memories in the form of beautiful smiles, belly laughs, and little bear hugs. The two of you provided me with the most meaningful reasons to push towards the "finish line". I would also like to thank my immediate and extended family. Many of them do not fully understand much about what I do, but support the endeavor acknowledging that if it is something I’m willing to put this much effort into, it must be worthwhile. -
South Pole-Aitken Basin
Feasibility Assessment of All Science Concepts within South Pole-Aitken Basin INTRODUCTION While most of the NRC 2007 Science Concepts can be investigated across the Moon, this chapter will focus on specifically how they can be addressed in the South Pole-Aitken Basin (SPA). SPA is potentially the largest impact crater in the Solar System (Stuart-Alexander, 1978), and covers most of the central southern farside (see Fig. 8.1). SPA is both topographically and compositionally distinct from the rest of the Moon, as well as potentially being the oldest identifiable structure on the surface (e.g., Jolliff et al., 2003). Determining the age of SPA was explicitly cited by the National Research Council (2007) as their second priority out of 35 goals. A major finding of our study is that nearly all science goals can be addressed within SPA. As the lunar south pole has many engineering advantages over other locations (e.g., areas with enhanced illumination and little temperature variation, hydrogen deposits), it has been proposed as a site for a future human lunar outpost. If this were to be the case, SPA would be the closest major geologic feature, and thus the primary target for long-distance traverses from the outpost. Clark et al. (2008) described four long traverses from the center of SPA going to Olivine Hill (Pieters et al., 2001), Oppenheimer Basin, Mare Ingenii, and Schrödinger Basin, with a stop at the South Pole. This chapter will identify other potential sites for future exploration across SPA, highlighting sites with both great scientific potential and proximity to the lunar South Pole. -
July 2019 Medicine’S Lunar Legacies • René T
OslerianaA Medical Humanities Journal-Magazine Volume 1 • July 2019 Medicine’s Lunar Legacies • René T. H. Laennec Walter R. Bett • Leonardo da Vinci OslerianaA Medical Humanities Journal-Magazine Editor-in-Chief Nadeem Toodayan MBBS Associate Editor Zaheer Toodayan MBBS Corrigendum: As indicated in the introductory piece to this journal and in footnotes to their respective articles, both editors are Basic Physician Trainees and therefore registered members of the Royal Australasian College of Physicians (RACP). In the initial printing of this volume (on this inner cover and on page 5) the postnominal of ‘MRACP’ was used to refer to the editors’ membership status. This postnominal was first applied to the Edi- tor-in-Chief in formal correspondence from The Osler Club of London. Subsequent discussions with the RACP have confirmed that the postnominal is not formally endorsed by the College for trainee members and so it has been removed in this digital edition. Osleriana – Volume 1 Published July 2019 © The William Osler Society of Australia & New Zealand (WOSANZ) e-mail: [email protected] All rights reserved. No part of this publication may be reproduced, stored in a retrieval system, or transmitted in any form or by any means, digital, print, photocopy, recording or otherwise, without the prior written permission of WOSANZ or the individual author(s). Permission to reproduce any copyrighted images used in this publication must be obtained from the appropriate rightsholder(s). Please contact WOSANZ for further information as required. Privately printed in Brisbane, Queensland, by Clark & Mackay Printers. Journal concept and WOSANZ logo by Nadeem Toodayan. Journal design and layout by Zaheer Toodayan. -
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. -
Index to JRASC Volumes 61-90 (PDF)
THE ROYAL ASTRONOMICAL SOCIETY OF CANADA GENERAL INDEX to the JOURNAL 1967–1996 Volumes 61 to 90 inclusive (including the NATIONAL NEWSLETTER, NATIONAL NEWSLETTER/BULLETIN, and BULLETIN) Compiled by Beverly Miskolczi and David Turner* * Editor of the Journal 1994–2000 Layout and Production by David Lane Published by and Copyright 2002 by The Royal Astronomical Society of Canada 136 Dupont Street Toronto, Ontario, M5R 1V2 Canada www.rasc.ca — [email protected] Table of Contents Preface ....................................................................................2 Volume Number Reference ...................................................3 Subject Index Reference ........................................................4 Subject Index ..........................................................................7 Author Index ..................................................................... 121 Abstracts of Papers Presented at Annual Meetings of the National Committee for Canada of the I.A.U. (1967–1970) and Canadian Astronomical Society (1971–1996) .......................................................................168 Abstracts of Papers Presented at the Annual General Assembly of the Royal Astronomical Society of Canada (1969–1996) ...........................................................207 JRASC Index (1967-1996) Page 1 PREFACE The last cumulative Index to the Journal, published in 1971, was compiled by Ruth J. Northcott and assembled for publication by Helen Sawyer Hogg. It included all articles published in the Journal during the interval 1932–1966, Volumes 26–60. In the intervening years the Journal has undergone a variety of changes. In 1970 the National Newsletter was published along with the Journal, being bound with the regular pages of the Journal. In 1978 the National Newsletter was physically separated but still included with the Journal, and in 1989 it became simply the Newsletter/Bulletin and in 1991 the Bulletin. That continued until the eventual merger of the two publications into the new Journal in 1997. -
Phacomatosis Pigmentokeratotica Complicated with Juvenile Onset Hypertension
Acta Derm Venereol 2004; 84: 397–416 LETTERS TO THE EDITOR Phacomatosis Pigmentokeratotica Complicated with Juvenile Onset Hypertension Etsuko Okada*, Atsushi Tamura and Osamu Ishikawa Department of Dermatology, Gunma University Graduate School of Medicine, 3-39-22 Showa-machi, Maebashi, Gunma 371-8511, Japan. *E-mail: [email protected] Accepted January 20, 2004. Sir, left orbit. The result of an electroencephalogram was The association of a speckled lentiginous naevus, an normal. organoid naevus with sebaceous differentiation and We performed surgical resections of several skin skeletal and neurological anomalies, constitutes a lesions. Histological studies of the verrucous plaques of specific syndrome that has been called phacomatosis the face showed hyperkeratosis and papillomatous pigmentokeratotica (1). hyperplasia of the epidermis. Numerous mature seb- It has been hypothesized that the co-occurrence of aceous glands were present in the upper dermis. The the two different naevi reflects a so-called twin spot histological findings of the plaques of the head and phenomenon (1 – 3). We herein describe an additional back were almost the same as those of the face, being case with this rare condition, consisting of organoid consistent with naevus sebaceous. epidermal naevus, speckled lentiginous naevus, micro- phthalmia, kyphoscoliosis, arachnoid cyst, solid tumours at the spinal roots and, in particular, juvenile DISCUSSION hypertension. The epidermal naevus syndromes include different diseases that have the common feature of mosaicism. Among these phenotypes, the Proteus, CHILD, naevus CASE REPORT comedonicus, Becker naevus and Schimmelpenning syndromes have been delineated (2). Happle et al. (1) An 18-year-old Japanese man presented with verrucous proposed phacomatosis pigmentokeratotica as the plaques on his head, which had been noted at birth and name for a distinct type of epidermal naevus syndrome became verrucous at puberty. -
Modeling Polarimetric Radar Scattering from the Lunar Surface: Study on the Effect of Physical Properties of the Regolith Layer Wenzhe Fa, Mark Wieczorek, Essam Heggy
Modeling polarimetric radar scattering from the lunar surface: Study on the effect of physical properties of the regolith layer Wenzhe Fa, Mark Wieczorek, Essam Heggy To cite this version: Wenzhe Fa, Mark Wieczorek, Essam Heggy. Modeling polarimetric radar scattering from the lunar sur- face: Study on the effect of physical properties of the regolith layer. Journal of Geophysical Research. Planets, Wiley-Blackwell, 2011, 116 (E3), pp.E03005. 10.1029/2010JE003649. hal-02458568 HAL Id: hal-02458568 https://hal.archives-ouvertes.fr/hal-02458568 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. JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 116, E03005, doi:10.1029/2010JE003649, 2011 Modeling polarimetric radar scattering from the lunar surface: Study on the effect of physical properties of the regolith layer Wenzhe Fa,1 Mark A. Wieczorek,1 and Essam Heggy1,2 Received 10 May 2010; revised 21 November 2010; accepted 15 December 2010; published 5 March 2011. [1] A theoretical model for radar scattering from the lunar regolith using the vector radiative transfer theory for random media has been developed in order to aid in the interpretation of Mini‐SAR data from the Chandrayaan‐1 and Lunar Reconnaissance Orbiter missions. -
2019 APS/CNM USERS MEETING Program and Abstracts
MAY 2019 2019 APS/CNM USERS MEETING Program and Abstracts 2019 APS/CNM USERS MEETING APS/CNM 2019 USERS MEETING PROGRAM AND ABSTRACTS I PROGRAM AND abstracts User Facilities at Argonne National Laboratory User Contacts Advanced Photon Source http://www.aps.anl.gov 630-252-9090 [email protected] Argonne Leadership Computing Facility http://www.alcf.anl.gov 630-252-0929 Argonne Tandem Linac Accelerator System http://www.phy.anl.gov/atlas 630-252-4044 Center for Nanoscale Materials http://nano.anl.gov 630-252-6952 [email protected] II 2019 APS/CNM USERS MEETING Table of Contents Comprehensive Program .........................................................................................................................................................................1 General Session Abstracts .................................................................................................................................................................... 15 Workshop Agendas and Abstracts ..................................................................................................................................................... 23 WK1 Joint APS/CNM: Driving Scientific Discovery with Artificial Intelligence, Advanced Data Analysis, and Data Management in the APS-U Era ............................................................................................. 25 WK2 Joint APS/CNM: Topological Quantum Information Science .......................................................................................... 30 WK3 APS: Workshop -
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. -
Arxiv:1403.6528V1 [Astro-Ph.IM] 25 Mar 2014
25 Years of Self-Organized Criticality: Solar and Astrophysics Markus J. Aschwanden Lockheed Martin, Solar and Astrophysics Laboratory (LMSAL), Advanced Technology Center (ATC), A021S, Bldg.252, 3251 Hanover St., Palo Alto, CA 94304, USA; e-mail: [email protected] Norma Crosby Belgian Institute for Space Aeronomy, Ringlaan-3-Avenue Circulaire, B-1180 Brussels, Belgium Michaila Dimitropoulou Kapodistrian University of Athens, Dept. Physics, 15483, Athens, Greece Manolis K. Georgoulis Research Center Astronomy and Applied Mathematics, Academy of Athens, 4 Soranou Efesiou St., Athens, Greece, GR-11527. Stefan Hergarten Institute f¨ur Geo- und Umweltnaturwissenschaften, Albert-Ludwigs-Universit¨at Freiburg, Albertstr. 23B, 79104 Freiburg, Germany James McAteer Dept. Astronomy, P.O.Box 30001, New Mexico State University, MSC 4500, Las Cruces, USA Alexander V. Milovanov Associazione EURATOM-ENEA sulla Fusione, Italian National Agency for New Technologies, Frascati Research Centre, Via E. Fermi 45, C.P.-65, I-00044 Frascati, Rome, Italy; Space Research Institute, Russian Academy of Sciences, Profsoyuznaya str. 84/32, 117997 Moscow, Russia; Max Planck Institute for the Physics of Complex Systems, Noethnitzer Str. 38, 01187 Dresden, Germany Shin Mineshige Dept. Astronomy, Kyoto University, Kyoto 606-8602, Japan arXiv:1403.6528v1 [astro-ph.IM] 25 Mar 2014 Laura Morales Canadian Space Agency, Space Science and Technology Branch, 6767 Route de l’Aeroport, Saint Hubert, Quebec, J3Y8Y9, Canada Naoto Nishizuka Inst. Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Kanagawa, 252-5210, Japan Gunnar Pruessner Dept. Mathematics, Imperial College London, 180 Queen’s Gate, London SW7 2AZ, United Kingdom Raul Sanchez –2– Dept. Fisica, Universidad Carlos III de Madrid, Avda.