Ubiquitous Argonium \(Arh+\) in the Diffuse Interstellar Medium: A
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Greek Sculpture and the Four Elements Art
University of Massachusetts Amherst ScholarWorks@UMass Amherst Greek Sculpture and the Four Elements Art 7-1-2000 Greek Sculpture and the Four Elements [full text, not including figures] J.L. Benson University of Massachusetts Amherst Follow this and additional works at: https://scholarworks.umass.edu/art_jbgs Part of the History of Art, Architecture, and Archaeology Commons Benson, J.L., "Greek Sculpture and the Four Elements [full text, not including figures]" (2000). Greek Sculpture and the Four Elements. 1. Retrieved from https://scholarworks.umass.edu/art_jbgs/1 This Article is brought to you for free and open access by the Art at ScholarWorks@UMass Amherst. It has been accepted for inclusion in Greek Sculpture and the Four Elements by an authorized administrator of ScholarWorks@UMass Amherst. For more information, please contact [email protected]. Cover design by Jeff Belizaire About this book This is one part of the first comprehensive study of the development of Greek sculpture and painting with the aim of enriching the usual stylistic-sociological approaches through a serious, disciplined consideration of the basic Greek scientific orientation to the world. This world view, known as the Four Elements Theory, came to specific formulation at the same time as the perfected contrapposto of Polykleitos and a concern with the four root colors in painting (Polygnotos). All these factors are found to be intimately intertwined, for, at this stage of human culture, the spheres of science and art were not so drastically differentiated as in our era. The world of the four elements involved the concepts of polarity and complementarism at every level. -
The Art of Hans Arp After 1945
Stiftung Arp e. V. Papers The Art of Hans Arp after 1945 Volume 2 Edited by Jana Teuscher and Loretta Würtenberger Stiftung Arp e. V. Papers Volume 2 The Art of Arp after 1945 Edited by Jana Teuscher and Loretta Würtenberger Table of Contents 10 Director’s Foreword Engelbert Büning 12 Foreword Jana Teuscher and Loretta Würtenberger 16 The Art of Hans Arp after 1945 An Introduction Maike Steinkamp 25 At the Threshold of a New Sculpture On the Development of Arp’s Sculptural Principles in the Threshold Sculptures Jan Giebel 41 On Forest Wheels and Forest Giants A Series of Sculptures by Hans Arp 1961 – 1964 Simona Martinoli 60 People are like Flies Hans Arp, Camille Bryen, and Abhumanism Isabelle Ewig 80 “Cher Maître” Lygia Clark and Hans Arp’s Concept of Concrete Art Heloisa Espada 88 Organic Form, Hapticity and Space as a Primary Being The Polish Neo-Avant-Garde and Hans Arp Marta Smolińska 108 Arp’s Mysticism Rudolf Suter 125 Arp’s “Moods” from Dada to Experimental Poetry The Late Poetry in Dialogue with the New Avant-Gardes Agathe Mareuge 139 Families of Mind — Families of Forms Hans Arp, Alvar Aalto, and a Case of Artistic Influence Eeva-Liisa Pelkonen 157 Movement — Space Arp & Architecture Dick van Gameren 174 Contributors 178 Photo Credits 9 Director’s Foreword Engelbert Büning Hans Arp’s late work after 1945 can only be understood in the context of the horrific three decades that preceded it. The First World War, the catastro- phe of the century, and the Second World War that followed shortly thereaf- ter, were finally over. -
Ubiquitous Argonium, Arh+, in the Diffuse Interstellar Medium
Ubiquitous Argonium, ArH+, in the Interstellar Medium P. Schilke, Holger S. P. Müller, C. Comito, Á. Sánchez-Monge, D. A. Neufeld, N. Indriolo, E. A. Bergin, D. C. Lis, M. Gerin, J. H. Black, M. G. Wolfire, J. C. Pearson, K. M. Menten, B. Winkel V.6, 13th International HITRAN Conference, CfA, Cambridge, MA, USA, June 23–25, 2014 What is Argonium? ArH+, 1Σ+, isoelectronic to HCl + + Formation: Ar + H2 → ArH + H + + Destruction (e.g.): ArH + H2 → Ar + H3 Isotopic ratio: 36Ar : 38Ar : 40Ar terrestrial: 84.2 : 15.8 : 25018.8 (from decay of 40K) solar/ISM: ~84.6 : ~15.4 : 0.025 36ArH+ toward Crab Nebula SNR: J = 1 – 0 & 2 – 1 in emission (w. OH+ N = 1 – 0); SPIRE/Herschel M. J. Barlow et al., Science 342 (2013) 1343 On the Spectroscopy of ArH+ 40ArH+; rotational spectroscopy: K. B. Laughlin et al., PRL 58 (1987) 996: J" = 0 J. M. Brown et al., JMSp 128 (1988) 587: J" = 1 – 6 D. J. Liu et al., JCP 87 (1987) 2442: J" = 20 – 24; v ≤ 4 (MIR) 40ArD+; rotational spectroscopy: W. C. Bowman et al., JCP 79 (1983) 2093: J" = 0 (+ 36ArD+ & 38ArD+ H. Odashima et al., JMSp 195 (1999) 356: J" = 2 – 14 rovibrational spectroscopy: J. W. Brault & S. P. Davis, Phys. Sript. 25 (1982) 268: 40ArH+ J. W. C. Johns, JMSp 106 (1984) 124: 40ArH+, 40ArD+ R. R. Filueira & C. E. Blom, JMSp 127 (1988) 279: 36ArH+, 38ArH+ M. Cueto et al., ApJ 783 (2014) L5: 36ArH+, 38ArH+ ArH+ toward Sagittarius B2(M) – HIFI Line Survey Absorption toward Sgr B2(M) massive star-forming regions as background sources with approximate origins Sagittarius B2(M) Interstellar Chemistry of ArH+ I + + + + Ar + H2 → ArH + H exothermic (endo. -
User Guide Multi Processor FX
MPX 1 Multi Processor FX User Guide Unpacking and Inspection After unpacking the MPX 1, save all packing materials in case you ever need to ship the unit. Thoroughly inspect the unit and packing materials for signs of damage. Report any shipment damage to the carrier at once; report equipment malfunction to your dealer. Precautions Save these instructions for later use. Follow all instructions and warnings marked on the unit. Always use with the correct line voltage. Refer to the manufacturer's operating instructions for power requirements. Be advised that different operating voltages may require the use of a different line cord and/or attachment plug. Do not install the unit in an unventilated rack, or directly above heat producing equipment such as power amplifiers. Observe the maximum ambient operating temperature listed in the product specification. Slots and openings on the case are provided for ventilation; to ensure reliable operation and prevent it from overheating, these openings must not be blocked or covered. Never push objects of any kind through any of the ventilation slots. Never spill a liquid of any kind on the unit. This product is equipped with a 3-wire grounding type plug. This is a safety feature and should not be defeated. Never attach audio power amplifier outputs directly to any of the unit's connectors. To prevent shock or fire hazard, do not expose the unit to rain or moisture, or operate it where it will be exposed to water. Do not attempt to operate the unit if it has been dropped, damaged, exposed to liquids, or if it exhibits a distinct change in performance indicating the need for service. -
Detection of Extragalactic Argonium, Arh+, Toward PKS 1830−211⋆
A&A 582, L4 (2015) Astronomy DOI: 10.1051/0004-6361/201527254 & c ESO 2015 Astrophysics Letter to the Editor Detection of extragalactic argonium, ArH+, toward PKS 1830−211 Holger S. P. Müller1, Sébastien Muller2, Peter Schilke1, Edwin A. Bergin3, John H. Black2, Maryvonne Gerin4, Dariusz C. Lis5,6, David A. Neufeld7, and Sümeyye Suri1 1 I. Physikalisches Institut, Universität zu Köln, Zülpicher Str. 77, 50937 Köln, Germany e-mail: [email protected] 2 Department of Earth and Space Sciences, Chalmers University of Technology, Onsala Space Observatory, 43992 Onsala, Sweden 3 Department of Astronomy, The University of Michigan, 500 Church Street, Ann Arbor, MI 48109-1042, USA 4 LERMA, Observatoire de Paris, PSL Research University, CNRS, Sorbonne Universités, UPMC Univ. Paris 06, École normale supérieure, 75005 Paris, France 5 LERMA, Observatoire de Paris, PSL Research University, CNRS, Sorbonne Universités, UPMC Univ. Paris 06, 75014 Paris, France 6 Cahill Center for Astronomy and Astrophysics 301-17, California Institute of Technology, Pasadena, CA 91125, USA 7 Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD 21218, USA Received 26 August 2015 / Accepted 22 September 2015 ABSTRACT Context. Argonium has recently been detected as a ubiquitous molecule in our Galaxy. Model calculations indicate that its abundance peaks at molecular fractions in the range of 10−4 to 10−3 and that the observed column densities require high values of the cosmic ray ionization rate. Therefore, this molecular cation may serve as an excellent tracer of the very diffuse interstellar medium (ISM), as well as an indicator of the cosmic ray ionization rate. -
Primordially Hydridic Earth Viacheslav Zgonnik, Hervé Toulhoat, Vladimir Larin, Nikolay Larin
Primordially hydridic Earth Viacheslav Zgonnik, Hervé Toulhoat, Vladimir Larin, Nikolay Larin Abundances of elements on Earth’s crust relative to Sun’s photosphere and Si plotted versus first ionization potential (IP) • Clearly shows separation of elements by their IP • Outliers are due to use of only Earth’s crust composition • Tested with success for other planets, Moon and asteroids • Described by a Boltzmann distribution depending on the distance to the protosun • Predicts high initial content of hydrogen • Earth currently has about 4% by weight of hydrogen. • It is mainly combined as hydrides and partly dissolved into other phases http://arxiv.org/abs/1208.2909v2 Non-Ionizing UV (< 7 eV) Photochemistry of Cosmic Ice Analogs of Ammonia Radiolysis involves electron Photochemistry involves electron excitation due to particle radiation excitation without ionization in addition to all ionization – reactions initiated by cations – production of low-energy electron cascade – non-uniform distribution of reaction intermediates, non-selective chemistry leading to multiple reaction products We see production of N2 and N3 species with high- energy electrons and < 8 eV photons, but not with < 6 eV photons Islem Bouhali Soumaya Bezzaouia Mourad Telmini Theoretical study of Rydberg states of HeH+ ion using the Halfium model Christian Jungen Presented by: Islem Bouhali 2 HeH+ molecular ion in Born-Oppenheimer approximation e2 r12 Max(extern region e1 r2a GMQDT r r 1a 2b r1b Max(reaction surface R MATCHING ++ + He H Max( : reaction volume R-MATRIX Combination of the Variational R-matrix method and of the Generalized Multichannel Quantum Defect Theory Telmini and Jungen, Phys. Rev. A 68 062704 (2003). -
Days & Hours for Social Distance Walking Visitor Guidelines Lynden
53 22 D 4 21 8 48 9 38 NORTH 41 3 C 33 34 E 32 46 47 24 45 26 28 14 52 37 12 25 11 19 7 36 20 10 35 2 PARKING 40 39 50 6 5 51 15 17 27 1 44 13 30 18 G 29 16 43 23 PARKING F GARDEN 31 EXIT ENTRANCE BROWN DEER ROAD Lynden Sculpture Garden Visitor Guidelines NO CLIMBING ON SCULPTURE 2145 W. Brown Deer Rd. Do not climb on the sculptures. They are works of art, just as you would find in an indoor art Milwaukee, WI 53217 museum, and are subject to the same issues of deterioration – and they endure the vagaries of our harsh climate. Many of the works have already spent nearly half a century outdoors 414-446-8794 and are quite fragile. Please be gentle with our art. LAKES & POND There is no wading, swimming or fishing allowed in the lakes or pond. Please do not throw For virtual tours of the anything into these bodies of water. VEGETATION & WILDLIFE sculpture collection and Please do not pick our flowers, fruits, or grasses, or climb the trees. We want every visitor to be able to enjoy the same views you have experienced. Protect our wildlife: do not feed, temporary installations, chase or touch fish, ducks, geese, frogs, turtles or other wildlife. visit: lynden.tours WEATHER All visitors must come inside immediately if there is any sign of lightning. PETS Pets are not allowed in the Lynden Sculpture Garden except on designated dog days. -
Astronomy in India
TRADITIONSKnowledg & PRACTICES OF INDIA e Textbook for Class XI Module 1 Astronomy in India CENTRAL BOARD OF SECONDARY EDUCATION Shiksha Kendra, 2, Community Centre, Preet Vihar, Delhi-110 092 India TRADITIONSKnowledg & PRACTICESe OF INDIA Textbook for Class XI Module 1 Astronomy in India CENTRAL BOARD OF SECONDARY EDUCATION Shiksha Kendra, 2, Community Centre, Preet Vihar, Delhi-110 092 India No part of this publication may be reproduced or stored in a retrieval system or transmitted in any form or by any means, electronic, mechanical photocopying, recording or otherwise, without the prior permission of the Central Board of Secondary Education (CBSE). Preface India has a rich tradition of intellectual inquiry and a textual heritage that goes back to several hundreds of years. India was magnificently advanced in knowledge traditions and practices during the ancient and medieval times. The intellectual achievements of Indian thought are found across several fields of study in ancient Indian texts ranging from the Vedas and the Upanishads to a whole range of scriptural, philosophical, scientific, technical and artistic sources. As knowledge of India's traditions and practices has become restricted to a few erudite scholars who have worked in isolation, CBSE seeks to introduce a course in which an effort is made to make it common knowledge once again. Moreover, during its academic interactions and debates at key meetings with scholars and experts, it was decided that CBSE may introduce a course titled ‘Knowledge Traditions and Practices of India’ as a new Elective for classes XI - XII from the year 2012-13. It has been felt that there are many advantages of introducing such a course in our education system. -
The Prospects for Petroleum Exploration in the Eastern Sector of Southern Baltic As Revealed by Sea Bottom Geochemical Survey Correlated with Seismic Data
Przegl¹d Geologiczny, vol. 52, no. 8/2, 2004 The prospects for petroleum exploration in the eastern sector of Southern Baltic as revealed by sea bottom geochemical survey correlated with seismic data Jerzy Dom¿alski*, Wojciech Górecki**, Andrzej Mazurek*, Andrzej Myœko**, Wojciech Strzetelski**, Krzysztof Szama³ek*** A b s t r a c t . In the Polish offshore £eba (B) tectonic block in the southeastern part of the Baltic Sea the oil and gas fields are accumu- lated in Middle Cambrian quartzose sandstone, often fractured and diagenetically sealed at depth by advanced silification developed in reservoir around the petroleum deposit. Petroleum traps are mainly of structure-tectonic type, i.e., anticlines closed with strike-slip faults. At least four gas-condensate and four oil deposits of total reserves more than 10 Gm3 gas and 30 Mt oil were discovered by the “Petrobaltic” Co. in the Polish Baltic sector. The subsurface petroleum deposits in the Cambrian reservoir are the source of secondary vertical hydrocarbon migration to the surface which produces surface microseepages and hydrocarbon anomalies. Geochemical survey of the sea bottom sediments and waters run along seismic profiles was completed in 1999–2002 within a joint project of “Petrobaltic” Co. Gdañsk and the Fossil Fuels Dept., AGH University of Science and Technology, Kraków, approved by the Ministry of Environmental Protection, Natural Resources and Forestry. It was found that seafloor hydrocarbon anomalies are closely related to subsurface geologic structure and location of petroleum deposits. Particularly the faults as principal venues for vertical hydrocarbon migration are reflected in high-magnitude seafloor anomalies. Above petroleum field there occurs a “halo” effect of high-magnitude anomalies contouring the deposit with damping related to productive zone situated inbetween. -
Microwave Spectroscopy Information Letter Vol
MICROWAVE SPECTROSCOPY INFORMATION LETTER VOL. LXI April 15, 2018 Compiled By: Garry S. Grubbs II Asst. Professor of Chemistry Department of Chemistry Missouri Univ. of Science & Technology 400 W. 11th St. Rolla, MO, 65409 [email protected] MICROWAVE SPECTROSCOPY NEWSLETTER LXI List of Contributors / Table of Contents Contributor Institution Lab, Page No. Alonso, J. L. Universidad de Valladolid 1, 5 Arunan, E. India Institute of Science, Bangalore 2, 7 Bird, R. University of Pittsburgh, Johnstown 3, 8 Bizzocchi, L. Max Planck Inst. for Extraterrestrial Physics 33, 103 Blanco, S. Universidad de Valladolid 31, 94 Bohn, R. K. University of Connecticut 4, 9 Brown, G. Coker College 5, 11 Caselli, P. Max Planck Inst. for Extraterrestrial Physics 33, 103 Christen, D. Institut für Physikalische Chemie, Tübingen 6, 13 Cocinero, E. Universidad del País Vasco 7, 14 Cooke, S. A. Purchase College SUNY 8, 17 Dore, L. Università di Bologna 40, 124 Douglass, K. O. National Institute of Standards and Technology 32, 98 Drouin, B. Jet Propulsion Laboratory, Pasadena 9, 21 Durig, J. R. University of Missouri, Kansas City 14, 44 Esposti, C. D. Università di Bologna 10, 23 Evangelisti, L. Università di Bologna 10, 23 Favero, L. B. Università di Bologna 10, 23 Feng, G. Chongqing University 12, 33 Fujitake, M. Kanazawa University 11, 30 Gou, Qian Chongqing University 12, 33 Grabow, J.-U. Institut für Physikalische Chemie, Hannover 13, 36 Groner, P. University of Missouri, Kansas City 14, 44 Grubbs, G. Missouri University of Science & Technology 15, 45 Harada, K. Kyushu University 16, 49 Hirota, E. Grad. Univ. for Advanced Studies, Kanagawa 17, 53 Ilyushin, V. -
User's Guide to Vertical Control and Geodetic Leveling for CO-OPS
User’s Guide to Vertical Control and Geodetic Leveling for CO-OPS Observing Systems by Minilek Hailegeberel, Kirk Glassmire, Artara Johnson, Manoj Samant, and Gregory Dusek Center for Operational Oceanographic Products and Services Silver Spring, MD May 2018 Acknowledgements Major portions of the publications of Steacy D. Hicks, Philip C. Morris, Harry A. Lippincott, and Michael C. O'Hargan have been included as well as from the older publication by Ralph M. Berry, John D. Bossler, Richard P. Floyd, and Christine M. Schomaker. These portions are both direct or adapted, and cited or inferred. Complete references to these publications are listed at the end of this document. A CO-OPS Vertical Control Committee was created in 2017 to update, with current practices, the 1984 Users Guide for Installation of Bench Marks. The committee met on a bi-weekly basis to document current practices and procedures for installing and surveying of bench marks. Through many months of collaborative efforts with National Geospatial Survey, the committee provided their input into this guide. The committee’s participation in writing this document is greatly appreciated. Vertical Control Committee Group Members Artara Johnson (CO-OPS) Mark Bailey (CO-OPS) Dan Roman (NGS) Michael Michalski (CO-OPS) Gregory Dusek (CO-OPS) Peter Stone (CO-OPS) Jeff Oyler (CO-OPS) Philippe Hensel (NGS) John Stepnowski (CO-OPS) Rick Foote (NGS) Kirk Glassmire (CO-OPS) Robert Loesch (CO-OPS) Laura Rear McLaughlin (CO-OPS) Ryan Hippenstiel (NGS) Manoj Samant (CO-OPS) The authors are especially grateful for Manoj Samant and Gregory Dusek for providing content as well as providing numerous edits into this guide. -
Special Project Progress Report
SPECIAL PROJECT PROGRESS REPORT All the following mandatory information needs to be provided. The length should reflect the complexity and duration of the project. Reporting year 2019 Project Title: Investigation of case studies using COSMO-based deterministic and ensemble systems Computer Project Account: spcoleps Principal Investigator(s): Montani Andrea (until 30/5/2019) Cerenzia Ines (hereafter) Affiliation: Arpae-SIMC Servizio IdroMeteoClima, Viale Silvani 6 40122 Bologna (Italy) Name of ECMWF scientist(s) ……………………………………………………….…… collaborating to the project (if applicable) ……………………………………………………….…… Start date of the project: 2018 Expected end date: 2020 Computer resources allocated/used for the current year and the previous one (if applicable) Please answer for all project resources Previous year Current year Allocated Used Allocated Used High Performance (units) 2.100.000 1.636.468 2.100.000 0 Computing Facility Data storage capacity (Gbytes) 600 600 600 0 July 2019 This template is available at: http://www.ecmwf.int/en/computing/access-computing-facilities/forms Summary of project objectives (10 lines max) To assess the sensitivity of model performance of horizontal resolution and, in particular, to the use of parameterised or explicit convection. Summary of problems encountered (10 lines max) …………………………………………………………………………………………………………… …………………………………………………………………………………………………………… …………………………………………………………………………………………………………… …………………………………………………………………………………………………………… …………………….... Summary of plans for the continuation of the project (10