Entropy Control in Discrete- and Continuous-Time Dynamic Systems S
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The Ball Lightning Conundrum
most famous deadis due to ball lightning occun-ed in 1752 or 1753, when die Swedish sci entist Professor Georg Wilhelm Richman was The Ball attempting to repeat Benjamin Franklin's observa dons with a lightning rcxl. An eyewitness report ed that when Richman w;is "a foot away from the iron rod, the] looked at die elecuical indicator Lightning again; just then a palish blue ball of fire, ;LS big as a fist, came out of die rod without any contaa whatst:)ever. It went right to the forehead of die Conundrum professor , who in diat instant fell back without uttering a sound."' Somedmes a luminous globe is said to rapidly descend 6own die path of a linear lightning WILLIAM D STANSFIELD strike and stop near the ground at die impact site. It may dien hover motionless in mid-air or THE EXISTENCE OF BALL UGHTNING HAS move randomly, but most often horizontally, at been questioned for hundreds of years. Today, die relatively slow velocities of walking speed. the phenomenon is a realit>' accepted by most Sometimes it touches or bounces along or near scientists, but how it is foniied and maintiiined the ground, or travels inside buildings, along has yet to be tully explained. Uncritical observers walls, or over floors before being extingui.shed. of a wide variety of glowing atmospheric entities Some balls have been observed to travel along may be prone to call tliem bail lightning. Open- power lines or fences. Wind does not .seem to minded skepdas might wish to delay judgment have any influence on how diese balls move. -
SCIENCE ORGANIZING COMMITTEE Patrick Pinet IRAP, Toulouse
SCIENCE ORGANIZING COMMITTEE Patrick Pinet IRAP, Toulouse University, France (Chair) Mahesh Anand Open University, UK (Co-Chair) James Carpenter Ana Cernok LOCAL ORGANIZING COMMITTEE Patrick Pinet Serge Chevrel Serge Chevrel Doris Daou Marie-Ange Albouy Simone Pirrotta Gaël David Yves Daydou Kristina Gibbs Dolorès Granat Harry Hiesinger Jérémie Lasue Greg Schmidt Alice Stephant Wim van Westrenen 2 Updated: 2 May 2018 European Lunar Symposium Toulouse 2018 Meeting information Welcome to Toulouse at the Sixth European Lunar Symposium (ELS)! We are hoping to have a great meeting, demonstrating the diversity of the current lunar research in Europe and elsewhere, and continuing to provide a platform to the European lunar researchers for networking as well as exchanging news ideas and latest results in the field of lunar exploration. We acknowledge the support of Toulouse University and NASA SSERVI (Solar System Exploration Research Virtual Institute). Our special thanks to our SSERVI colleagues, Kristina Gibbs, Jennifer Baer, Ashcon Nejad and to Dolorès Granat at IRAP (Institut de Recherche en Astrophysique et Planétologie)/ OMP (Observatoire Midi-Pyrénées) for their contribution to the meeting preparation and program implementation. Members of the Science Organizing Committee are thanked for their input in putting together an exciting program and for volunteering to chair various sessions in this meeting. Our special thanks for Ana Cernok and Alice Stephant from the Open University for putting together the abstract booklet. MEETING VENUE The ELS will take place at the museum of modern and contemporary art, called “Les Abattoirs”. It is located in the center of Toulouse, close to the “Garonne” river. The street address is 76 Allées Charles de Fitte, 31300 Toulouse. -
Ball Lightning As a Self- Organized Complexity
Ball Lightning as a Self- Organized Complexity Erzilia Lozneanu, Sebastian Popescu and Mircea Sanduloviciu Department of Plasma Physics “Al. I. Cuza” University 6600 Iasi, Romania [email protected] The ball lightning phenomenon is explained in the frame of a self-organization scenario suggested by experiments performed on the spontaneously generated complex spherical space charge configuration in plasma. Originated in a hot plasma, suddenly created in a point where a lightning flash strikes the Earth surface, the ball lightning appearance proves the ability of nature to generate, by self-organization, complex structures able to ensure their own existence by exchange of matter and energy with the surroundings. Their subsequent evolution depends on the environment where they are born. Under contemporary Earth conditions the lifetime of such complexities is relatively short. A similar self-organization mechanism, produced by simple sparks in the earl Earth's atmosphere (chemically reactive plasma) is suggested to explain the genesis of complexities able to evolve into prebiotic structures. 1. Introduction The enigmatic ball lightning phenomenon has stimulated the people interest for a very long time. Thus the ball lightning appearance was noted with more than a hundred years ago in prestigious periodicals as for example “Nature”. The vast literature on ball lightning comprises books entirely dedicated to this subject [1-3], review papers focussed on this topic [4-7], as well as data banks. The data banks contain collections of characteristics for lightning balls that where occasionally observed under different circumstances. For example, in the United States, lightning balls have been observed by about 5% of the adult population at some time of their lives [8]. -
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. -
Using Fireballs to Uncover the Mysteries of Ball Lightning 18 February 2008, by Miranda Marquit
Using fireballs to uncover the mysteries of ball lightning 18 February 2008, By Miranda Marquit “People have been pondering ball lightning for a Mitchell explains, the accelerator for the synchrotron couple of centuries,” says James Brian Mitchell, a is more than a kilometer in circumference: “We can scientist the University of Rennes in France. get measurements here that we couldn’t get in Mitchell says that different theories of how it forms, many other places.” and why it burns in air, have been considered, but until now there were no experimental indications of “We passed an x-ray beam through the fireball we what might be happening as part of the ball made, and saw that it was scattered. This indicated lightning phenomenon. that there were particles inside the fireball.” Not only were Mitchell and his peers able to determine Now, working with fellow Rennes scientist that nanoparticles must exist in fireballs similar to LeGarrec, as well as Dikhtyar and Jerby from Tel ball lightning, but they were also able to take Aviv University and Sztucki and Narayanan at the measurements. “Particle size, density, distribution European Synchrotron Radiation Facility in and even decay rate were measured using this Grenoble, France, Mitchell can prove that technique,” he says. nanoparticles likely exist in ball lightning. The results of the work by Mitchell and his colleagues Mitchell’s work with fireballs isn’t finished. can be found in Physical Review Letters: When PhysOrg.com spoke to him for this article, he “Evidence for Nanoparticles in Microwave- was back in Grenoble taking more measurements. -
Lpi Summer Intern Program in Planetary Science
LPI SUMMER INTERN PROGRAM IN PLANETARY SCIENCE Papers Presented at the August 11, 2011 — Houston, Texas Papers Presented at the Twenty-Seventh Annual Summer Intern Conference August 11, 2011 Houston, Texas 2011 Summer Intern Program for Undergraduates Lunar and Planetary Institute Sponsored by Lunar and Planetary Institute NASA Johnson Space Center Compiled in 2011 by Meeting and Publication Services Lunar and Planetary Institute USRA Houston 3600 Bay Area Boulevard, Houston TX 77058-1113 The Lunar and Planetary Institute is operated by the Universities Space Research Association under a cooperative agreement with the Science Mission Directorate of the National Aeronautics and Space Administration. Any opinions, findings, and conclusions or recommendations expressed in this volume are those of the author(s) and do not necessarily reflect the views of the National Aeronautics and Space Administration. Material in this volume may be copied without restraint for library, abstract service, education, or personal research purposes; however, republication of any paper or portion thereof requires the written permission of the authors as well as the appropriate acknowledgment of this publication. 2011 Intern Conference iii HIGHLIGHTS Special Activities June 6, 2011 Tour of the Stardust Lab and Lunar Curatorial Facility JSC July 22, 2011 Tour of the Meteorite Lab JSC August 4, 2011 NASA VIP Tour JSC/ NASA Johnson Space Center and Sonny Carter SCTF Training Facility Site Visit Intern Brown Bag Seminars Date Speaker Topic Location June 8, 2011 Paul -
Adams Adkinson Aeschlimann Aisslinger Akkermann
BUSCAPRONTA www.buscapronta.com ARQUIVO 27 DE PESQUISAS GENEALÓGICAS 189 PÁGINAS – MÉDIA DE 60.800 SOBRENOMES/OCORRÊNCIA Para pesquisar, utilize a ferramenta EDITAR/LOCALIZAR do WORD. A cada vez que você clicar ENTER e aparecer o sobrenome pesquisado GRIFADO (FUNDO PRETO) corresponderá um endereço Internet correspondente que foi pesquisado por nossa equipe. Ao solicitar seus endereços de acesso Internet, informe o SOBRENOME PESQUISADO, o número do ARQUIVO BUSCAPRONTA DIV ou BUSCAPRONTA GEN correspondente e o número de vezes em que encontrou o SOBRENOME PESQUISADO. Número eventualmente existente à direita do sobrenome (e na mesma linha) indica número de pessoas com aquele sobrenome cujas informações genealógicas são apresentadas. O valor de cada endereço Internet solicitado está em nosso site www.buscapronta.com . Para dados especificamente de registros gerais pesquise nos arquivos BUSCAPRONTA DIV. ATENÇÃO: Quando pesquisar em nossos arquivos, ao digitar o sobrenome procurado, faça- o, sempre que julgar necessário, COM E SEM os acentos agudo, grave, circunflexo, crase, til e trema. Sobrenomes com (ç) cedilha, digite também somente com (c) ou com dois esses (ss). Sobrenomes com dois esses (ss), digite com somente um esse (s) e com (ç). (ZZ) digite, também (Z) e vice-versa. (LL) digite, também (L) e vice-versa. Van Wolfgang – pesquise Wolfgang (faça o mesmo com outros complementos: Van der, De la etc) Sobrenomes compostos ( Mendes Caldeira) pesquise separadamente: MENDES e depois CALDEIRA. Tendo dificuldade com caracter Ø HAMMERSHØY – pesquise HAMMERSH HØJBJERG – pesquise JBJERG BUSCAPRONTA não reproduz dados genealógicos das pessoas, sendo necessário acessar os documentos Internet correspondentes para obter tais dados e informações. DESEJAMOS PLENO SUCESSO EM SUA PESQUISA. -
An Experimental Model of Ball Lightning
University of Tennessee, Knoxville TRACE: Tennessee Research and Creative Exchange Masters Theses Graduate School 8-2004 An Experimental Model of Ball Lightning Madras Parameswaran Sriram University of Tennessee - Knoxville Follow this and additional works at: https://trace.tennessee.edu/utk_gradthes Part of the Electrical and Electronics Commons Recommended Citation Sriram, Madras Parameswaran, "An Experimental Model of Ball Lightning. " Master's Thesis, University of Tennessee, 2004. https://trace.tennessee.edu/utk_gradthes/2204 This Thesis is brought to you for free and open access by the Graduate School at TRACE: Tennessee Research and Creative Exchange. It has been accepted for inclusion in Masters Theses by an authorized administrator of TRACE: Tennessee Research and Creative Exchange. For more information, please contact [email protected]. To the Graduate Council: I am submitting herewith a thesis written by Madras Parameswaran Sriram entitled "An Experimental Model of Ball Lightning." I have examined the final electronic copy of this thesis for form and content and recommend that it be accepted in partial fulfillment of the equirr ements for the degree of Master of Science, with a major in Electrical Engineering. Igor Alexeff, Major Professor We have read this thesis and recommend its acceptance: Douglas J Birdwell, Paul B Crilly Accepted for the Council: Carolyn R. Hodges Vice Provost and Dean of the Graduate School (Original signatures are on file with official studentecor r ds.) To the Graduate Council: I am submitting herewith a thesis written by Madras Parameswaran Sriram entitled “An Experimental Model of Ball Lightning”. I have examined the final electronic copy of this thesis for form and content and recommend that it be accepted in partial fulfillment of the requirements for the degree of Master of Science, with a major in Electrical Engineering. -
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. -
Hazards to Aircraft Crews, Passengers, and Equipment from Thunderstorm-Generated X-Rays and Gamma-Rays
Review Hazards to Aircraft Crews, Passengers, and Equipment from Thunderstorm-Generated X-rays and Gamma-Rays Karl D. Stephan 1 and Mikhail L. Shmatov 2,* 1 Ingram School of Engineering, Texas State University, San Marcos, TX 78666, USA; [email protected] 2 Division of Solid State Electronics, Ioffe Institute, 194021 St. Petersburg, Russia * Correspondence: [email protected] Simple Summary: Until recently, it was not known that thunderstorms generate X-rays and gamma- rays, which are high-energy forms of ionizing radiation that can cause both physical harm to living organisms and damage to electronics. Over the last four decades, we have learned that thunderstorms produce X-rays during lightning strikes and also generate gamma-rays by processes that are not yet completely understood. This paper examines what is known about the sources of ionizing radiation associated with thunderstorms with a view to evaluating the possible hazards to aircraft crews, passengers, and equipment. Abstract: Both observational and theoretical research in the area of atmospheric high-energy physics since about 1980 has revealed that thunderstorms produce X-rays and gamma-rays into the MeV region by a number of mechanisms. While the nature of these mechanisms is still an area of active research, enough observational and theoretical data exists to permit an evaluation of hazards presented by ionizing radiation from thunderstorms to aircraft crew, passengers, and equipment. In this paper, we use data from existing studies to evaluate these hazards in a quantitative way. Citation: Stephan, K.D.; Shmatov, We find that hazards to humans are generally low, although with the possibility of an isolated rare M.L. -
Hazard Mitigation 6
State of New Hampshire, Natural Hazards Mitigation Plan, Executive Summary: October 2000 Edition State of New Hampshire Natural Hazards Mitigation Plan October 2000 Edition Ice Storm – January 1998, FEMA DR-1199-NH Rt. 175A Holderness – Plymouth October 1995 Prepared by the New Hampshire Office of Emergency Management 107 Pleasant Street Concord, New Hampshire 03301 (603) 271-2231 1 State of New Hampshire, Natural Hazards Mitigation Plan, Executive Summary: October 2000 Edition Table of Contents Table of Tables 4 Table of Maps 4 Table of Graphs 4 Table of Figures 4 Introduction 5 Authority 6 Definition of Hazard Mitigation 6 Purpose 6 Scope of the Plan 6 Overall Goals and Objectives of the State of New Hampshire 7 Disaster Declarations: An Overview 8 Presidential Disaster Declarations January 1, 1965 to December 31, 1998 9 State of N.H. Major Disasters and Emergency Declarations 1/1/82 to 10/21/98 10 Plan Sections: (Including Hazard Definitions and Vulnerability Assessments) I. Flood, Drought, Extreme Heat and Wildfire A. Flooding 12 1. Riverine Flooding: Heavy Rains and/or; 13 a. Debris Impacted Infrastructure 12 b. Rapid Snowpack Melt 15 c. River Ice 16 d. Dam Failure 17 NH Dam Safety Strategic Hazard Mitigation Overview 19 2. Coastal a. Excessive Stormwater Runoff 20 b. Storm Surge 20 c. Tsunami 22 3. New Hampshire Flood History 23 4. New Hampshire Strategic Flood Hazard Mitigation Plan Overview 29 B. Drought 30 New Hampshire Strategic Drought Mitigation Plan Overview 31 C. Extreme Heat 32 New Hampshire Strategic Extreme Heat Hazard Mitigation Plan Overview D. Wildfire 34 NH DRED Strategic Wildfire Hazard Mitigation Initiatives 34 Phragmites Australis 35 NH Strategic Phragmites Australis Wildfire Hazard Mitigation Plan Overview 36 2 State of New Hampshire, Natural Hazards Mitigation Plan, Executive Summary: October 2000 Edition II. -
Radar Imaging of Solar System Ices
RADAR IMAGING OF SOLAR SYSTEM ICES A DISSERTATION SUBMITTED TO THE DEPARTMENT OF ELECTRICAL ENGINEERING AND THE COMMITTEE ON GRADUATE STUDIES OF STANFORD UNIVERSITY IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF DOCTOR OF PHILOSOPHY Leif J. Harcke May 2005 © Copyright by Leif J. Harcke 2005 All Rights Reserved ii iv Abstract We map the planet Mercury and Jupiter’s moons Ganymede and Callisto using Earth-based radar telescopes and find that all bodies have regions exhibiting high, depolarized radar backscatter and polarization inversion (µc > 1). Both characteristics suggest volume scat- tering from water ice or similar cold-trapped volatiles. Synthetic aperture radar mapping of Mercury’s north and south polar regions at fine (6 km) resolution at 3.5 cm wavelength corroborates the results of previous 13 cm investigations of enhanced backscatter and po- larization inversion (0:9 µc 1:3) from areas on the floors of craters at high latitudes, ≤ ≤ where Mercury’s near-zero obliquity results in permanent Sun shadows. Co-registration with Mariner 10 optical images demonstrates that this enhanced scattering cannot be caused by simple double-bounce geometries, since the bright, reflective regions do not appear on the radar-facing wall but, instead, in shadowed regions not directly aligned with the radar look direction. A simple scattering model accounts for exponential, wavelength-dependent attenuation through a protective regolith layer. Thermal models require the existence of this layer to protect ice deposits in craters at other than high polar latitudes. The additional attenuation (factor 1:64 15%) of the 3.5 cm wavelength data from these experiments over previous 13 cm radar observations supports multiple interpretations of layer thickness, ranging from 0 11 to 35 15 cm, depending on the assumed scattering law exponent n.