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Sintering of Niobium Containing AISI M2 High Speed Steel
Sintering of AISI M2 high speed steel with the addition of NbC Alexandre Wentzcovitch1, Francisco Ambrozio Filho1, Luis Carlos Elias da Silva2, Maurício David Martins das Neves2 1Centro Universitário da FEI 2Instituto de Pesquisas Energéticas e Nucleares – IPEN-CNEN/SP [email protected]; [email protected]; [email protected]; [email protected] Keywords: powder metallurgy, high speed steel, NbC, sintering and microstructure. Abstract. The influence of adding 6 wt% (NbC) niobium carbide on the sintering temperature and microstructure of high speed steel - AISI M2 (0.87% C, 5.00% Mo, 6.00% W, 4,00% Cr, 2.00% V and Fe bal.) powder was studied. The starting material was obtained by vacuum melting followed by atomization in water. The samples were axially cold compacted in a cylindrical matrix and then vacuum sintered at 1250 and 1350 °C. Dilatometry and differential scanning calorimetry measurements indicated an increase in sintering temperature with addition of niobium to the AISI M2 steel. Optical and scanning electron microscope observations revealed a microstructure with uniformly distributed niobium carbides. Introduction High-speed steels have been widely used in the manufacture of cutting tools and wear-resistant materials [1]. Several techniques have been used to improve the properties of sintered high speed steels and these include: addition of alloying elements to increase carbide formation [2, 3], addition of ceramic reinforcements and use of high- energy milling [4]. Niobium is an alloying element that can be added to high speed steels to form stable carbides and provide reinforcement to the matrix. The niobium added to the steel combines with carbon to form a MC-type carbide, which can increase the hardness and wear resistance of the high speed steel and prevent austenite grain growth during sintering and heat treatment. -
Institute for Clinical and Economic Review
INSTITUTE FOR CLINICAL AND ECONOMIC REVIEW FINAL APPRAISAL DOCUMENT BRACHYTHERAPY & PROTON BEAM THERAPY FOR TREATMENT OF CLINICALLY-LOCALIZED, LOW-RISK PROSTATE CANCER December 22, 2008 Senior Staff Daniel A. Ollendorf, MPH, ARM Chief Review Officer Julia Hayes, MD Lead Decision Scientist Pamela McMahon, PhD Sr. Decision Scientist Steven D. Pearson, MD, MSc President, ICER Associate Staff Michelle Kuba, MPH Sr. Technology Analyst Angela Tramontano, MPH Research Assistant © ICER, 2008 1 CONTENTS About ICER .................................................................................................................................. 3 Acknowledgments ...................................................................................................................... 4 Executive Summary .................................................................................................................... 5 Evidence Review Group Deliberation.................................................................................. 15 ICER Integrated Evidence Rating.......................................................................................... 21 Evidence Review Group Members........................................................................................ 24 Appraisal Overview.................................................................................................................. 28 Background ............................................................................................................................... -
小型飛翔体/海外 [Format 2] Technical Catalog Category
小型飛翔体/海外 [Format 2] Technical Catalog Category Airborne contamination sensor Title Depth Evaluation of Entrained Products (DEEP) Proposed by Create Technologies Ltd & Costain Group PLC 1.DEEP is a sensor analysis software for analysing contamination. DEEP can distinguish between surface contamination and internal / absorbed contamination. The software measures contamination depth by analysing distortions in the gamma spectrum. The method can be applied to data gathered using any spectrometer. Because DEEP provides a means of discriminating surface contamination from other radiation sources, DEEP can be used to provide an estimate of surface contamination without physical sampling. DEEP is a real-time method which enables the user to generate a large number of rapid contamination assessments- this data is complementary to physical samples, providing a sound basis for extrapolation from point samples. It also helps identify anomalies enabling targeted sampling startegies. DEEP is compatible with small airborne spectrometer/ processor combinations, such as that proposed by the ARM-U project – please refer to the ARM-U proposal for more details of the air vehicle. Figure 1: DEEP system core components are small, light, low power and can be integrated via USB, serial or Ethernet interfaces. 小型飛翔体/海外 Figure 2: DEEP prototype software 2.Past experience (plants in Japan, overseas plant, applications in other industries, etc) Create technologies is a specialist R&D firm with a focus on imaging and sensing in the nuclear industry. Createc has developed and delivered several novel nuclear technologies, including the N-Visage gamma camera system. Costainis a leading UK construction and civil engineering firm with almost 150 years of history. -
Naming the Extrasolar Planets
Naming the extrasolar planets W. Lyra Max Planck Institute for Astronomy, K¨onigstuhl 17, 69177, Heidelberg, Germany [email protected] Abstract and OGLE-TR-182 b, which does not help educators convey the message that these planets are quite similar to Jupiter. Extrasolar planets are not named and are referred to only In stark contrast, the sentence“planet Apollo is a gas giant by their assigned scientific designation. The reason given like Jupiter” is heavily - yet invisibly - coated with Coper- by the IAU to not name the planets is that it is consid- nicanism. ered impractical as planets are expected to be common. I One reason given by the IAU for not considering naming advance some reasons as to why this logic is flawed, and sug- the extrasolar planets is that it is a task deemed impractical. gest names for the 403 extrasolar planet candidates known One source is quoted as having said “if planets are found to as of Oct 2009. The names follow a scheme of association occur very frequently in the Universe, a system of individual with the constellation that the host star pertains to, and names for planets might well rapidly be found equally im- therefore are mostly drawn from Roman-Greek mythology. practicable as it is for stars, as planet discoveries progress.” Other mythologies may also be used given that a suitable 1. This leads to a second argument. It is indeed impractical association is established. to name all stars. But some stars are named nonetheless. In fact, all other classes of astronomical bodies are named. -
Space) Barriers for 50 Years: the Past, Present, and Future of the Dod Space Test Program
SSC17-X-02 Breaking (Space) Barriers for 50 Years: The Past, Present, and Future of the DoD Space Test Program Barbara Manganis Braun, Sam Myers Sims, James McLeroy The Aerospace Corporation 2155 Louisiana Blvd NE, Suite 5000, Albuquerque, NM 87110-5425; 505-846-8413 [email protected] Colonel Ben Brining USAF SMC/ADS 3548 Aberdeen Ave SE, Kirtland AFB NM 87117-5776; 505-846-8812 [email protected] ABSTRACT 2017 marks the 50th anniversary of the Department of Defense Space Test Program’s (STP) first launch. STP’s predecessor, the Space Experiments Support Program (SESP), launched its first mission in June of 1967; it used a Thor Burner II to launch an Army and a Navy satellite carrying geodesy and aurora experiments. The SESP was renamed to the Space Test Program in July 1971, and has flown over 568 experiments on over 251 missions to date. Today the STP is managed under the Air Force’s Space and Missile Systems Center (SMC) Advanced Systems and Development Directorate (SMC/AD), and continues to provide access to space for DoD-sponsored research and development missions. It relies heavily on small satellites, small launch vehicles, and innovative approaches to space access to perform its mission. INTRODUCTION Today STP continues to provide access to space for DoD-sponsored research and development missions, Since space first became a viable theater of operations relying heavily on small satellites, small launch for the Department of Defense (DoD), space technologies have developed at a rapid rate. Yet while vehicles, and innovative approaches to space access. -
Abstracts of Papers and Posters Presented at the 97Th Annual Meeting of the AAVSO, Held in Nantucket, Massachusetts, October 16–19, 2008
Abstracts, JAAVSO Volume 37, 2009 193 Abstracts of Papers and Posters Presented at the 97th Annual Meeting of the AAVSO, Held in Nantucket, Massachusetts, October 16–19, 2008 The International Year of Astronomy and Citizen Science Aaron Price AAVSO, 49 Bay State Road, Cambridge, MA 02138 Abstract 2009 has been endorsed as the International Year of Astronomy by both the United Nations and the United States Congress. This talk will briefly outline the IYA cornerstone projects and then will go into more detail regarding the AAVSO’s role as leading a citizen science project regarding the variable star epsilon Aurigae. Variable Star Astronomy Education Outreach Initiative Donna L. Young The Wright Center for Innovative Science, Tufts University, 4 Colby Street, Medford, MA 02155 Abstract The American Association of Variable Star Observers (AAVSO) published a comprehensive variable star curriculum, Hands-On Astrophysics, Variable Stars in Science, Math, and Computer Education in 1997. The curriculum, funded by the National Science Foundation, was developed for a comprehensive audience—amateur astronomers, classroom educators, science fair projects, astronomy clubs, family learning, and anyone interested in learning about variable stars. Some of the activities from the Hands-On Astrophysics curriculum have been incorporated into the educational materials for the Chandra X-Ray Observatory’s Educational and Public Outreach (EPO) Office. On two occasions, in 2000 and 2001, triggered by alerts from amateur astronomers, Chandra observed the outburst of the dwarf nova SS Cygni. The cooperation of amateur variable star astronomers and Chandra X-Ray scientists provided proof that the collaboration of amateur and professional astronomers is a powerful tool to study cosmic phenomena. -
Magnetic Field, Chemical Composition and Line Profile Variability of The
Mon. Not. R. Astron. Soc. 000, 1–11 (2010) Printed 20 November 2018 (MN LATEX style file v2.2) Magnetic field, chemical composition and line profile variability of the peculiar eclipsing binary star AR Aur⋆ C.P. Folsom1†, O. Kochukhov2, G.A. Wade3, J. Silvester3,4, S. Bagnulo1 1Armagh Observatory, College Hill, Armagh Northern Ireland BT61 9DG 2Department of Astronomy and Space Physics, Uppsala University, 751 20 Uppsala, Sweden 3Department of Physics, Royal Military College of Canada, P.O. Box 17000, Station ‘Forces’, Kingston, Ontario, Canada, K7K 7B4 4Department of Physics, Engineering Physics & Astronomy, Queen’s University, Kingston, Ontario, Canada, K7L 3N6 Received: 2010; Accepted: 2010 ABSTRACT AR Aur is the only eclipsing binary known to contain a HgMn star, making it an ideal case for a detailed study of the HgMn phenomenon. HgMn stars are a poorly understood class of chemically peculiar stars, which have traditionally been thought not to possess significant magnetic fields. However, the recent discovery of line profile variability in some HgMn stars, apparently attributable to surface abundance patches, has brought this belief into question. In this paper we investigate the chemical abun- dances, line profile variability, and magnetic field of the primary and secondary of the AR Aur system, using a series of high resolution spectropolarimetric observations. We find the primary is indeed a HgMn star, and present the most precise abundances yet determined for this star. We find the secondary is a weak Am star, and is possibly still on the pre-main sequence. Line profile variability was observed in a range of lines in the primary, and is attributed to inhomogeneous surface distributions of some el- ements. -
Magnetoshell Aerocapture: Advances Toward Concept Feasibility
Magnetoshell Aerocapture: Advances Toward Concept Feasibility Charles L. Kelly A thesis submitted in partial fulfillment of the requirements for the degree of Master of Science in Aeronautics & Astronautics University of Washington 2018 Committee: Uri Shumlak, Chair Justin Little Program Authorized to Offer Degree: Aeronautics & Astronautics c Copyright 2018 Charles L. Kelly University of Washington Abstract Magnetoshell Aerocapture: Advances Toward Concept Feasibility Charles L. Kelly Chair of the Supervisory Committee: Professor Uri Shumlak Aeronautics & Astronautics Magnetoshell Aerocapture (MAC) is a novel technology that proposes to use drag on a dipole plasma in planetary atmospheres as an orbit insertion technique. It aims to augment the benefits of traditional aerocapture by trapping particles over a much larger area than physical structures can reach. This enables aerocapture at higher altitudes, greatly reducing the heat load and dynamic pressure on spacecraft surfaces. The technology is in its early stages of development, and has yet to demonstrate feasibility in an orbit-representative envi- ronment. The lack of a proof-of-concept stems mainly from the unavailability of large-scale, high-velocity test facilities that can accurately simulate the aerocapture environment. In this thesis, several avenues are identified that can bring MAC closer to a successful demonstration of concept feasibility. A custom orbit code that dynamically couples magnetoshell physics with trajectory prop- agation is developed and benchmarked. The code is used to simulate MAC maneuvers for a 60 ton payload at Mars and a 1 ton payload at Neptune, both proposed NASA mis- sions that are not possible with modern flight-ready technology. In both simulations, MAC successfully completes the maneuver and is shown to produce low dynamic pressures and continuously-variable drag characteristics. -
The Strutjet Rocket Based Combined Cycle Engine A. Siebenhaar And
J The Strutjet Rocket Based Combined Cycle Engine A. Siebenhaar and M.J. Bulman GenCorp Aerojet Sacramento, CA And D.K. Bonnar Boeing Company Huntington Beach, Ca TABLE OF CONTENTS 1C) In_.roduc_o;', 2 0 Struuet t n_ine 2.1 FIo_ Path Description 2.2 Engine Architecture 2.2.1 FIo_path Elements 2.2.2 Turbo Machine D . Propellant Supply & Thermal Management 2.2.3 Engine C)cle 2.2.4 Structural Concept 2.3 Strutjet Operating Modes 2.3.1 Ducted Rocket Mode 2.3.2 Ramjet Mode 2.3.3 Scramjet Mode 2.3.4 Scram Rocket and Ascent Rocket Modes 2.4 Optimal Propulsion System Selection 2.4.1 Boost Mode Selection 2.4.2 Engine Design Point Selection 2.4.3 Ascent Rocket Transition Point Selection 3.0 Strutjet Vehicle Inte_ation 3.1 Strutjet Reference Mission 3.2 Engine-Vehicle Considerations 33 Vehicle Pitching Moment 3.4 Engine Performance 3.5 Reduced Operating Cost Through Robustness 3.6 Vehicle Comparisons 4.0 Available Hydrocarbon'and Hydrogen Test Data and plan_d Future Test Activities 4.1 Storable Hydrocarbon System Tests 4.2 CD'ogenic H.xdrogen System Tests 4.3 Planned Flight Tests 5.0 Maturit2. Of Required Su'utjet Technologies 6.0 Summar) and Conclusions 7.0 References J List of Tables 1. Comparison of Rocket and Strut.let Turbopumps 2. Sensitixitx to Engine Robustness 3. Vehicle Design Features and System Robustness 4. All-Rocket Vehicle Mass Breakdown 5. Strutjet Vehicle Mass Breakdown 6. Design Parameters for the All-Rocket and the RBCC-SSTO Vehicle 7. -
Výročná Správa Za Rok 2005
2005 3.1. Research output – publications 3. Monographs published in Slovakia 1. PITTICH, E.M. Astronomická ročenka 2006. Hurbanovo: Slovenská ústredná hvezdáreň, 2005. ISBN 80-85221-50-0. p. 1-272. (in Slovak) 7. Chapters in monographs published in Slovakia 2. HRIC, L. Premenné hviezdy. In PITTICH, E.M. Astronomická ročenka 2006. Hurbanovo: Slovenská ústredná hvezdáreň, 2005. ISBN 80-85221-50-0. p. 186-202. (in Slovak) 3. PITTICH, E. Čas, obloha od januára do decembra. In PITTICH, E.M. Astronomická ročenka 2006. Hurbanovo: Slovenská ústredná hvezdáreň, 2005. ISBN 80-85221-50-0. p. 3-89. (in Slovak) 4. PITTICH, E. Pohyb planét po oblohe, elongácie a jasnosti, Mesiac krátko po nove. In PITTICH, E.M. Astronomická ročenka 2006. Hurbanovo: Slovenská ústredná hvezdáreň, 2005. ISBN 80-85221-50-0. p. 90-103. (in Slovak) 5. PITTICH, E. Kométy. In PITTICH, E.M. Astronomická ročenka 2006. Hurbanovo: Slovenská ústredná hvezdáreň, 2005. ISBN 80-85221-50-0. p. 106-143. (in Slovak) 6. PITTICH, E. Galileiho mesiace. In PITTICH, E.M. Astronomická ročenka 2006. Hurbanovo: Slovenská ústredná hvezdáreň, 2005. ISBN 80-85221-50-0. p. 159-172. (in Slovak) 7. PITICHOVÁ, J. Kométy roka 2004. In PITTICH, E.M. Astronomická ročenka 2006. Hurbanovo: Slovenská ústredná hvezdáreň, 2005. ISBN 80-85221-50-0. p. 241-268. (in Slovak) 8. PORUBČAN, V. Meteorické roje. In PITTICH, E.M. Astronomická 2006. Hurbanovo: Slovenská ústredná hvezdáreň, 2005. ISBN 80-85221-50-0. p. 104-105. (in Slovak) 9. SVOREŇ, J. Teórie vzniku a vývoja asteroidov. In PITTICH, E.M. Astronomická ročenka 2006. Hurbanovo: Slovenská ústredná hvezdáreň, 2005. -
600 Technology (Applied Sciences)
600 600 Technology (Applied sciences) Class here inventions See also 303.48 for technology as a cause of cultural change; also 306.4 for sociology of technology; also 338.1–338.4 for economic aspects of industries based on specific technologies; also 338.9 for technology transfer, appropriate technology See Manual at 300 vs. 600; also at 363 vs. 302–307, 333.7, 570–590, 600; also at 363.1 vs. 600; also at 583–585 vs. 600 SUMMARY 601–609 Standard subdivisions and technical drawing, hazardous materials technology, patents 610 Medicine and health 620 Engineering and allied operations 630 Agriculture and related technologies 640 Home and family management 650 Management and auxiliary services 660 Chemical engineering and related technologies 670 Manufacturing 680 Manufacture of products for specific uses 690 Construction of buildings 601 Philosophy and theory 602 Miscellany Do not use for patents; class in 608 Class interdisciplinary works on trademarks and service marks in 929.9 Interdisciplinary collections of standards relocated to 389 .9 Commercial miscellany Class commercial miscellany of products and services used in individual and family living in 640.29; class commercial miscellany of manufactured products in 670.29; class interdisciplinary commercial miscellany in 381.029 603 Dictionaries, encyclopedias, concordances 604 Technical drawing, hazardous materials technology; groups of people 657 604 Dewey Decimal Classification 604 .2 Technical drawing Including arrangement and organization of drafting rooms, preservation and storage of drawings; specific drafting procedures and conventions (e.g., production illustration, dimensioning; lettering, titling; shades, shadows, projections); preparation and reading of copies Class here engineering graphics, mechanical drawing For architectural drawing, see 720.28. -
Evaluation of Anticorrosive Effect of Niobium Carbide Coating
1387 A publication of CHEMICAL ENGINEERING TRANSACTIONS VOL. 57, 2017 The Italian Association of Chemical Engineering Online at www.aidic.it/cet Guest Editors: Sauro Pierucci, Jiří Jaromír Klemeš, Laura Piazza, Serafim Bakalis Copyright © 2017, AIDIC Servizi S.r.l. DOI: 10.3303/CET1757232 ISBN 978-88-95608- 48-8; ISSN 2283-9216 Evaluation of Anticorrosive Effect of Niobium Carbide Coating Applied on Carbon Steel b a b a Luisa Novoa , Luis E. Cortes , Eliana Gonzalez , Arnaldo Jimenez , Luis G. a a a Cortes , Mario Ojeda , Aida L. Barbosa* a Laboratory of Research of Catalysis and New materials (LICATUC), Science Faculty, Chemistry Program, University of Cartagena, Campus of Zaragocilla, Kra 50 Nº 30-40, Cartagena, Colombia b Dept of Civil Engineering, Civil Enginering programm, University of Cartagena, Campus of Piedra de Bolivar, Av. El Consulado Calle 30. No. 48 - 152, Cartagena, Colombia [email protected] South America and particularly Colombia, has niobium and tantalum deposits, which can be used as a carbon steel protective agent. A preliminary step is the raw material characterization. Fresh and calcinated samples of niobium mineral in ores and sand were analyzed through optic microscopy, laser-Raman spectroscopy, DRX and textural aspects. The main components of the ore and alluvial sand were Ferrotapiolite and ferrocolumbite with chemical formula (Fe,Mn)•(Ta,Nb)2O6 and associated oxides like Fe2O3, SiO2. In the shape of Tectosilicates, Mn-Tantalite, Nb=O terminal and polyatomic octahedral structures of NbO6, highly distorted, susceptible to form carbides. Ferrocolumbite synthetic (FeNb50) was used as precursor of NbC coating for the surfaces protection of AISI 1020 steel samples having dimensions of 3/8 inch diameter and 1/2 inch length.