Laser Technology in Photonic Applications for Space
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Planetary Science Division Status Report
Planetary Science Division Status Report Jim Green NASA, Planetary Science Division January 26, 2017 Astronomy and Astrophysics Advisory CommiBee Outline • Planetary Science ObjecFves • Missions and Events Overview • Flight Programs: – Discovery – New FronFers – Mars Programs – Outer Planets • Planetary Defense AcFviFes • R&A Overview • Educaon and Outreach AcFviFes • PSD Budget Overview New Horizons exploresPlanetary Science Pluto and the Kuiper Belt Ascertain the content, origin, and evoluFon of the Solar System and the potenFal for life elsewhere! 01/08/2016 As the highest resolution images continue to beam back from New Horizons, the mission is onto exploring Kuiper Belt Objects with the Long Range Reconnaissance Imager (LORRI) camera from unique viewing angles not visible from Earth. New Horizons is also beginning maneuvers to be able to swing close by a Kuiper Belt Object in the next year. Giant IcebergsObjecve 1.5.1 (water blocks) floatingObjecve 1.5.2 in glaciers of Objecve 1.5.3 Objecve 1.5.4 Objecve 1.5.5 hydrogen, mDemonstrate ethane, and other frozenDemonstrate progress gasses on the Demonstrate Sublimation pitsDemonstrate from the surface ofDemonstrate progress Pluto, potentially surface of Pluto.progress in in exploring and progress in showing a geologicallyprogress in improving active surface.in idenFfying and advancing the observing the objects exploring and understanding of the characterizing objects The Newunderstanding of Horizons missionin the Solar System to and the finding locaons origin and evoluFon in the Solar System explorationhow the chemical of Pluto wereunderstand how they voted the where life could of life on Earth to that pose threats to and physical formed and evolve have existed or guide the search for Earth or offer People’sprocesses in the Choice for Breakthrough of thecould exist today life elsewhere resources for human Year forSolar System 2015 by Science Magazine as exploraon operate, interact well as theand evolve top story of 2015 by Discover Magazine. -
Concept for Cryogenic Kj-Class Yb:YAG Amplifier K
OSA / ASSP/LACSEA/LS&C 2010 AWB20.pdf a288_1.pdf Concept for Cryogenic kJ-Class Yb:YAG Amplifier K. Ertel, C. Hernandez-Gomez, P. D. Mason, I. O. Musgrave, I. N. Ross, J. L. Collier STFC Rutherford Appleton Laboratory, Central Laser Facility, Chilton, Didcot, OX11 0QX, United Kingdom [email protected] Abstract: More and more projects and applications require the development of ns, kJ-class DPSSL systems with multi-Hz repetition rate. We present an amplifier concept based on cryogenically cooled Yb:YAG, promising high optical-to-optical efficiency and high gain. ©2010 Optical Society of America OCIS codes: (140.3280) Laser amplifiers; (140.3480) Lasers, diode-pumped, (140.3615) Lasers, ytterbium, (140.5560) Pumping 1. Introduction Currently, most lasers for producing multi-J to multi-kJ ns pulses are based on flashlamp pumped Nd:glass technology. These lasers show very poor electrical-to-optical (e-o) efficiency and can only be operated at very low repetition rates (few shots per minute to few shots per day, depending on size). A new approach is required to overcome these limitations in order to advance fundamental laser-plasma research and to enable envisioned real world applications such as laser driven particle accelerators and inertial fusion energy (IFE) production. Two multi-national laser research projects have been started in Europe. The first is ELI [1], focussed on ultra- short pulse laser research and applications, and the second is HiPER [2], focussed on IFE research. Both projects require the development of kJ-class ns-lasers operating at high e-o efficiency and at repetition rates around 10 Hz. -
Astronomy News KW RASC FRIDAY JANUARY 8 2021
Astronomy News KW RASC FRIDAY JANUARY 8 2021 JIM FAIRLES What to expect for spaceflight and astronomy in 2021 https://astronomy.com/news/2021/01/what-to-expect-for- spaceflight-and-astronomy-in-2021 By Corey S. Powell | Published: Monday, January 4, 2021 Whatever craziness may be happening on Earth, the coming year promises to be a spectacular one across the solar system. 2020 - It was the worst of times, it was the best of times. First landing on the lunar farside, two impressive successes in gathering samples from asteroids, the first new pieces of the Moon brought home in 44 years, close-up explorations of the Sun, and major advances in low-cost reusable rockets. First Visit to Jupiter's Trojan Asteroids First Visit to Jupiter's Trojan Asteroids In October, NASA is set to launch the Lucy spacecraft. Over its 12-year primary mission, Lucy will visit eight different asteroids. One target lies in the asteroid belt. The other seven are so-called Trojan asteroids that share an orbit with Jupiter, trapped in points of stability 60 degrees ahead of or behind the planet as it goes around the sun. These objects have been trapped in their locations for billions of years, probably since the time of the formation of the solar system. They contain preserved samples of water-rich and carbon-rich material in the outer solar system; some of that material formed Jupiter, while other bits moved inward to contribute to Earth's life-sustaining composition. As a whimsical aside: When meteorites strike carbon-rich asteroids, they create tiny carbon crystals. -
EDL – Lessons Learned and Recommendations
."#!(*"# 0 1(%"##" !)"#!(*"#* 0 1"!#"("#"#(-$" ."!##("""*#!#$*#( "" !#!#0 1%"#"! /!##"*!###"#" #"#!$#!##!("""-"!"##&!%%!%&# $!!# %"##"*!%#'##(#!"##"#!$$# /25-!&""$!)# %"##!""*&""#!$#$! !$# $##"##%#(# ! "#"-! *#"!,021 ""# !"$!+031 !" )!%+041 #!( !"!# #$!"+051 # #$! !%#-" $##"!#""#$#$! %"##"#!#(- IPPW Enabled International Collaborations in EDL – Lessons Learned and Recommendations: Ethiraj Venkatapathy1, Chief Technologist, Entry Systems and Technology Division, NASA ARC, 2 Ali Gülhan , Department Head, Supersonic and Hypersonic Technologies Department, DLR, Cologne, and Michelle Munk3, Principal Technologist, EDL, Space Technology Mission Directorate, NASA. 1 NASA Ames Research Center, Moffett Field, CA [email protected]. 2 Deutsches Zentrum für Luft- und Raumfahrt e.V. (DLR), German Aerospace Center, [email protected] 3 NASA Langley Research Center, Hampron, VA. [email protected] Abstract of the Proposed Talk: One of the goals of IPPW has been to bring about international collaboration. Establishing collaboration, especially in the area of EDL, can present numerous frustrating challenges. IPPW presents opportunities to present advances in various technology areas. It allows for opportunity for general discussion. Evaluating collaboration potential requires open dialogue as to the needs of the parties and what critical capabilities each party possesses. Understanding opportunities for collaboration as well as the rules and regulations that govern collaboration are essential. The authors of this proposed talk have explored and established collaboration in multiple areas of interest to IPPW community. The authors will present examples that illustrate the motivations for the partnership, our common goals, and the unique capabilities of each party. The first example involves earth entry of a large asteroid and break-up. NASA Ames is leading an effort for the agency to assess and estimate the threat posed by large asteroids under the Asteroid Threat Assessment Project (ATAP). -
Vulnerable Web Application Framework
University of Rhode Island DigitalCommons@URI Open Access Master's Theses 2015 Vulnerable Web Application Framework Nicholas J. Giannini University of Rhode Island, [email protected] Follow this and additional works at: https://digitalcommons.uri.edu/theses Recommended Citation Giannini, Nicholas J., "Vulnerable Web Application Framework" (2015). Open Access Master's Theses. Paper 629. https://digitalcommons.uri.edu/theses/629 This Thesis is brought to you for free and open access by DigitalCommons@URI. It has been accepted for inclusion in Open Access Master's Theses by an authorized administrator of DigitalCommons@URI. For more information, please contact [email protected]. VULNERABLE WEB APPLICATION FRAMEWORK BY NICHOLAS J. GIANNINI A THESIS SUBMITTED IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF MASTER OF SCIENCE IN COMPUTER SCIENCE AND STATISTICS UNIVERSITY OF RHODE ISLAND 2015 MASTER OF SCIENCE THESIS OF NICHOLAS GIANNINI APPROVED: Thesis Committee: Major Professor Victor Fay-Wolfe Lisa DiPippo Haibo He Nasser H. Zawia DEAN OF THE GRADUATE SCHOOL UNIVERSITY OF RHODE ISLAND 2015 ABSTRACT Utilizing intentionally vulnerable web applications to teach and practice cyber security principles and techniques provides a unique hands-on experience that is otherwise unobtainable without working in the real world. Creating such applications that emulate those of actual businesses and organizations without exposing actual businesses to inadvertent security risks can be a daunting task. To address these issues, this project has created Porous, an open source framework specifically for creating intentionally vulnerable web applications. The implementation of Porous offers a simplified approach to building realistic vulnerable web applications that may be tailored to the needs of specific cyber challenges or classroom exercises. -
1 Cross-Calibration of Laser-Induced Breakdown Spectroscopy (LIBS)
ISSI/ISSI-BJ Joint Call for Proposals 2018 International Teams in Space and Earth Sciences Cross-calibration of Laser-Induced Breakdown Spectroscopy (LIBS) instruments for planetary exploration. 1 Summary of the project : A revolutionary technique for planetary science: Laser-induced Breakdown Spectroscopy (LIBS) is an active analytical technique that makes use of a pulsed laser to ablate material of interest at a distance. The atoms in the high temperature plasma emit at specific wavelengths from the UV to near- IR and the light can be analyzed by spectrometry to determine the composition of the target [1]. Since 2012, LIBS has been successfully used under low atmospheric pressure for exploring the geology of Mars at Gale Crater with the Mars Science Laboratory rover’s ChemCam instrument [2-4]. LIBS can be used to analyze single regolith mineral particles and larger rocks, giving major and minor elements compositions. Moreover, LIBS is sensitive to volatile elements (H, Na, etc.) that are of intrinsic interest to understand key planetary processes. The generated shock wave can also ablate dust covering rocks to allow further analysis by other instruments on the mission platform (rover, lander). In order to quantify the elemental composition of various targets, large laboratory samples analyses are required for calibration, with ChemCam’s calibration database containing more than 400 standards [5-6]. LIBS is becoming international: Due to its ease of deployment and rapidity of analysis, LIBS has shown a great potential as a chemistry survey instrument for the next generation of in situ space missions to planets, satellites and small bodies. In the next couple of years, three more LIBS space instruments will be sent for planetary exploration by teams representing several different nationalities In 2018, the Indian space mission to the Moon Chandrayaan 2 will comprise a rover equipped with a small portable LIBS instrument for regolith reconnaissance around the landing site [7]. -
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7'tie;T;e ~;&H ~ t,#t1tMftllSieotOg, UCLA VOLUME 3 1986 EDITORIAL BOARD Mark E. Forry Anne Rasmussen Daniel Atesh Sonneborn Jane Sugarman Elizabeth Tolbert The Pacific Review of Ethnomusicology is an annual publication of the UCLA Ethnomusicology Students Association and is funded in part by the UCLA Graduate Student Association. Single issues are available for $6.00 (individuals) or $8.00 (institutions). Please address correspondence to: Pacific Review of Ethnomusicology Department of Music Schoenberg Hall University of California Los Angeles, CA 90024 USA Standing orders and agencies receive a 20% discount. Subscribers residing outside the U.S.A., Canada, and Mexico, please add $2.00 per order. Orders are payable in US dollars. Copyright © 1986 by the Regents of the University of California VOLUME 3 1986 CONTENTS Articles Ethnomusicologists Vis-a-Vis the Fallacies of Contemporary Musical Life ........................................ Stephen Blum 1 Responses to Blum................. ....................................... 20 The Construction, Technique, and Image of the Central Javanese Rebab in Relation to its Role in the Gamelan ... ................... Colin Quigley 42 Research Models in Ethnomusicology Applied to the RadifPhenomenon in Iranian Classical Music........................ Hafez Modir 63 New Theory for Traditional Music in Banyumas, West Central Java ......... R. Anderson Sutton 79 An Ethnomusicological Index to The New Grove Dictionary of Music and Musicians, Part Two ............ Kenneth Culley 102 Review Irene V. Jackson. More Than Drumming: Essays on African and Afro-Latin American Music and Musicians ....................... Norman Weinstein 126 Briefly Noted Echology ..................................................................... 129 Contributors to this Issue From the Editors The third issue of the Pacific Review of Ethnomusicology continues the tradition of representing the diversity inherent in our field. -
The Pancam Instrument for the Exomars Rover
ASTROBIOLOGY ExoMars Rover Mission Volume 17, Numbers 6 and 7, 2017 Mary Ann Liebert, Inc. DOI: 10.1089/ast.2016.1548 The PanCam Instrument for the ExoMars Rover A.J. Coates,1,2 R. Jaumann,3 A.D. Griffiths,1,2 C.E. Leff,1,2 N. Schmitz,3 J.-L. Josset,4 G. Paar,5 M. Gunn,6 E. Hauber,3 C.R. Cousins,7 R.E. Cross,6 P. Grindrod,2,8 J.C. Bridges,9 M. Balme,10 S. Gupta,11 I.A. Crawford,2,8 P. Irwin,12 R. Stabbins,1,2 D. Tirsch,3 J.L. Vago,13 T. Theodorou,1,2 M. Caballo-Perucha,5 G.R. Osinski,14 and the PanCam Team Abstract The scientific objectives of the ExoMars rover are designed to answer several key questions in the search for life on Mars. In particular, the unique subsurface drill will address some of these, such as the possible existence and stability of subsurface organics. PanCam will establish the surface geological and morphological context for the mission, working in collaboration with other context instruments. Here, we describe the PanCam scientific objectives in geology, atmospheric science, and 3-D vision. We discuss the design of PanCam, which includes a stereo pair of Wide Angle Cameras (WACs), each of which has an 11-position filter wheel and a High Resolution Camera (HRC) for high-resolution investigations of rock texture at a distance. The cameras and electronics are housed in an optical bench that provides the mechanical interface to the rover mast and a planetary protection barrier. -
Volume 16 –Number 3 National Park Service • U.S
PARKARK P CIENCECIENCE SS Integrating Research and Resource Management Volume 16 –Number 3 National Park Service • U.S. Department of the Interior Summer 1996 THE NATURAL RESOURCE TRAINEE PROGRAM: PROFESSIONALIZATION TRIUMPH OF THE 1980S AND EARLY 1990S Who are they and where are they now? See the key on page 17 to identify these participants of the first Natural Resource Trainee Program and learn what they are up to now. BY THE EDITOR imparting the skills. Regional office funding allowed parks to HE NEED TO ESTABLISH AND PROFES- send staff to the training and backfill behind them to take care sionalize science and resource management func- of unfinished park work. Other superintendents soon heard tions and apply them in the management of na- about the training opportunity and wanted to be a part of it. tional parks was recognized as early as the 1930s. Wauer then prioritized individual park needs, opting for placing Then, biologist George Wright published several resource management trainees at parks that formerly didn’t have Tpapers on wildlife management and made the clear connection any resource management expertise. between science and informed park resource management ac- The program went national in the early 1980s following pub- tivities. Yet, for the next 5 decades, resource management work lication of two different conservation organization reports on continued to be done mostly by park rangers who were trained threats to national parks and a response by the National Park primarily in law enforcement and other operational areas, not Service in the form of a state-of-the-parks report. -
18Th EANA Conference European Astrobiology Network Association
18th EANA Conference European Astrobiology Network Association Abstract book 24-28 September 2018 Freie Universität Berlin, Germany Sponsors: Detectability of biosignatures in martian sedimentary systems A. H. Stevens1, A. McDonald2, and C. S. Cockell1 (1) UK Centre for Astrobiology, University of Edinburgh, UK ([email protected]) (2) Bioimaging Facility, School of Engineering, University of Edinburgh, UK Presentation: Tuesday 12:45-13:00 Session: Traces of life, biosignatures, life detection Abstract: Some of the most promising potential sampling sites for astrobiology are the numerous sedimentary areas on Mars such as those explored by MSL. As sedimentary systems have a high relative likelihood to have been habitable in the past and are known on Earth to preserve biosignatures well, the remains of martian sedimentary systems are an attractive target for exploration, for example by sample return caching rovers [1]. To learn how best to look for evidence of life in these environments, we must carefully understand their context. While recent measurements have raised the upper limit for organic carbon measured in martian sediments [2], our exploration to date shows no evidence for a terrestrial-like biosphere on Mars. We used an analogue of a martian mudstone (Y-Mars[3]) to investigate how best to look for biosignatures in martian sedimentary environments. The mudstone was inoculated with a relevant microbial community and cultured over several months under martian conditions to select for the most Mars-relevant microbes. We sequenced the microbial community over a number of transfers to try and understand what types microbes might be expected to exist in these environments and assess whether they might leave behind any specific biosignatures. -
NANOSAT 1B COMUNICACIONES Orbita NANOSAT 1B
COMMUNICATIONS NANOSAT 1B COMUNICACIONES Orbita NANOSAT 1B Tipo: Polar heliosíncrona Keflavik Altura: 660 km. ANTARCTICA Inclinación: 98º INTA Madrid El Arenosillo ANTARTIDA Izaña Pune NANOSAT 1B NANOTECNOLOGIA Buenos Aires NANOTECHNOLOGY Usuhaia Marambio Belgrano una nueva filosofía de diseño Estaciones INTA INTA stations Estación Antártica Belgrano Belgrano Antarctic Station para sistemas espaciales Comunicaciones con la Antártida Communications with Antarctica Gracias a su órbita polar el NANOSAT 1B viene a sustituir a su ante- Thanks to his polar orbit, the NANOSAT 1B will replace his predecessor, cesor, el NANOSAT 01, para enlazar el INTA en Madrid con estaciones the NANOSAT 01, in order to link INTA-Madrid with scientific stations in científicas en lugares remotos como las situadas en la Antártida. remote places as the ones in the Antarctica. Los satélites geoestacionarios de comunicaciones no cubren esas (The geostationary communications satellites do not cover extreme latitudes extremas. latitudes.) A new philosophy for space systems design www.inta.es www.inta.es COMMUNICATIONS Carga útil de NANOSAT 1B NANOSAT 1B Payload NANOSAT 1B es un nanosatélite, pesa menos de 20 kg y mide COMUNICACIONES menos de medio metro de lado. Tiene forma hexagonal y va cu- LDT, Las Dos Torres bierto de paneles solares igual que su antecesor el NANOSAT Desarrollado totalmente por el INTA, es un detector de proto- 01 al que toma el relevo al acabar su vida útil. nes de alta energía que servirá para caracterizar el ambiente ANTARCTICA espacial en este rango de radiación. ANTARTIDA Incorpora como novedad en su carga útil: NANOSAT 1B it is a nanosatellite that weights about 20 kg and LDT, The Two Towers Totally developed by INTA, is a high energy protons detector which will measures less than half a meter side. -
Implementación De Framework De Desarrollo Web Durante Un Proyecto”
UNIVERSIDAD POLITÉCNICA DE SINALOA PROGRAMA ACADÉMICO DE INGENIERÍA EN INFORMÁTICA Tesina “Implementación de Framework de desarrollo web durante un proyecto” Para obtener la acreditación de las estadías profesionales y contar con los créditos para el grado de Ingeniero en Informática. Autor: Bernal Corral Daniel Asesor: M. C. Alejandro Pérez Pasten Borja Asesor OR: Ing. Omar Vidaña Peraza Mazatlán, Sinaloa 13 de Diciembre del 2019 Agradecimientos Agradezco a mis padres por brindarme todo su apoyo durante mis estudios, por darme las clases más importantes, por haber hecho posible que llegara a este momento, por enseñarme que no siempre todo sale perfecto y que debo esforzarme para obtener lo que quiero, por darme ánimos para seguir, por preocuparse por mí y esforzarse para que mi vida fuera mejor. A mi asesor por aconsejarme y corregir los errores que cometí durante el desarrollo de la tesina, por tomarse el tiempo para ver cada detalle y hacer recomendaciones, sugerir opciones, etc. A mi hermano por ayudarme a no rendirme, por asumir su rol de hermano mayor y tratar de guiar, por preocuparse por mí y ayudarme siempre que lo he necesitado. A los profesores que he tenido a lo largo de mis estudios y que me aportaron un poco de su conocimiento para enriquecer el mío. A todos mis compañeros que me ayudaron a hacer más amenas las clases. 6 ÍNDICE TEMÁTICO Índice de imágenes. 9 Resumen. ….. .11 Abstract. …. .11 Introducción. 11 Capítulo I. .. ... …12 1. Antecedentes. .. 13 1.1. Localización. .. ….. 13 1.2. Objetivos de la institución. …………….. 13 1.3. Visión. .14 1.4.