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Slide 1Jim Matthews Louisiana State University Results from the Pierre Auger Observatory ECRS, Moscow, 4 July 2012 1 Slide 2 ~ E -2.7 ~ E -3.1 Above 10 20 eV (50 Joules!):…
MRO of military helicopter engines Innovative solutions for a crit ical asset in mil i tary operations June 2015 By Etienne Daum and William Pauquet In collaboration…
FLASH-B FLuorescent Advanced Stratospheric Hygrometer (for balloon) Instrument design. Observations and comparison. Central Aerological Observatory Khaykin S., Yushkov V.,…
Slide 1 www.cogeneurope.eu Cogeneration Observatory and Dissemination Europe - CODE2 ROADMAP FOR COGENERATION OF HEAT & POWER FOR CYPRUS Costas G. Theofylaktos BoD of…
Convection Simulation of an A-star By Regner Trampedach Mt. Stromlo Observatory, Australian National University 8/19/04 Hydro-dynamics Solve Euler equations Conservation…
Radioastronomie à Nançay: physique solaire et héliosphérique Solar Radio Monitoring at Nançay Observatory - spectrography and imaging K.-L. Klein, A. Kerdraon, A. Lecacheux…
NATIONAL AND KAPODISTRIAN UNIVERSITY OF ATHENS SCHOOL OF SCIENCE DEPARTMENT OF INFORMATICS AND TELECOMMUNICATION GRADUATE PROGRAM COMPUTER NETWORKING MASTER THESIS A STORM…
Slide 1 Centimeter Receiver Design Considerations with a look to the future Steven White National Radio Astronomy Observatory Green Bank, WV Slide 2 Slide 3 Todd. Hunter,…
Cosmic-Ray Detection at the ARGO-YBJ observatory P. Camarri University of Roma “Tor Vergata” INFN Roma Tor Vergata P. Camarri - WAPP 2011 - Darjeeling, India - Dec 2011…
Gene Regulatory Network Identification Korkut Uygun and Yinlun Huang Department of Chemical Engineering and Materials Science Wayne State University AIChE Annual National…
University of Cyprus Department of Computer Science Παύλος Αντωνίου Γραφείο: B109 ΘΕΕ01 EPL660: Information Retrieval and Search Engines – Lab 11…
CC5212-1 PROCESAMIENTO MASIVO DE DATOS OTOÑO 2020 Lecture 5 Apache Spark Core Aidan Hogan aidhog@gmailcom Spark vs Hadoop What is the main weakness of Hadoop Let’s see…
Patrick Stuedi IBM Research Data Processing at the Speed of 100 Gbps using Apache Crail The CRAIL Project: Overview Crail Store Data Processing Framework eg Spark TensorFlow…
An Investigation of Matter Enhanced Neutrino Oscillation with the Sudbury Neutrino Observatory Miles Walter Eldon Smith A dissertation submitted in partial fulfillment of…
The Optical Counterpart of NGC6946 ULX-1 P. Abolmasov, S. Fabrika, O. Sholukhova, V. Afanasiev Special Astrophysical Observatory, Russia (a peculiar ULX nebula MF16) ULX…
(東京) Nobuyuki Sakai, National Astronomical Observatory of Japan October 9, 2014@EVN Symp. 2014 in Italy Direct Comparison between Astrometry Results and an Analytic Dynamics…
PowerPoint Presentation• Small size of the antenna (diameter of 3 – 5 meters) • Dual polarization • “Acceptable” G/T Gain of Reflector Antennas
FOREBYGGELSESPAKKE Fysisk Aktivitet FOREBYGGELSESPAKKE – FYSISK AKTIVITET 3 INDholDsfortegNelse fakta 4 FOREKOMST 5 TABTE LEVEÅR SOM FØLGE AF FYSISK InAKTIVITET 6 BRuG…
Patrick Stuedi IBM Research Data Processing at the Speed of 100 Gbps using Apache Crail The CRAIL Project: Overview Crail Store Data Processing Framework eg Spark TensorFlow…
An ultrahigh-speed digitizer for the Harvard College Observatory astronomical plates R.J. Simcoe ξ 1, J.E. Grindlay1, E.J. Los1, A.Doane1, S.G. Laycock1, D.J.Mink2, G. Champine1,…