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1 1. Seja o retificador mostrado abaixo, onde V1(ωt)=220sen(wt); R= 20Ω e L=100mH; f=50Hz. Calcular VLmed, ILmed.e o FP da estrutura. Solução: Cálculo do ângulo de…

Comments on OPERA OPERA is going on. We will have good Tau neutrino interactions within years, if νμ-ντ oscillation is the real solution. New Techniques developed in…

OPERA physics motivation - CNGS OPERA detector ντ appearance physics program 2006 Dortmund, April 2006 physics motivation provide an unambiguous evidence for νμ→ντ…

S I G LA C O D I C U M FAMILIA β Cod. Bodl. MS Ε. D. Clarke 39 aηηο 895 Cod. Veη. gr. Ι85 saec. XII Β D FAMILIA 11 τ Cod. Veη. app. cl. 4· 1 saec. Χ τ FAMI LIA…

S I G LA C O D I C U M FAMILIA β Cod. Bodl. MS Ε. D. Clarke 39 aηηο 895 Cod. Veη. gr. Ι85 saec. XII Β D FAMILIA 11 τ Cod. Veη. app. cl. 4· 1 saec. Χ τ FAMI LIA…

Antonio Scaturro παλαiός Opera Prima 2013 Autore Antonio Scaturro Titolo παλαiός Anno 2013 A cura di Poesia 2.0 Copertina adattamento di una scultura di Roberto…

Brick Finding Package – Status ReportA. A. ChukanovChukanov DubnaDubna, 25, 25thth January, 2007January, 2007 OutlineOutline OPERA:OPERA: OOscillation scillation PProjectroject

Slide 1 OPERA experiment T.Toshito (Nagoya univ. Japan) for the OPERA collaboration Apr.21 2002 APS2002@Albuquerque Slide 2 CNGS beam Due to CERN financial situation we have…

reconstructed vT candidate event Caren Hagner, Universität Hamburg DESY Seminar, 12.10.2010 VARIABLE Value kink (mrad) 41 ± 2 decay length (mm) 1335 ± 35 P (daughter)…

Soluções de exerćıcios seleccionados Caṕıtulo 1 1.9. Seja D um domı́nio de integridade. Mostre que: (a) Para cada d ∈ D − {0}, a aplicação φd : D →…

reconstructed vT candidate event Caren Hagner, Universität Hamburg DESY Seminar, 12.10.2010 VARIABLE Value kink (mrad) 41 ± 2 decay length (mm) 1335 ± 35 P (daughter)…

PowerPoint Presentation Updated results of the OPERA long baseline neutrino experiment On behalf of the OPERA Collaboration S.Dusini – INFN Padova EPS-HEP 2011 - Grenoble…

1 Björn Wonsak Recent results from the OPERA experiment University of Hamburg The Collaboration ~140 physicists, 28 institutions, 11 countries 3Björn WonsakMIAMI2013, 13.12.13…

LNGS August 21st CNGSOPERA starting OPERA collaboration 1 Starting OPERA data taking with the CNGS beam LNGS August 21st CNGSOPERA starting OPERA collaboration 2 Structure…

R ZimmermannR Zimmermann Dortmund April 2006Dortmund April 2006 11 OPERAOPERA •• physics motivation physics motivation -- CNGSCNGS •• OPERA detectorOPERA detector…

070212 1Paolo Walter Cattaneo ν superluminali : Situazione sperimentale e prospettive future Paolo W. Cattaneo INFN Pavia 070212 2Paolo Walter Cattaneo Definitions Direct…

νµ ντ Test results from a prototype RPC setup for the OPERA Target Tracker VI Workshop on RPC Coimbra 26-27 November 2001 Presented by: Dario Autiero CERNEP ντ ν 8…

Slide 1Observation of ν μ → ν τ oscillations in the CNGS beam with the OPERA experiment M. De Serio University of Bari & INFN Bari On behalf of the OPERA Collaboration…

TUGAS UNIT OPERASI DAN PROSES UNIT FILTRASI Disusun Oleh: Nama NPM Jurusan : Febry Dahyani : 0906636825 : Teknik Lingkungan For Problem 10.1 ; 10.3. ; and 10.4. A rapid sand…

Grammar Βοοκ for A’ Class wwwaglikapastrascom - Free EFL material -–Not for commercial use 1 CONTENTS Unit 1: Verb BE Unit 1: Personal pronouns Possessive adjectives…