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Snowmass 2021 Letter of Interest: Ultra-High-Energy Neutrinos
Snowmass 2021 Letter of Interest: Ultra-High-Energy Neutrinos Markus Ahlers,1 Jaime Alvarez-Mu~niz,´ 2 Rafael Alves Batista,3 Luis Anchordoqui,4 Carlos A. Arg¨uelles,5 Jos´e Bazo,6 James Beatty,7 Douglas R. Bergman,8 Dave Besson,9, 10 Stijn Buitink,11 Mauricio Bustamante,1, 12, ∗ Olga Botner,13 Anthony M. Brown,14 Washington Carvalho Jr.,15 Pisin Chen,16 Brian A. Clark,17 Amy Connolly,7 Linda Cremonesi,18 Cosmin Deaconu,19 Valentin Decoene,20 Paul de Jong,21, 22 Sijbrand de Jong,23, 22 Peter B. Denton,24, y Krijn De Vries,25 Michele Doro,26 Michael A. DuVernois,27 Ke Fang,28 Christian Glaser,13 Peter Gorham,29 Claire Gu´epin,30 Allan Hallgren,13 Jordan C. Hanson,31 Tim Huege,32, 11 Martin H. Israel,33 Albrecht Karle,27 Spencer R. Klein,34, 35 Kumiko Kotera,20 Ilya Kravchenko,36 John Krizmanic,30, 37 John G. Learned,29 Olivier Martineau-Huynh,38 Peter M´esz´aros,39 Thomas Meures,27 Miguel A. Mostaf´a,39, 40 Katharine Mulrey,11 Kohta Murase,39, 40, 41 Jiwoo Nam,16 Anna Nelles,42, 43 Eric Oberla,44 Foteini Oikonomou,45 Angela V. Olinto,44 Yasar Onel,46 A. Nepomuk Otte,47 Sergio Palomares-Ruiz,48 Alex Pizzuto,27 Steven Prohira,7 Brian Rauch,49 Mary Hall Reno,46 Juan Rojo,50, 51 Andr´esRomero-Wolf,52 Ibrahim Safa,5, 27 Olaf Scholten,53, 25 Frank G. Schr¨oder,54, 32 Wayne Springer,55 Irene Tamborra,1, 12 Charles Timmermans,51, 23 Diego F. Torres,56 Jo~aoR. -
Mediatek Linkit™ Development Platform for RTOS Get Started Guide
MediaTek LinkIt™ Development Platform for RTOS Get Started Guide Version: 3.0 Release date: 30 June 2016 © 2015 - 2016 MediaTek Inc. This document contains information that is proprietary to MediaTek Inc. (“MediaTek”) and/or its licensor(s). MediaTek cannot grant you permission for any material that is owned by third parties. You may only use or reproduce this document if you have agreed to and been bound by the applicable license agreement with MediaTek (“License Agreement”) and been granted explicit permission within the License Agreement (“Permitted User”). If you are not a Permitted User, please cease any access or use of this document immediately. Any unauthorized use, reproduction or disclosure of this document in whole or in part is strictly prohibited. THIS DOCUMENT IS PROVIDED ON AN “AS-IS” BASIS ONLY. MEDIATEK EXPRESSLY DISCLAIMS ANY AND ALL WARRANTIES OF ANY KIND AND SHALL IN NO EVENT BE LIABLE FOR ANY CLAIMS RELATING TO OR ARISING OUT OF THIS DOCUMENT OR ANY USE OR INABILITY TO USE THEREOF. Specifications contained herein are subject to change without notice. MediaTek LinkIt™ Development Platform for RTOS Get Started Guide Document Revision History Revision Date Description 1.0 24 March 2016 Initial version. 2.0 17 May 2016 Move the contents relative to flash, HDK, and build comments to corresponding documents. Add the support of Keil 3.0 30 June 2016 Add the support of IAR. Refine the architecture and provide more information on the SDK usage. © 2015 - 2016 MediaTek Inc. Page i of v This document contains information that is proprietary to MediaTek Inc. -
Hannes Tschofenig
Securing IoT applications with Mbed TLS Hannes Tschofenig Part#2: Public Key-based authentication March 2018 © 2018 Arm Limited Munich Agenda • For Part #2 of the webinar we are moving from Pre-Shared Secrets (PSKs) to certificated-based authentication. • TLS-PSK ciphersuites have • great performance, • low overhead, • small code size. • Drawback is the shared key concept. • Public key cryptography was invented to deal with this drawback (but itself has drawbacks). 2 © 2018 Arm Limited Public Key Infrastructure and certificate configuration © 2018 Arm Limited Public Key Infrastructure Various PKI deployments in existence Structure of our PKI The client has to store: self-signed • Client certificate plus corresponding private key. CA cert • CA certificate, which serves as the trust anchor. The server has to store: Signed by CA Signed by CA • Server certificate plus corresponding private key. Client cert Server cert (Some information for authenticating the client) 4 © 2018 Arm Limited Generating certificates (using OpenSSL tools) • When generating certificates you will be prompted to enter info. You are about to be asked to enter information that will be • The CA cert will end up in the trust incorporated into your certificate request. What you are about to enter is what is called a Distinguished anchor store of the client. Name or a DN. There are quite a few fields but you can leave some blank For some fields there will be a default value, • The Common Name used in the server If you enter '.', the field will be left blank. ----- cert needs to be resolvable via DNS Country Name (2 letter code) [AU]:. -
Arxiv:1906.07209V1 [Astro-Ph.HE] 17 Jun 2019 Hole-Black Hole and Neutron Star-Neutron Star Mergers)
POEMMA's target of opportunity sensitivity to cosmic neutrino transient sources Tonia M. Venters Astrophysics Science Division, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA Mary Hall Reno Department of Physics and Astronomy, University of Iowa, Iowa City, IA 52242, USA John F. Krizmanic CRESST/NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA University of Maryland, Baltimore County, Baltimore, MD 21250, USA Luis A. Anchordoqui Department of Physics, Graduate Center, City University of New York (CUNY), NY 10016, USA Department of Physics and Astronomy, Lehman College (CUNY), NY 10468, USA Department of Astrophysics, American Museum of Natural History, NY 10024, USA Claire Gu´epin Sorbonne Universit´e,CNRS, UMR 7095, Institut d'Astrophysique de Paris, 98 bis bd Arago, 75014 Paris, France Angela V. Olinto Department of Astronomy & Astrophysics, KICP, EFI, The University of Chicago, Chicago, IL 60637, USA (Dated: June 19, 2019) We calculate the sensitivity of space-based cosmic neutrino detection from transient sources in the context of the Probe Of Extreme Multi-Messenger Astrophysics (POEMMA) mission using Target- of-Opportunity (ToO) observations. POEMMA uses two spacecraft each with a large Schmidt telescope to simultaneously view the optical signals generated by extensive air showers (EASs). POEMMA is designed for both ultrahigh-energy cosmic ray and very-high-energy neutrino mea- surements. POEMMA has significant neutrino sensitivity starting in the 10 PeV decade via mea- surements of Cherenkov signals from upward-moving EASs initiated by tau neutrinos interacting in the Earth. For ToO observations, POEMMA uses the ability to quickly repoint (90◦ in 500 seconds) each of the two spacecraft to the direction of the transient source. -
Freescale Iot Solutions APF-SHB-T1454
Freescale IoT Solutions APF-SHB-T1454 James Huang | Asia MICRO Business Development M A Y . 2 0 1 5 TM External Use The Internet of Things is Driving Explosive Growth 50 In Connected Devices BILLION 25 BILLION 12.5 BILLION 7.6B 7.2B 6.8B 6.5B World 6.3B Population # Connected <1x 1x 2x 3.5x 6.5x Devices/Person 2003 2008 2010 2015 2020 TM External Use 1 * Sources: Ericsson, February 2011; Cisco Internet Business Solutions Group (IBSG), April 2011 IoT emerging as the next mega-trend Internet subscribers over time Source: Goldman Sachs Global Investment Research TM External Use 2 * Sources: Ericsson, February 2011; Cisco Internet Business Solutions Group (IBSG), April 2011 Our Products Power The Internet of Things Microcontrollers | Digital Networking | Auto MCU | Analog and Sensors | RF Traffic Monitoring Metro Cells Base Stations Small Cells Advanced Safety Security Networked Printers Infotainment Radar + Vision Enterprise Gateways, Cloud Data Switchers, Routers Computing Center Home Health Monitors + Fitness Energy Management, Wind + Solar Telehealth Industrial Smart Energy Connected Networking Connected Grid Farms Appliances Digital Power Conversion Energy Human – Machine Meters Interface Home Hubs Machine – Machine Security TM External Use 3 IoT Is More Than M2M The Internet of Things (IoT) is about Machine to Entity (M2E): • Machine to Machine: − Automatic diagnostics for cars: Automatic information collection from your car’s engine management system and sending real- time alerts to drivers or service centers Machine to • Machine to -
CR1000X Product Manual
Revision: 07/20/2021 Copyright © 2000 – 2021 Campbell Scientific, Inc. Table of Contents 1. Introduction 1 2. Precautions 2 3. Initial inspection 3 4. CR1000X data acquisition system components 4 4.1 The CR1000X Datalogger 5 4.1.1 Overview 5 4.1.2 Operations 6 4.1.3 Programs 6 4.2 Sensors 6 5. Wiring panel and terminal functions 8 5.1 Power input 11 5.1.1 Powering a data logger with a vehicle 12 5.1.2 Power LED indicator 12 5.2 Power output 12 5.3 Grounds 13 5.4 Communications ports 15 5.4.1 USB device port 15 5.4.2 Ethernet port 15 5.4.3 C terminals for communications 16 5.4.3.1 SDI-12 ports 16 5.4.3.2 RS-232, RS-422, RS-485, TTL, and LVTTL ports 16 5.4.3.3 SDM ports 16 5.4.4 CS I/O port 17 5.4.5 RS-232/CPI port 18 5.5 Programmable logic control 19 6. Setting up the CR1000X 21 6.1 Setting up communications with the data logger 21 6.1.1 USB or RS-232 communications 21 6.1.2 Virtual Ethernet over USB (RNDIS) 23 6.1.3 Ethernet communications option 24 Table of Contents - i 6.1.3.1 Configuring data logger Ethernet settings 25 6.1.3.2 Ethernet LEDs 26 6.1.3.3 Setting up Ethernet communications between the data logger and computer 26 6.2 Testing communications with EZSetup 27 6.3 Making the software connection 29 6.4 Creating a Short Cut data logger program 29 6.5 Sending a program to the data logger 32 7. -
IP Production IBC Preview Cloud Playout AMC/Sundance Q&A
IP production www.csimagazine.com IBC preview Cloud playout AMC/Sundance Q&A Welcome to High Dynamic Range television September 2015 cover.indd 1 19/08/2015 12:33:55 Expect More. AMOS Satellites. Meet us at More Coverage. More Throughput. More Services. IBC September 11-15, 2015 Across the Middle East, Europe, Africa and Asia. Amsterdam Hall 1, Booth C.65 Spacecom’s AMOS satellite constellation, consisting of AMOS-2 and AMOS-3 co-located at 4°W, AMOS-4 at 65°E and AMOS-5 at 17°E provides high-quality broadcast and communications services across Europe, Africa, Russia, Asia and the Middle East. With the upcoming launch of AMOS-6, Spacecom is expanding its coverage over Europe and Africa. The result: greater capacity, high-throughput Ka multibeam capabilities and affordable end-to-end satellite services. Spacecom. Expect More. EXPECT MORE www.amos-spacecom.com Untitled-2 1 10/08/2015 12:00:19 Contents IP production www.csimagazine.com IBC preview Cloud playout AMC/Sundance Q&A 30 Online piracy Editor Goran Nastic A new way of thinking about connected revenue security Commercial Welcome to High Dynamic Range television John Woods, Hammad Uddin September 2015 cover.indd 1 19/08/2015 12:33:55 36 Data corner A closer look at SVoD customers Design and production Matt Mills (Manager) 10 Analyst corner Jason Tucker With the first 4k channels launching in Europe, 40 IP production Matleena Lilja-Pelling an assessment of early services and the future It has its pros and cons, which broadcasters would do well to start preparing for Regular contributors 12 COVER STORY - HDR special Adrian Pennington, Philip Hunter, 44 Smart home David Adams, Stephen Cousins, High Dynamic Range really will take TV up a Anna Tobin level but it is not without challenges. -
Arxiv:1903.01609V2 [Astro-Ph.IM] 24 Jun 2019 the Origin of Ultra-High Energy Cosmic Rays (Uhecrs) Is One of the Biggest Mysteries in Astroparticle Physics
Targeting ultra-high energy neutrinos with the ARIANNA experiment A. Ankera, S. W. Barwicka, H. Bernhoffb, D. Z. Bessonc,d, Nils Bingeforse, G. Gaswinta, C. Glasera,∗, A. Hallgrene, J. C. Hansonf, R. Lahmanna,g, U. Latifc, J. Namh, A. Novikovc,d, S. R. Kleini, S. A. Kleinfelderj, A. Nellesk,l, M. P. Paula, C. Persichillia, S. R. Shivelya, J. Tatara,m, E. Ungere, S.-H. Wangh, G. Yodha aDepartment of Physics and Astronomy, University of California, Irvine, CA 92697, USA bUppsala University Department of Engineering Sciences, Division of Electricity, Uppsala, SE-752 37 Sweden cDepartment of Physics and Astronomy, University of Kansas, Lawrence, KS 66045, USA dNational Research Nuclear University MEPhI (Moscow Engineering Physics Institute), Moscow 115409, Russia eUppsala University Department of Physics and Astronomy, Uppsala, SE-752 37, Sweden fWhittier College Department of Physics, Whittier, CA 90602, USA gECAP, Friedrich-Alexander Universit¨atErlangen-N¨urnberg, 91058 Erlangen, Germany hDepartment of Physics and Leung Center for Cosmology and Particle Astrophysics, National Taiwan University, Taipei 10617, Taiwan iLawrence Berkeley National Laboratory, Berkeley, CA 94720, USA jDepartment of Electrical Engineering and Computer Science, University of California, Irvine, CA 92697, USA kDESY, 15738 Zeuthen, Germany lHumbolt-Universit¨atzu Berlin, Institut f¨urPhysik, 12489 Berlin, Germany mResearch Cyberinfrastructure Center, University of California, Irvine, CA 92697 USA Abstract The measurement of ultra-high energy (UHE) neutrinos (E > 1016 eV) opens a new field of astronomy with the potential to reveal the sources of ultra-high energy cosmic rays especially if combined with observations in the electromagnetic spectrum and gravitational waves. The ARIANNA pilot detector explores the detection of UHE neutrinos with a surface array of independent radio detector stations in Antarctica which allows for a cost-effective instrumentation of large volumes. -
Iot Development Platform
.org IoT Development Platform 1 Q&A . How many ARM cores shipped in 2012? 8,700,000,000 2020 . 2011 . Per Day: 23,835,616 . Per Hour: 993,151 150+ 25+ billion . Per Minute: 16,553 billion . Per Second: 276 2002 1+ billion 1998 2010 2020 2 ARM is a Semiconductor IP Company ARM’s Ecosystem Financial Tools/Technology IDM Foundry Fabless Semicon Co. Equipment Manufacturer ARM CPU GPU Software Platforms Networking Video RF Security DSP Other IP Carriers + Developers 3 ARM Cortex Advanced Processors Architectural innovation, compatibility across diverse application spectrum MP Cortex-A15 . ARM Cortex™-A family: ...2.5GHz . Applications processors for feature- Cortex-A9 rd rich OS and 3 party applications Cortex-A8 Cortex-A7 ARM Cortex-R family: Cortex-A5 . Cortex-R7 . Embedded processors for real-time Cortex-R5 signal processing, control applications Cortex-R4 Cortex-M4 . ARM Cortex-M family: Cortex-M3 Cortex-M1 . Microcontroller-oriented processors Cortex-M0 for MCU, ASSP, and SoC applications SC300 TM SC000 Applicability Unparalleled . ARM SecureCore Cortex-M0+ . Tamper-resistant security <12k gates... 4 ARM Cortex-M: Ultra Low Power, Size, + Cost 1.9 billion ARM Cortex-M devices shipped in 2012 by leading semiconductor companies MCUs radios sensors Think Powered by Watch Batteries & Energy Harvesting 5 MBED: Enabling Monetization of Disruption “By 2018, 50% of IoT solutions will be from start-ups less than 3 years old” - Gartner 6 From Sensor to Cloud Edge Clients Gateway Network Cloud Temp thin client Device Prox Provisioning and M2M Apps control Cortex-M Modem Diagnostics M2M Apps Smartphone / M2M Apps Short-Range Headless Radio e.g. -
Ultra-High-Energy Cosmic-Ray Nuclei and Neutrinos in Models of Gamma-Ray Bursts and Extragalactic Propagation
Ultra-high-energy cosmic-ray nuclei and neutrinos in models of gamma-ray bursts and extragalactic propagation DISSERTATION zur Erlangung des akademischen Grades doctor rerum naturalium (Dr. rer. nat.) im Fach: Physik Spezialisierung: Theoretische Physik eingereicht an der Mathematisch-Naturwissenschaftlichen Fakultät der Humboldt-Universität zu Berlin von M.Sc. Jonas Heinze Präsidentin der Humboldt-Universität zu Berlin: Prof. Dr.-Ing. Dr. Sabine Kunst Dekan der Mathematisch-Naturwissenschaftlichen Fakultät: Prof. Dr. Elmar Kulke Gutachter: 1. PD Dr. Walter Winter 2. Prof. Dr. Thomas Lohse 3. Prof. Dr. Günter Sigl Tag der mündlichen Prüfung: 27. Januar 2020 Selbständigkeitserklärung Ich erkläre, dass ich die Dissertation selbständig und nur unter Verwendung der von mir gemäß § 7 Abs. 3 der Promotionsordnung der Mathematisch-Naturwissenschaftlichen Fakultät, veröf- fentlicht im Amtlichen Mitteilungsblatt der Humboldt-Universität zu Berlin Nr. 42/2018 am 11.07.2018, angegebenen Hilfsmittel angefertigt habe. Abstract Ultra-high-energy cosmic rays (UHECRs) are the most energetic particles observed in the Uni- verse. Their energy spectrum, chemical composition and arrival directions are observed in extensive air-shower (EAS) experiments, notably the Pierre Auger Observatory (Auger) and Telescope Array (TA). While the astrophysical sources of UHECRs have not yet been uniquely identified, there are strong indications for an extragalactic origin. The interpretation of theob- servations requires both simulations of UHECR acceleration and energy losses inside the source environment as well as interactions during extragalactic propagation. Due to their extreme en- ergies, UHECR will interact with photons in these environments, producing a flux of secondary neutrinos. The IceCube observatory has detected a neutrino flux of astrophysical origin, which likely consists of neutrinos from astrophysical sources and not of neutrinos produced during extragalactic propagation of UHECRs (so-called ‘cosmogenic’ neutrinos). -
Cybercrime Prevention Principles for Internet Service Providers
Shaping the Future of Cybersecurity and Digital Trust Cybercrime Prevention Principles for Internet Service Providers January 2020 World Economic Forum 91-93 route de la Capite CH-1223 Cologny/Geneva Switzerland Tel.: +41 (0)22 869 1212 Fax: +41 (0)22 786 2744 Email: [email protected] www.weforum.org © 2020 World Economic Forum. All rights reserved. No part of this publication may be reproduced or transmitted in any form or by any means, including photocopying and recording, or by any information storage and retrieval system. 1 Cybercrime Prevention: Principles for Internet Service Providers Contents Preface 3 Foreword 4 Executive Summary 5 Incentives for Action and Expected Outcomes 6 Context – Scale of the Threat 7 Principle 1. Protect consumers by default from widespread cyberattacks and act collectively with peers to identify and respond to known threats 8 1.1 What challenge does this principle address? 8 1.2 How can this principle create impact? 8 1.3 Recommendations for implementation 10 Principle 2. Take action to raise awareness and understanding of threats and support consumers in protecting themselves and their networks 11 2.1 What challenge does this principle address? 11 2.2 How can this principle create impact? 12 2.3 Recommendations for implementation 14 Principle 3. Work more closely with manufacturers and vendors of hardware, software and infrastructure to raise minimum levels of security 16 3.1 What challenge does this principle address? 16 3.2 How can this principle create impact? 16 3.3 Recommendations for implementation -
Estudio De Un Slot Digital E Implementación De Nuevas
ESCUELA TÉCNICA SUPERIOR DE INGENIERÍA INFORMÁTICA INGENIERÍA INFORMÁTICA – GRADO EN INGENIERÍA DE COMPUTADORES Sistema embebido para recolección de datos ambientales alojado en bicicletas de uso público. Realizado por ABDESSAMAD EL ABBASSI HAMIDI Dirigido por DANIEL CAGIGAS MUÑIZ Departamento ARQUITECTURA Y TECNOLOGÍA DE COMPUTADORES Sevilla, 11 Septiembre de 2014 1 2 Contenido ÍNDICE DE FIGURAS ............................................................................ 5 INTRODUCCIÓN .................................................................................. 6 Motivación ..................................................................................... 6 Objetivos........................................................................................ 6 Análisis de requisitos ...................................................................... 7 DESARROLLO DEL SISTEMA ................................................................. 15 Introducción .................................................................................. 15 Desarrollo hardware ....................................................................... 20 Sistema de montaje y Alimentación .............................................. 20 Microcontrolador Cortex-M3 NXP LPC1768 .................................... 21 Introduccion ............................................................................ 21 Características LPC1768 ............................................................ 24 Sensores de gases resistivos ........................................................