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The Early Explorers by Andrew J
The Early Explorers by Andrew J. LePage August 8, 1999 Among these programs were the next generation of Introduction Explorer satellites the ABMA was planning. In the chaos that swept the United States after the launching of the first Soviet Sputniks, a variety of The First New Explorers satellite programs was sponsored by the Department The first of the new series of larger Explorer satellites of Defense (DoD) to supplement (and in some cases was the 39.7 kilogram (87.5 pound) satellite NASA supplant) the country's flagging "official" satellite designated as S-1. Built by JPL, the spin stabilized program, Vanguard. One of the stronger programs S-1 consisted of a pair of fiberglass cones joined at was sponsored by the ABMA (Army Ballistic Missile their bases with a diameter and height of 76 Agency) with its engineering team lead by the centimeters each. The scientific payload consisted of German rocket expert, Wernher von Braun. Using instruments to study cosmic rays, solar X-ray and the Juno I launch vehicle, the ABMA team launched ultraviolet emissions, micrometeorites, as well as the America's first satellite, Explorer 1, which was built globe's heat balance. This was all powered by a bank by Caltech's Jet Propulsion Laboratory (JPL) (see of 15 nickel-cadmium batteries recharged by 3,000 Explorer: America's First Satellite in the February solar cells mounted on the satellite's exterior. This 1998 issue of SpaceViews). advanced payload was equipped with a timer to turn itself off after a year in orbit. While these first satellites returned a wealth of new data, they were limited by the tiny 11 kilogram (25 Explorer S-1 was launched from Cape Canaveral on pound) payload capability of the Juno I. -
Getting Started with Your VXI-1394 Interface for Windows NT/98 And
VXI Getting Started with Your VXI-1394 Interface for Windows NT/98 VXI-1394 Interface for Windows NT/98 November 1999 Edition Part Number 322109D-01 Worldwide Technical Support and Product Information www.ni.com National Instruments Corporate Headquarters 11500 North Mopac Expressway Austin, Texas 78759-3504 USA Tel: 512 794 0100 Worldwide Offices Australia 03 9879 5166, Austria 0662 45 79 90 0, Belgium 02 757 00 20, Brazil 011 284 5011, Canada (Calgary) 403 274 9391, Canada (Ontario) 905 785 0085, Canada (Québec) 514 694 8521, China 0755 3904939, Denmark 45 76 26 00, Finland 09 725 725 11, France 01 48 14 24 24, Germany 089 741 31 30, Greece 30 1 42 96 427, Hong Kong 2645 3186, India 91805275406, Israel 03 6120092, Italy 02 413091, Japan 03 5472 2970, Korea 02 596 7456, Mexico (D.F.) 5 280 7625, Mexico (Monterrey) 8 357 7695, Netherlands 0348 433466, Norway 32 27 73 00, Poland 48 22 528 94 06, Portugal 351 1 726 9011, Singapore 2265886, Spain 91 640 0085, Sweden 08 587 895 00, Switzerland 056 200 51 51, Taiwan 02 2377 1200, United Kingdom 01635 523545 For further support information, see the Technical Support Resources appendix. To comment on the documentation, send e-mail to [email protected] © Copyright 1998, 1999 National Instruments Corporation. All rights reserved. Important Information Warranty The National Instruments VXI-1394 board is warranted against defects in materials and workmanship for a period of one year from the date of shipment, as evidenced by receipts or other documentation. National Instruments will, at its option, repair or replace equipment that proves to be defective during the warranty period. -
A Technology Comparison Adopting Ultra-Wideband for Memsen’S File Sharing and Wireless Marketing Platform
A Technology Comparison Adopting Ultra-Wideband for Memsen’s file sharing and wireless marketing platform What is Ultra-Wideband Technology? Memsen Corporation 1 of 8 • Ultra-Wideband is a proposed standard for short-range wireless communications that aims to replace Bluetooth technology in near future. • It is an ideal solution for wireless connectivity in the range of 10 to 20 meters between consumer electronics (CE), mobile devices, and PC peripheral devices which provides very high data-rate while consuming very little battery power. It offers the best solution for bandwidth, cost, power consumption, and physical size requirements for next generation consumer electronic devices. • UWB radios can use frequencies from 3.1 GHz to 10.6 GHz, a band more than 7 GHz wide. Each radio channel can have a bandwidth of more than 500 MHz depending upon its center frequency. Due to such a large signal bandwidth, FCC has put severe broadcast power restrictions. By doing so UWB devices can make use of extremely wide frequency band while emitting very less amount of energy to get detected by other narrower band devices. Hence, a UWB device signal can not interfere with other narrower band device signals and because of this reason a UWB device can co-exist with other wireless devices. • UWB is considered as Wireless USB – replacement of standard USB and fire wire (IEEE 1394) solutions due to its higher data-rate compared to USB and fire wire. • UWB signals can co-exists with other short/large range wireless communications signals due to its own nature of being detected as noise to other signals. -
Windows 7 Operating Guide
Welcome to Windows 7 1 1 You told us what you wanted. We listened. This Windows® 7 Product Guide highlights the new and improved features that will help deliver the one thing you said you wanted the most: Your PC, simplified. 3 3 Contents INTRODUCTION TO WINDOWS 7 6 DESIGNING WINDOWS 7 8 Market Trends that Inspired Windows 7 9 WINDOWS 7 EDITIONS 10 Windows 7 Starter 11 Windows 7 Home Basic 11 Windows 7 Home Premium 12 Windows 7 Professional 12 Windows 7 Enterprise / Windows 7 Ultimate 13 Windows Anytime Upgrade 14 Microsoft Desktop Optimization Pack 14 Windows 7 Editions Comparison 15 GETTING STARTED WITH WINDOWS 7 16 Upgrading a PC to Windows 7 16 WHAT’S NEW IN WINDOWS 7 20 Top Features for You 20 Top Features for IT Professionals 22 Application and Device Compatibility 23 WINDOWS 7 FOR YOU 24 WINDOWS 7 FOR YOU: SIMPLIFIES EVERYDAY TASKS 28 Simple to Navigate 28 Easier to Find Things 35 Easy to Browse the Web 38 Easy to Connect PCs and Manage Devices 41 Easy to Communicate and Share 47 WINDOWS 7 FOR YOU: WORKS THE WAY YOU WANT 50 Speed, Reliability, and Responsiveness 50 More Secure 55 Compatible with You 62 Better Troubleshooting and Problem Solving 66 WINDOWS 7 FOR YOU: MAKES NEW THINGS POSSIBLE 70 Media the Way You Want It 70 Work Anywhere 81 New Ways to Engage 84 INTRODUCTION TO WINDOWS 7 6 WINDOWS 7 FOR IT PROFESSIONALS 88 DESIGNING WINDOWS 7 8 WINDOWS 7 FOR IT PROFESSIONALS: Market Trends that Inspired Windows 7 9 MAKE PEOPLE PRODUCTIVE ANYWHERE 92 WINDOWS 7 EDITIONS 10 Remove Barriers to Information 92 Windows 7 Starter 11 Access -
LPT, COM, 1394, USB, USB-C LPT IEEE 1284, LPT (Англ. Line Print Terminal; Также Параллельный Порт, По
LPT, COM, 1394, USB, USB-C LPT IEEE 1284, LPT (англ. Line Print Terminal; также параллельный порт, порт принтера) — международный стандарт параллельного интерфейса для подключения периферийных устройств персонального компьютера. В основном используется для подключения к компьютеру принтера, сканера и других внешних устройств (часто использовался для подключения внешних устройств хранения данных), однако может применяться и для других целей (организация связи между двумя компьютерами, подключение каких-либо механизмов телесигнализации и телеуправления). В основе данного стандарта лежит интерфейс Centronics и его расширенные версии (ECP, EPP). Название LPT образовано от наименования стандартного устройства принтера LPT1 (Line Printer Terminal или Line PrinTer) в операционных системах семейства MS-DOS. Параллельный порт Centronics — порт, используемый с 1981 года в персональных компьютерах фирмы IBM для подключения печатающих устройств, разработан фирмой Centronics Data Computer Corporation; уже давно стал стандартом де-факто, хотя в действительности официально на данный момент он не стандартизирован. Изначально этот порт был разработан только для симплексной (однонаправленной) передачи данных, так как предполагалось, что порт Centronics должен использоваться только для работы с принтером. Впоследствии разными фирмами были разработаны дуплексные расширения интерфейса (byte mode, EPP, ECP). Затем был принят международный стандарт IEEE 1284, описывающий как базовый интерфейс Centronics, так и все его расширения. Разъемы. Порт на стороне управляющего -
PC 97 Hardware Design Guide
Part 4 — Device Design Guidelines CHAPTER 21 Printers This chapter presents the requirements and recommendations for printers under the Microsoft Windows family of operating systems. Version 1.1 Includes changes to References for Printers Contents Overview for Printers.............................. ............... 312 Basic Printer Features............................. ................ 312 Basic Features for IEEE 1394 Printers. ................. 312 Basic Features for USB Printers . ............... 312 Basic Features for IEEE 1284 Printers. ................. 313 PC 97 Design for Printers .......................... ................ 314 Plug and Play for Printers. ............... 314 Power Management for Print Components . .............. 315 Device Drivers and Installation for Printers . .................... 315 References for Printers ............................ ................ 318 Checklist for Printers ............................. ................ 320 312 PC 97 Design — Part 4 Device Design Guidelines Overview for Printers This section presents the key design issues for printers under Microsoft Windows. Printers and other devices attached to parallel ports should be capable of high- speed, bidirectional data transfers. The design criteria for parallel devices follow those for parallel ports described in the “Serial, Parallel, and Wireless Support” chapter. The PC 97 requirements for printers and parallel ports seek to ensure the following: • Ensure maximum speed for transfer of parallel data between the system and the peripheral. • Ensure a true Plug and Play experience for users. Basic Printer Features This section summarizes the basic hardware requirements for printers for PC 97. Basic Features for IEEE 1394 Printers This section defines requirements for printers that use IEEE 1394. 1. Compliance with PC 97 requirements for IEEE 1394 Required This bus is recommended in PC 97 for support of fast, high-density data transfer. For information about implementing IEEE 1394 for PC 97, see the “IEEE 1394” chapter in Part 3 of this guide. -
From Camac to Wireless Sensor Networks and Time- Triggered Systems and Beyond: Evolution of Computer Interfaces for Data Acquisition and Control
Janusz Zalewski / International Journal of Computing, 15(2) 2016, 92-106 Print ISSN 1727-6209 [email protected] On-line ISSN 2312-5381 www.computingonline.net International Journal of Computing FROM CAMAC TO WIRELESS SENSOR NETWORKS AND TIME- TRIGGERED SYSTEMS AND BEYOND: EVOLUTION OF COMPUTER INTERFACES FOR DATA ACQUISITION AND CONTROL. PART I Janusz Zalewski Dept. of Software Engineering, Florida Gulf Coast University Fort Myers, FL 33965, USA [email protected], http://www.fgcu.edu/zalewski/ Abstract: The objective of this paper is to present a historical overview of design choices for data acquisition and control systems, from the first developments in CAMAC, through the evolution of their designs operating in VMEbus, Firewire and USB, to the latest developments concerning distributed systems using, in particular, wireless protocols and time-triggered architecture. First part of the overview is focused on connectivity aspects, including buses and interconnects, as well as their standardization. More sophisticated designs and a number of challenges are addressed in the second part, among them: bus performance, bus safety and security, and others. Copyright © Research Institute for Intelligent Computer Systems, 2016. All rights reserved. Keywords: Data Acquisition, Computer Control, CAMAC, Computer Buses, VMEbus, Firewire, USB. 1. INTRODUCTION which later became international standards adopted by IEC and IEEE [4]-[7]. The design and development of data acquisition The CAMAC standards played a significant role and control systems has been driven by applications. in developing data acquisition and control The earliest and most prominent of those were instrumentation not only for nuclear research, but applications in scientific experimentation, which also for research in general and for industry as well arose in the early sixties of the previous century, [8]. -
The Space Infrared Interferometric Telescope (SPIRIT): High- Resolution Imaging and Spectroscopy in the Far-Infrared
Leisawitz, D. et al., J. Adv. Space Res., in press (2007), doi:10.1016/j.asr.2007.05.081 The Space Infrared Interferometric Telescope (SPIRIT): High- resolution imaging and spectroscopy in the far-infrared David Leisawitza, Charles Bakera, Amy Bargerb, Dominic Benforda, Andrew Blainc, Rob Boylea, Richard Brodericka, Jason Budinoffa, John Carpenterc, Richard Caverlya, Phil Chena, Steve Cooleya, Christine Cottinghamd, Julie Crookea, Dave DiPietroa, Mike DiPirroa, Michael Femianoa, Art Ferrera, Jacqueline Fischere, Jonathan P. Gardnera, Lou Hallocka, Kenny Harrisa, Kate Hartmana, Martin Harwitf, Lynne Hillenbrandc, Tupper Hydea, Drew Jonesa, Jim Kellogga, Alan Koguta, Marc Kuchnera, Bill Lawsona, Javier Lechaa, Maria Lechaa, Amy Mainzerg, Jim Manniona, Anthony Martinoa, Paul Masona, John Mathera, Gibran McDonalda, Rick Millsa, Lee Mundyh, Stan Ollendorfa, Joe Pellicciottia, Dave Quinna, Kirk Rheea, Stephen Rineharta, Tim Sauerwinea, Robert Silverberga, Terry Smitha, Gordon Staceyf, H. Philip Stahli, Johannes Staguhn j, Steve Tompkinsa, June Tveekrema, Sheila Walla, and Mark Wilsona a NASA’s Goddard Space Flight Center, Greenbelt, MD b Department of Astronomy, University of Wisconsin, Madison, Wisconsin, USA c California Institute of Technology, Pasadena, CA, USA d Lockheed Martin Technical Operations, Bethesda, Maryland, USA e Naval Research Laboratory, Washington, DC, USA f Department of Astronomy, Cornell University, Ithaca, USA g Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA h Astronomy Department, University of Maryland, College Park, Maryland, USA i NASA’s Marshall Space Flight Center, Huntsville, Alabama, USA j SSAI, Lanham, Maryland, USA ABSTRACT We report results of a recently-completed pre-Formulation Phase study of SPIRIT, a candidate NASA Origins Probe mission. SPIRIT is a spatial and spectral interferometer with an operating wavelength range 25 - 400 µm. -
Cable Discharge Event (CDE) Automated Test System Based on TLP Method
Cable Discharge Event (CDE) Automated Test System Based on TLP Method Draft V3-2016.03.18 Wei Huang, Jerry Tichenor Web: www.esdemc.com Email: [email protected] Tel: (+1) 573-202-6411 Fax: (+1) 877-641-9358 Address: 4000 Enterprise Drive, Suite 103, Rolla, MO, 65401 Cable Discharge Event (CDE) Background What is CDE Event ? A Cable Discharge Event (CDE) is electrostatic discharge(s) between metal of a cable connector and the mating cable connector or plug. It is very common in daily life. When CDE happens, transient high current and high voltage pulses are generated into the connector pins and cause potential damage to the system with connector. The pulse characteristic is determined by the cable type, cable length, physical arrangement of the cable and system with connector, and system with connector side circuitry. A Generic CDE System Concept Why understanding CDE robustness is important ? The discharge processes are complicated due to the number of pins involved and their connections to a system. In addition, the occurrence rate and severity of the static discharge is important to design a robust system. Basic System Features: A well repeatable test setup to reproduce cable discharge events Pulse injection level covers different types of cable connections Additional System Features: Automatic computer controlled test for all available connector pins Automatic remove DUT residue charge safely after each pulse safely Integrate current and voltage probes to monitor CDE events on each pin ESDEMC Collected Cable Pins and Practical Passive -
Nowak 2019 Apj 874 69
Downloaded from orbit.dtu.dk on: Oct 05, 2021 Chandra-HETGS Characterization of an Outflowing Wind in the Accreting Millisecond Pulsar IGR J17591–2342 Nowak, Michael A.; Paizis, Adamantia; Jaisawal, Gaurava Kumar; Chenevez, Jerome; Chaty, Sylvain; Fortin, Francis; Rodriguez, Jerome; Wilms, Jorn Published in: Astrophysical Journal Link to article, DOI: 10.3847/1538-4357/ab0a71 Publication date: 2019 Document Version Publisher's PDF, also known as Version of record Link back to DTU Orbit Citation (APA): Nowak, M. A., Paizis, A., Jaisawal, G. K., Chenevez, J., Chaty, S., Fortin, F., Rodriguez, J., & Wilms, J. (2019). Chandra-HETGS Characterization of an Outflowing Wind in the Accreting Millisecond Pulsar IGR J17591–2342. Astrophysical Journal, 874(1), [69]. https://doi.org/10.3847/1538-4357/ab0a71 General rights Copyright and moral rights for the publications made accessible in the public portal are retained by the authors and/or other copyright owners and it is a condition of accessing publications that users recognise and abide by the legal requirements associated with these rights. Users may download and print one copy of any publication from the public portal for the purpose of private study or research. You may not further distribute the material or use it for any profit-making activity or commercial gain You may freely distribute the URL identifying the publication in the public portal If you believe that this document breaches copyright please contact us providing details, and we will remove access to the work immediately and investigate your claim. The Astrophysical Journal, 874:69 (13pp), 2019 March 20 https://doi.org/10.3847/1538-4357/ab0a71 © 2019. -
Astronomy Magazine 2011 Index Subject Index
Astronomy Magazine 2011 Index Subject Index A AAVSO (American Association of Variable Star Observers), 6:18, 44–47, 7:58, 10:11 Abell 35 (Sharpless 2-313) (planetary nebula), 10:70 Abell 85 (supernova remnant), 8:70 Abell 1656 (Coma galaxy cluster), 11:56 Abell 1689 (galaxy cluster), 3:23 Abell 2218 (galaxy cluster), 11:68 Abell 2744 (Pandora's Cluster) (galaxy cluster), 10:20 Abell catalog planetary nebulae, 6:50–53 Acheron Fossae (feature on Mars), 11:36 Adirondack Astronomy Retreat, 5:16 Adobe Photoshop software, 6:64 AKATSUKI orbiter, 4:19 AL (Astronomical League), 7:17, 8:50–51 albedo, 8:12 Alexhelios (moon of 216 Kleopatra), 6:18 Altair (star), 9:15 amateur astronomy change in construction of portable telescopes, 1:70–73 discovery of asteroids, 12:56–60 ten tips for, 1:68–69 American Association of Variable Star Observers (AAVSO), 6:18, 44–47, 7:58, 10:11 American Astronomical Society decadal survey recommendations, 7:16 Lancelot M. Berkeley-New York Community Trust Prize for Meritorious Work in Astronomy, 3:19 Andromeda Galaxy (M31) image of, 11:26 stellar disks, 6:19 Antarctica, astronomical research in, 10:44–48 Antennae galaxies (NGC 4038 and NGC 4039), 11:32, 56 antimatter, 8:24–29 Antu Telescope, 11:37 APM 08279+5255 (quasar), 11:18 arcminutes, 10:51 arcseconds, 10:51 Arp 147 (galaxy pair), 6:19 Arp 188 (Tadpole Galaxy), 11:30 Arp 273 (galaxy pair), 11:65 Arp 299 (NGC 3690) (galaxy pair), 10:55–57 ARTEMIS spacecraft, 11:17 asteroid belt, origin of, 8:55 asteroids See also names of specific asteroids amateur discovery of, 12:62–63 -
Desktop Troubleshooting and Configuration Guide
Desktop Troubleshooting and Configuration Guide Product and Versions Contract Version 6.8.1 Document Dated August, 2011, Updated November, 2013 Overview of Known Issues Prodagio Contract is a browser based application. This Guide details the known issues and troubleshooting recommendations, as well as the desktop hardware and software requirements to optimize Prodagio Contact 6.8.1 performance. This document is intended for use by those IT members responsible for desktop management and third-party software configuration. Troubleshooting issues are grouped as follows: UCF and Java related issues Java only issues Browser issues Drag and Drop issues Add-On issues Workflow Instances issues An Appendix details recommended browser hardware, software and operating environments and provides more details about the role of UCF and how it can be pre-installed. The Table of Contents on the next page lists more details of this Guide’s various sections. Note: the screen captures used in this document are from Internet Explorer 9 and Windows 7. The appearance of your screen captures many differ if using other browsers and browser versions and operating system versions. If at all possible, troubleshooting issues in the order presented in this document. Desktop Troubleshooting and Configuration Guide — Prodagio Contract Page 1 Table of Contents Overview of Known Issues ........................................................................................................................ 1 UCF and Java Issues Defined .................................................................................................................