Group-Based Discovery in Low-Duty-Cycle Mobile Sensor Networks

Total Page:16

File Type:pdf, Size:1020Kb

Group-Based Discovery in Low-Duty-Cycle Mobile Sensor Networks 2012 9th Annual IEEE Communications Society Conference on Sensor, Mesh and Ad Hoc Communications and Networks (SECON) Group-based Discovery in Low-duty-cycle Mobile Sensor Networks Liangyin Chen∗,YuGu†, Shuo Guo§,TianHe§, Yuanchao Shu‡†, Fan Zhang‡ and Jiming Chen‡ ∗College of Computer Science, Sichuan University † Singapore University of Technology and Design §Department of Computer Science and Engineering, University of Minnesota ‡ Department of Control, Zhejiang University Abstract—Wireless Sensor Networks have been used in many is to reduce duty-cycle by listening briefly and shutting down mobile applications such as wildlife tracking and participatory radios most of the time (e.g., 99% or more). Such a simple urban sensing. Because of the combination of high mobility and low-duty-cycle operation, however, leads to a challenging low-duty-cycle operations, it is a challenging issue to reduce discovery delay among mobile nodes, so that mobile nodes can issue: how nodes within physical vicinity can discovery each establish connection quickly once they are within each other’s other if they listen to the channel in an asynchronous manner. vicinity. Existing discovery designs are essentially pair-wise based, This issue becomes even more challenging when low-duty- in which discovery is passively achieved when two nodes are cycle operation is combined with the mobility of sensor nodes pre-scheduled to wake-up at the same time. In contrast, for in many applications such as in ZerbraNet [7], opportunistic the first time, this work reduces discovery delay significantly by proactively referring wake-up schedules among a group of data collection (SNIP) [19] and urban sensing [5]. Because nodes. Because proactive references incur additional overhead, mobility invalidates many assumptions implicit in low power we introduce a novel selective reference mechanism based on static designs [4], such a combination imposes a time con- spatiotemporal properties of neighborhood and the mobility of straint on how fast nodes shall finish discovery before they the nodes. Our quantitative analysis indicates that the discovery are physically disconnected. delay of our group-based mechanism is significantly smaller than that of the pair-wise one. Our testbed experiments using Node discovery in low-duty-cycle network has attracted 40 sensor nodes confirm our theoretical analysis, showing one research attention in recent years. Previous works mainly focus order of magnitude reduction in discovery delay compared with on how to ensure a pair of nodes can wake up simultaneously traditional pair-wise methods with only 0.5%∼8.8% increase in through a certain type of scheduling algorithms. Notable energy consumption. discovery designs include: stochastic-based protocols [2], [13], quorum-based protocols [11], [12], [16], [20], Disco [3] and I. INTRODUCTION U-Connect [8]. These designs successfully ensure that a pair Wireless Sensor Networks have been proposed for use in of nodes finish discovery within a bounded delay. Although lit- many challenging applications, such as military surveillance, erature is encouraging, we believe there are rooms to improve. scientific exploration and structural monitoring. Sustainable Specifically, we notice all existing designs essentially are pair- deployment of these systems calls for energy-efficient designs. wise based. Discovery is achieved only when two nodes are Extensive research has indicated that energy in low-power pre-scheduled to wake-up simultaneously. However, if nodes sensors is consumed mostly by being ready for potential can share their known schedules with each other, discovery incoming packets, a problem commonly referred to as idle can be achieved in a more proactive and fast manner with listening. For example, the widely used ChipCon CC2420 small overhead. radio [1] draws 19.7mA when receiving or idle listening, This paper presents a Group-based Discovery method as which is actually larger than the 17.4mA used when trans- a performance add-on to existing pair-wise mobile discovery mitting. More importantly, packet transmission time is usually designs. It essentially builds a schedule reference mechanism very small (e.g., about 1 millisecond to transmit a TinyOS among nodes to expedite the discovery process. The operation packet using a CC2420 radio), while the duration of idle of schedule reference is straightforward. For example, after listening for reception can be orders of magnitude longer. node A discovers node B using a traditional pair-wise method, For example, most environmental applications, such as Great node B can proactively refer (push) the wakeup-schedules of Duck Island [15], sample the environment at relatively low its known neighbors (such as node C) to node A. Consequent- rates (on the order of minutes between samples). With a ly, node A can quickly discover node C indirectly via node comparable current draw and a 3∼4 orders of magnitude B. Clearly, excessive reference operations would introduce longer duration waiting for reception, idle listening is a major high overhead in communication. The challenging issue of energy drain that, if not optimized, accounts for most energy our work is to design a selective reference mechanism to trade in communication. off between reducing discovery delay and overhead to achieve Therefore, the most effective energy conservation technique that. 978-1-4673-1905-8/12/$31.00 ©2012 IEEE 542 In summary, our contributions are as follows: a centralized solution. To provide a distributed solution in an • To the best of our knowledge, all previous work focuses asymmetric design, Disco [3] introduces a neighbor discovery on scheduling designs for pair-wise discovery. We inves- method based on the Chinese Reminder Theorem [14], in tigate how group-based discovery can reduce discovery which each node selects a pair of primes as period inde- delay with small overhead. We are the first to provide pendently based on the requirement of its duty cycle. For theoretical analysis of group-based discovery delay for example, if node i select Ti0 and Ti1 as its working periods, mobile low-duty-cycle networks and compared with pair- after node i start to work, once its time counter can divide by wise one. Ti0 or Ti1, it will wake up, or else be in sleep. In addition to • Utilizing spatiotemporal properties of neighborhood, we Disco [3], CQS-pair [12] and GQS-pair [11] present wakeup propose a selective reference mechanism that can avoid scheduling schemes for heterogeneous quorum-based system. unnecessary references while still speeding up overall Using heterogeneous quorums, nodes can have different cycle discovery process. lengths and hence different duty-cycle settings. Recently, U- • We implement and evaluate our design in a physical test- connect [8] proposes a unified neighbor discovery protocol bed consisting of 40 nodes, indicating that our design is for symmetric and asymmetric duty cycle settings. Specifi- suitable for resource constrained sensor nodes. One order cally authors show that U-Connect is an 1.5-approximation of magnitude reduction in discovery delay indicates our algorithm for the symmetric asynchronous discovery scenario, design is very effective for mobile sensor network with and the existing protocols such as Quorum and Disco are 2- high density. approximation algorithms. The rest of the paper is organized as follows: Section II Although neighbor discovery techniques are diverse, all of discusses the related work. Section III introduces the network them focus on pair-wise discovery. None of aforementioned model and assumptions. Section IV introduces the basic design works investigate how to increase discovery probability and and makes a theoretical analysis of discovery delay. Section V decrease discovery delay by sharing schedule information introduces an advanced selective reference design. Section VI among a group of nodes during the discovery process. In this presents the experiment results using a 40-node testbed. Sec- work, we introduce a generic reference mechanism on top of tion VII concludes the work. current discovery methods. It serves as a performance add-on to existing discovery methods, therefore is complementary to II. RELATED WORK the state-of-the-art. Node discovery is nothing new and has a rich literature in both ad hoc and wireless sensor networks. Discovery in III. SYSTEM MODELS AND ASSUMPTIONS always-awake networks mainly focuses on network models In this section, we define the network model and as- with directional antennas [17], [6], [18], while solutions for sumptions related to group-based discovery design for mobile discovery in duty-cycled networks are highly diverse, especial- networks. ly in mobile environments which impose time constraints on how fast discovery should be finished. Notable ones includes: A. Network Model stochastic-based protocols [13], [2], quorum-based protocol- s [16], [20], [12], [11], Disco [3], U-Connect [8], multi- We assume a network with n mobile nodes running under channel discovery [9] and collision-aware discovery [10]. In a low-duty-cycle mode, i.e., a node remains dormant most of birthday protocol [13], nodes listen, transmit or sleep in a time and becomes active only briefly (e.g., less than 5%) to probabilistic round-robin fashion, which statistically trades sense and communicate. When a node is in the active state, it off between discovery energy with discovery latency. Due to can receive packets transmitted from neighboring nodes. When the stochastic nature of its operation, there is no guarantee a node is in the dormant state, it turns off all function modules on the worst-case discovery latency. Quorum-based protocol- except a timer for the purpose of waking itself up. In other s [16], [20], [12], [11] address this limitation by ensuring words, a node can wake up to transmit a packet at any time, existence of overlapped wake-up durations between pair-wise but can receive packets only when it is in its active state. nodes within a bounded time. For instances, in [16], Tseng The working schedule of a mobile node denotes the active- construct a m×m grid matrix within contiguous slots.
Recommended publications
  • DOCUMENT RESUME ED 262 129 UD 024 466 Hawaiian Studies
    DOCUMENT RESUME ED 262 129 UD 024 466 TITLE Hawaiian Studies Curriculum Guide. Grades K-1. INSTITUTION Hawaii State Dept. of Education, Honolulu. Office of Instructional Services. PUB DATE Dec 83 NOTE 316p.; For the Curriculum Guides for Grades 2,3, and 4, see UD 024 467-468, and ED 255 597. "-PUB TYPE Guides Classroom Use - Guides (For Teachers) (052) EDRS PRICE MF01/PC13 Plus Postage. DESCRIPTORS Community Resources; *Cultural Awareness; *Cultural Education; *Early Childhood Education; Grade 1; Hawaiian; *Hawaiians; Instructional Materials; Kindergarten; *Learning Activities; Pacific Americans; *Teacher Aides; Vocabulary IDENTIFIERS *Hawaii ABSTRACT This curriculum guide suggests activities and educational experiences within a Hawaiian cultural context for kindergarten and Grade 1 students in Hawaiian schools. First, a introduction-discusses the contents of the guide, the relations Hip of - the classroom teacher and the kupuna (ljawaiian-speaking elder); the identification and scheduling of Kupunas; and how to use the ide. The remainder of the guide is divided into two major sections. Each is preceded by an overview which outlines the subject areas into which Hawaiian Studies instruction is integrated; the emphases or major lesson topics taken up within each subject, area; the learning objectives addressed by the instructional activities; and a key to the unit's appendices, which provide cultural information to supplement the activities. The activities in Unit I focus on the "self" and the immediate environment. They are said to give children ___Dppor-tumit-ies to investigate and experience feelings and ideas and then to determine whether they are acceptable within classroom and home situations. The activities of Unit II involve the children in experiences dealing with the "'ohana" (family) by having them identify roles, functions, dependencies, rights, responsibilities, occupations, and other cultural characteristics of the 'ohana.
    [Show full text]
  • Discovery III Multimedia Installation V1.2
    Land Rover Discovery 3 Extending the multimedia capabilities of the Discovery III An installation guide to add a GVIF interface, a rear view camera and a DVD player to your Discovery III. A www.disco3.co.uk resource Version 1.2 © Copyright discoBizz Disclaimer: this guide is for information and illustration ONLY. Any work you do on your car, either explicitly or implicitly following this guide, is at your own risk and with the understanding the steps followed below have worked for me, in my car, at my own risk and given my own knowledge of the matter and with my own disregard to potential consequences on the vehicle’s warranty. Neither the author, the website WWW.DISCO3.CO.UK, Martin Lewis or and other website forum members mentioned in this document will be held liable for any warranty consequences or any damage of any severity caused on your vehicle as a result of you choosing to follow this fictional procedure. Any trademarks, copyright or references to words or actions of individuals other than the author, are hereby acknowledged to be the property of their respective owners. The author is simply an enthusiast, with no training at all in electrical or mechanical engineering and as such some of the methods and procedures used may be far from best practice in each respective field. N.B. The modifications/additions in this document can be done separately and in varying ways/locations. I have chosen to put everything together as I did most of the work in one go. My vehicle is an HSE model, which means it was already fitted with the factory SatNav screen and the auxiliary audio input in the rear of the centre console, the wires of which I taped into to feed the head unit with the audio output from my AV sources.
    [Show full text]
  • Bodsy's Brake Bible
    Land Rover Discovery 3 Bodsy’s Brake Bible Ian Bodsworth Disco3Club.co.uk June 2010 Version 1.2a Change Record DATE Revision Update Notes Made By May 2010 1.2 Amended Torque Figures and bolt Ian Bodsworth sizes, cleaned up photo areas. Updated text. June 2010 1.2a Re-worded EPB adjust procedure, Ian Bodsworth updated EBP Allen key size. Added Change record © Copyright Ian Bodsworth 2010. All descriptions and photo’s contained within remain the property of the Author. Commercial images of products with copyrights acknowledged. E&OE. - Created by Bodsy – D3C Page 2 of 28 Table of Contents 1. Introduction ................................................................................................................................................................. 4 2. Tools that may be required ...................................................................................................................................... 5 3. Jacking Points and Axle Stands ............................................................................................................................... 6 4. How to change the Brake Pads - Front .................................................................................................................. 9 5. How to change the Brake Pads – Rear ................................................................................................................. 13 6. How to change the Brake Disks – Front ..............................................................................................................
    [Show full text]
  • JELLYBEAN JAM Songlist Medleys
    JELLYBEAN JAM songlist Medleys (Please note Medleys cannot be broken down in form) 80s- Born To Be Alive, Shake Your Groove Thing, Don’t Leave me This way, Jessie’s Girl, Video Killed The Radio Star, Its Raining Men, You Spin me Round, Love Shack, We Built This City, My Sharona 80s2- Girls Just Wanna Have Fun, Venus, Just Can’t Get Enough, Xanadu, Hungry Like The Wolf , Funky Town. Chicks- Holiday, Step Back in Time, Lets Hear It for the Boy, Express Yourself, Finally, Better the Devil You Know Disco 1 - Blame it on the Boogie, Disco Inferno, Car Wash, Celebration, We are Family, Le Freak. Disco 2 - Jungle Boogie, Upside Down, Can’t Stand the Rain, Get down on it, Funky Music, Everyone's a Winner, Can’t Get Enough of Your Love, Tragedy, Lady Marmalade, Love Is in the Air, Kung Fu Fighting Disco 3 – Give It Up, Long Train Running, That’s the Way I like It, If I Can’t Have You, Don’t Stop Till You Get Enough, Can You Feel It Disco 4 - I will survive, You should be dancing, Got To be real, Young Hearts Run Free, Do Ya think I'm Sexy, September, Hot Stuff, Boogie Wonderland. Jacko- Thriller, Shake Your Body, Billie Jean, Rock with You, Black or White, Wanna Be Starting Something, Bad Abba- Dancing Queen, SOS, Money Money Money, Ring Ring, Mamma Mia Latin – I Go To Rio, Conga, Hot Hot Hot, Copacabana, The Love Boat Mambo- Tequila, Yeh Yeh, Mambo no 5 Motown - Uptight, can’t help myself, same ole song, dancing in the street, aint too proud to beg, joy to the world, get ready , stop, its my party, never can say good bye Movie- Flashdance, fame,
    [Show full text]
  • Storage Systems Main Points
    Storage Systems Main Points • File systems – Useful abstractions on top of physical devices • Storage hardware characteristics – Magnetic disks and flash memory File Systems • Abstraction on top of persistent storage – Magnetic disk – Flash memory (e.g., USB thumb drive) • Devices provide – Storage that (usually) survives across machine crashes – Block level (random) access – Large capacity at low cost – Relatively slow performance • Magnetic disk read takes 10-20M processor instructions File System as Illusionist: Hide Limitations of Physical Storage • Persistence of data stored in file system: – Even if crash happens during an update – Even if disk block becomes corrupted – Even if flash memory wears out • Naming: – Named data instead of disk block numbers – Directories instead of flat storage – Byte addressable data even though devices are block- oriented • Performance: – Cached data – Data placement and data structure organization • Controlled access to shared data File System Abstraction • File system – Hierarchical organization (directories, subdirectories) – Access control on data • File: named collection of data – Linear sequence of bytes (or a set of sequences) – Read/write or memory mapped • Crash and storage error tolerance – Operating system crashes (and disk errors) leave file system in a valid state • Performance – Achieve close to the hardware limit* in the average case File System Abstraction • Directory – Group of named files or subdirectories – Mapping from file name to file metadata location • Path – String that uniquely
    [Show full text]
  • ©2017 Renata J. Pasternak-Mazur ALL RIGHTS RESERVED
    ©2017 Renata J. Pasternak-Mazur ALL RIGHTS RESERVED SILENCING POLO: CONTROVERSIAL MUSIC IN POST-SOCIALIST POLAND By RENATA JANINA PASTERNAK-MAZUR A dissertation submitted to the Graduate School-New Brunswick Rutgers, The State University of New Jersey In partial fulfillment of the requirements For the degree of Doctor of Philosophy Graduate Program in Music Written under the direction of Andrew Kirkman And approved by _____________________________________ _____________________________________ _____________________________________ _____________________________________ New Brunswick, New Jersey January 2017 ABSTRACT OF THE DISSERTATION Silencing Polo: Controversial Music in Post-Socialist Poland by RENATA JANINA PASTERNAK-MAZUR Dissertation Director: Andrew Kirkman Although, with the turn in the discipline since the 1980s, musicologists no longer assume their role to be that of arbiters of “good music”, the instruction of Boethius – “Look to the highest of the heights of heaven” – has continued to motivate musicological inquiry. By contrast, music which is popular but perceived as “bad” has generated surprisingly little interest. This dissertation looks at Polish post-socialist music through the lenses of musical phenomena that came to prominence after socialism collapsed but which are perceived as controversial, undesired, shameful, and even dangerous. They run the gamut from the perceived nadir of popular music to some works of the most renowned contemporary classical composers that are associated with the suffix -polo, an expression
    [Show full text]
  • Album Backup List
    Updated 20/08/2008 Index to My Albums - Quote FULL titles please File Artist Title Notes CD Year 0148 A Hi Fi Serious 128 2002 0296 A Teen Dance Ordinance VBR 2005 0047 A1 Here We Come 1999 0014 A1 A List 2000 0082 A1 Make It Good 2002 0157 Aaliyah One In A Million 128 1996 Hits & Unreleased - The Ultimate 0233 Aaliyah Collection 192 2002 0182 Aaliyah I Care 4 U 128 2002 0024/27 ABBA Gold - Greatest Hits VBR 1992 AD32 ABBA Gold - Greatest Hits CDA 1992 Thank You For The Music (3CD) 0004 ABBA Collectors set 1995 0054 ABBA The Definitive Collection (2CD) VBR 2001 AB39 ABBA The Definitive Collection (2CD) CDA 2001 0104 ABC Absolutely 1990 0118 ABC The Remix Collection 1993 AD39 ABC The Collection CDA 0070 Paula Abdul Greatest Hits Of Paula Abdul 2000 0076 Ace Of Base Ace Of Base 1983 0085 Ace Of Base Happy Nation 1993 0233 Adam & The Ants Dirk Wears White Socks 192 1979 0150 Adam & The Ants Ant Music 192 1980 0002 Adam & The Ants Friend or Foe 1982 0191 Adam & The Ants Antics In The Forbidden Zone 128 1990 0237 Adam & The Ants Very Best Of Adam & The Ants 128 1999 0194 Adam Ant Strip 256 1983 0315 Adam Ant Strip 320 1983 AD27 Adam Ant Hits CDA 0262 Bryan Adams Cuts Like A Knife 192 1990 0262 Bryan Adams Into The Fire 192 1990 0200 Bryan Adams Waking Up The Neighbours VBR 1991 0163 Bryan Adams Unplugged (Live) 128 1997 0189 Bryan Adams On A Day Like Today 320 1998 AD30 Bryan Adams On A Day Like Today CDA 1998 0198 Bryan Adams The Best Of Me VBR 1999 AD29 Bryan Adams The Best Of Me CDA 1999 0114 Bryan Adams Spirit OST 2002 0293 Bryan Adams
    [Show full text]
  • Im Not Scared! Free
    FREE IM NOT SCARED! PDF Jonathan Allen | 32 pages | 10 Jan 2008 | Boxer Books Limited | 9781905417285 | English | St Albans, United Kingdom I'm Not Scared () - IMDb The group's fifth singlethe first single from the album Fearlesswas released in Written by Pet Shop Boysthe original version contains several words in French. The 12" "disco mix" combines the two versions into one long mix. Pet Shop Boys also released their own version of the song, with Neil Tennant vocals, on the album Introspective. From Wikipedia, the free encyclopedia. Neil Tennant Chris Lowe. The Encyclopaedia of Classic 80s Pop. Yes, it's the one Im Not Scared! Patsy Kensit—who, halfway through 'Im Not Scared', an enjoyable piece of atmospheric synth-pop, delivers some French lyrics in a deliciously good accent. Slant Magazine. Im Not Scared! 16 April Ultratop Les classement single. Archived from the original on Retrieved Single Top Swiss Singles Chart. Official Charts Company. GfK Entertainment Charts. Retrieved April 7, Pet Shop Boys. Chris Lowe Neil Tennant. Disco Disco 2 Disco 3 Disco 4. Concrete Pandemonium Inner Sanctum. Christmas Agenda. Hidden Im Not Scared! Webarchive Im Not Scared! webcite links CS1 maint: archived copy as title Pages using infobox song with unknown parameters Articles with hAudio Im Not Scared! Singlechart usages for Austria Singlechart usages for Flanders Singlechart usages for France All articles with unsourced statements Articles with unsourced statements from April Singlechart usages for Dutch Singlechart usages for Switzerland Singlechart usages for UK Singlechart usages for West Germany. Namespaces Article Talk. Views Read Edit View history. Help Learn to edit Community portal Recent changes Upload file.
    [Show full text]
  • Land Rover Discovery 3
    Land Rover Discovery 3 Inexpensive AV Modification An installation guide to inexpensively add any AV source to the Discovery III A www.disco3.co.uk resource Version 1.0 © Copyright discoBizz Disclaimer: this guide is for information and illustration ONLY. Any work you do on your car, either explicitly or implicitly following this guide, is at your own risk and with the understanding the steps followed below have worked for me, in my car, at my own risk and given my own knowledge of the matter and with my own disregard to potential consequences on the vehicle’s warranty. Neither the author, the website WWW.DISCO3.CO.UK, Martin Lewis or and other website forum members mentioned in this document will be held liable for any warranty consequences or any damage of any severity caused on your vehicle as a result of you choosing to follow this fictional procedure. Any trademarks, copyright or references to words or actions of individuals other than the author, are hereby acknowledged to be the property of their respective owners. Contents Introduction ................................................................................................................................................... 2 Part I – video feed: ........................................................................................................................................ 3 Part II – audio feed: ....................................................................................................................................... 8 Further refinements: ................................................................................................................................... 11 A www.disco3.co.uk resource Page 1 Introduction This has been discussed on a number of threads and I’m not trying to re‐invent the wheel here, just thought I’d put everything in one place for future reference. I acknowledge the majority of the procedures are not my own invention and credit is due to the forum members who have posted contributions in a number of threads.
    [Show full text]
  • The Bubble Our Oak Classroom, Affectionately Known As the ‘Bubble’ Has Been Awarded Grade 2 Listed Status
    20th October 2017 The Bubble Our Oak classroom, affectionately known as the ‘Bubble’ has been awarded Grade 2 Listed status. This is part of a project run by Historic England looking at post war architecture in education. Built in 1973 – 1974, the Bubble was the first fully structural plastic building in Britain and made from GRP (glass fibre- reinforced plastic). Its design comprises of 35 white, tetrahedron panels arranged into a modified icosahedron bolted to a concrete base. The building cost £28 400 at the time which in today’s prices would have been approximately £320 000! The Bubble was a prototype built to test the new design and was intended for whole schools to be built using the architecture, one giant bubble as a hall with several smaller satellite bubbles around it as classrooms. The plans were soon abandoned due to the price of oil rising during the war in the middle east. So the Bubble remains unique in the country and maybe the world as a one off design. The granting of the status is a bit of a double-edged sword. There is great pride to be had from the listing but unfortunately no pot of money for its restoration or upkeep. Last year we had it redecorated externally but 12 months later, it is back to its black and green state. It is cold in the winter and hot in the summer and there are many areas of damp due to the condensation on the single paned windows. (continued on the next page) 1 We did have a quote for the exterior to be treated with a ‘system’ but this came in at £16 000 which the school budget cannot justify spending.
    [Show full text]
  • RSE Retrofit Guide
    A Guide to Retro-fitting the OEM Factory Supplied Rear Screen Entertainment System to a Discovery 3 HSE Since 2008 model year Land Rover finally made the RSE system available to order for the Discovery 3, but only as a factory supplied option and at a cost of £2250. Strange really as this touch screen controlled rear entertainment system has been available since 2005 on both Range Rover and Sport models. Although Land Rover claims this cannot be retrofitted - it can! The following is a guide to the parts required and how I went about fitting them but should you wish to attempt this you do so at your own risk - the information contained in this document is for reference purposes only. Parts List: Pair of Headrests with OEM monitors installed including cables in LH stems. RSE Module – YIL000053 / LR011330 DVD 6 Disc Changer – Region Specific so many part numbers! AVIO Panel (Optional) - XVN500040 DVD Remote Control (Optional) – YUH50060 DVD Mounting Bracket – YIP500430 DVD Retainer Bracket – YIP500420 RSE Mounting Bracket – XQU500180 Cabling List: 13 Pin to 13 Pin Alpine Cable Black (RSE to DVD) 13 Pin to 13 Pin Alpine Cable Blue (RSE to AVIO) 20 Pin Mitsumi to 13 Pin Alpine Cable (RSE to LH Headrest Monitor) 20 Pin Mitsumi to 13 Pin Alpine Cable (RSE to RH Headrest Monitor) M.O.S.T Fibre Optic Extension Cable 4 Pin SVideo Cable for video signal out (to touch screen) and, if fitted, video in from TV tuner 8 Pin BlackDISCO3.CO.UK Connector for RSE Power & Earth 4 Pin White Connector for DVD Power & Earth SPDIF (Toslink) Fibre Optic Cable for DVD audio to Logic 7 Amp under front RH seat.
    [Show full text]
  • Rock Album Discography Last Up-Date: September 27Th, 2021
    Rock Album Discography Last up-date: September 27th, 2021 Rock Album Discography “Music was my first love, and it will be my last” was the first line of the virteous song “Music” on the album “Rebel”, which was produced by Alan Parson, sung by John Miles, and released I n 1976. From my point of view, there is no other citation, which more properly expresses the emotional impact of music to human beings. People come and go, but music remains forever, since acoustic waves are not bound to matter like monuments, paintings, or sculptures. In contrast, music as sound in general is transmitted by matter vibrations and can be reproduced independent of space and time. In this way, music is able to connect humans from the earliest high cultures to people of our present societies all over the world. Music is indeed a universal language and likely not restricted to our planetary society. The importance of music to the human society is also underlined by the Voyager mission: Both Voyager spacecrafts, which were launched at August 20th and September 05th, 1977, are bound for the stars, now, after their visits to the outer planets of our solar system (mission status: https://voyager.jpl.nasa.gov/mission/status/). They carry a gold- plated copper phonograph record, which comprises 90 minutes of music selected from all cultures next to sounds, spoken messages, and images from our planet Earth. There is rather little hope that any extraterrestrial form of life will ever come along the Voyager spacecrafts. But if this is yet going to happen they are likely able to understand the sound of music from these records at least.
    [Show full text]