DocumentCode
3036617
Title
Scalability of wavelength division multiplexed optical passive star networks with range limited tunable transceivers
Author
Pavan, Allalaghatta ; Cao, Feng ; Du, David H C
Author_Institution
Minnesota Univ., Minneapolis, MN, USA
fYear
1998
fDate
16-18 Feb 1998
Firstpage
86
Lastpage
93
Abstract
The size of an optical passive star and the wavelength range of tunable optical transceivers is limited by current technology. Scalability of passive star networks built with these two limitations is thus an important issue for building large networks. Previously, Cao, Du and Pavan (see Technical Report, Department of Computer Science, University of Minnesota, 1996) explored the design issues for single star networks employing transceivers with limited tuning range. Here we extend that study by considering the problem of connecting several optical passive stars, each embedded with a given virtual topology, to create larger aggregate networks. The design issues are analyzed and a number of design rules are proposed for building such aggregate networks. We consider the most commonly employed virtual topologies-complete graph, mesh and hypercube
Keywords
graph theory; hypercube networks; network topology; optical fibre networks; transceivers; wavelength division multiplexing; WDM; aggregate networks; complete graph; design rules; hypercube; mesh; optical passive star networks; optical transceivers; range limited tunable transceivers; scalability; virtual topology; wavelength division multiplexing; wavelength range; Aggregates; Buildings; Computer science; Joining processes; Optical fiber networks; Optical tuning; Scalability; Transceivers; Wavelength division multiplexing; Writing;
fLanguage
English
Publisher
ieee
Conference_Titel
Performance, Computing and Communications, 1998. IPCCC '98., IEEE International
Conference_Location
Tempe/Phoenix, AZ
ISSN
1097-2641
Print_ISBN
0-7803-4468-5
Type
conf
DOI
10.1109/PCCC.1998.659911
Filename
659911
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