scholarly journals Evaluation of a Large-Scale Topology Discovery Algorithm

Author(s):  
Benoit Donnet ◽  
Bradley Huffaker ◽  
Timur Friedman ◽  
kc claffy
2020 ◽  
Vol 13 (5) ◽  
pp. 1720-1743 ◽  
Author(s):  
Haojun Teng ◽  
Kaoru Ota ◽  
Anfeng Liu ◽  
Tian Wang ◽  
Shaobo Zhang

2013 ◽  
Vol 13 (3) ◽  
pp. 05-12
Author(s):  
Ranjit Nukathati ◽  

2006 ◽  
Vol 24 (12) ◽  
pp. 2210-2220 ◽  
Author(s):  
B. Donnet ◽  
P. Raoult ◽  
T. Friedman ◽  
M. Crovella

2005 ◽  
Vol 33 (1) ◽  
pp. 327-338 ◽  
Author(s):  
Benoit Donnet ◽  
Philippe Raoult ◽  
Timur Friedman ◽  
Mark Crovella

2018 ◽  
Vol 14 (5) ◽  
pp. 2261-2270 ◽  
Author(s):  
Tianqi Yu ◽  
Xianbin Wang ◽  
Jiong Jin ◽  
Kenneth McIsaac

2020 ◽  
Vol 16 (11) ◽  
pp. 155014772097452
Author(s):  
Liao Wenxing ◽  
Shi Xiaofei ◽  
Chen Xinying

In wireless multi-hop networks, especially large-scale wireless multi-hop networks, obtaining the network topology is of vital significance. In fact, in both proactive and reactive routing protocols, before establishing an appropriate end-to-end route, the source node needs to obtain the global or local topology. Our previous research has studied the impacts of weak links on reactive routing protocols, which can also be considered as local topology discovery process. In this article, in order to get insight of the impacts of weak links on topology discovery process, especially the global topology discovery on which the proactive routing protocols rely, we apply a Markov chain to model the most common used topology discovery process in large-scale wireless multi-hop networks. Considering the fading characteristics of wireless channel, we analyze the impacts of weak links on topology discovery algorithms. Simulation and theoretical results show that, with the increase in the network scale, the weak links have great impacts on the stability and even on the feasibility of wireless multi-hop networks.


1999 ◽  
Vol 173 ◽  
pp. 243-248
Author(s):  
D. Kubáček ◽  
A. Galád ◽  
A. Pravda

AbstractUnusual short-period comet 29P/Schwassmann-Wachmann 1 inspired many observers to explain its unpredictable outbursts. In this paper large scale structures and features from the inner part of the coma in time periods around outbursts are studied. CCD images were taken at Whipple Observatory, Mt. Hopkins, in 1989 and at Astronomical Observatory, Modra, from 1995 to 1998. Photographic plates of the comet were taken at Harvard College Observatory, Oak Ridge, from 1974 to 1982. The latter were digitized at first to apply the same techniques of image processing for optimizing the visibility of features in the coma during outbursts. Outbursts and coma structures show various shapes.


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