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14th Workshop COST289 – April 11th 2007
D-STAR MAC Protocol: a Cross Layer D-STAR MAC Protocol: a Cross Layer
Solution for Wireless Sensor Networks Solution for Wireless Sensor Networks
Endowed with Directive AntennasEndowed with Directive Antennas
Gianfranco Manes, Romano Fantacci, Francesco Chiti, Michele Ciabatti, Giovanni Collodi, Davide Di Palma, Ilaria Nelli, and Antonio
Manes
Department of Electronics and Telecommunications
University of Florence
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24th Workshop COST289 – April 11th 2007
OutlineOutline
1. Motivations WSNs
Directive antennas
2. Proposed protocol Discovery phase
Regime phase
3. Performance analysis
4. Conclusions
Outline Outline
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34th Workshop COST289 – April 11th 2007
Wireless Sensor NetworkingWireless Sensor Networking
Enabling technology to the aim of intelligent environments instrumenting
Affordable solution to some challenging problems: environmental sensing, productive chains control, real-time phenomena monitoring, safety and rescue application.
WSNs represent a special case of the more general wireless Ad Hoc networking paradigm with additional constraints: limited energetic, storage, processing and communication
capabilities low degree of mobility presence of a small number of sinks
1. Motivations 1. Motivations
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44th Workshop COST289 – April 11th 2007
Wireless Sensor NetworkingWireless Sensor Networking
This challenge might be got over through careful system design with particular regard to the communications protocols:
MAC layer:
management of both sleep and active power states
PHY layer:
introduction of directional antennas and their integration within the communications framework
1. Motivations 1. Motivations
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54th Workshop COST289 – April 11th 2007
Directive AntennasDirective Antennas
Expected benefits Antenna gain maximization towards desired directions,
concentrating energy in smaller area:
Transmitted power decreasing
Power consumption reduction
Network life time increasing
Received power increasing
Coverage range increasing
Error probability reduction
1. Motivations 1. Motivations
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64th Workshop COST289 – April 11th 2007
Directive AntennasDirective Antennas
Expected benefits Radiation towards undesired directions minimization
Interference caused by other transmissions reduction
Co-channel interference mitigation
multiple-access problems mitigation
Collision probability reduction
Adaptability to time varying communication conditions: Mote’s failure
Channel errors
Congestion
1. Motivations 1. Motivations
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74th Workshop COST289 – April 11th 2007
Directive AntennasDirective Antennas
Criticalities Cost and size
On board integration
Beam switching management: Set-up phase signaling overhead
Latency for end-to-end communications setting-up
Algorithm complexity
Switching agility
Support both to synchronous (source-initiated) and asynchronous (event-based) sensing
1. Motivations 1. Motivations
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84th Workshop COST289 – April 11th 2007
Directive-Synchronous Transmission Directive-Synchronous Transmission Asynchronous Reception (D-STAR)Asynchronous Reception (D-STAR)
STAR MAC concept for time synchronization [Chiti et al. in Proc. of IEEE ICC’06]
Cross-layer protocol design (MAC+PHY) Space-time synchronization Suitable for flat topology Scalable
2. Proposal2. Proposal
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94th Workshop COST289 – April 11th 2007
Directive-Synchronous Transmission Directive-Synchronous Transmission Asynchronous Reception (D-STAR)Asynchronous Reception (D-STAR)
Hypothesis
Beam width = θ [rad]
N possible angular sectors:
N = 2π/θ
Quasi ideal switching
Tswitch << Tpkt
2. Proposal2. Proposal
θ = π/2 [rad]
N = 4
Tswitch ≈ μs << Tpkt ≈ ms
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104th Workshop COST289 – April 11th 2007
D-STAR: State DiagramD-STAR: State Diagram
DISCOVERY
1 < EmptySectors < Ns
Emptysectors = Ns
Switch on
nf < Nfd
Battery < Battery_low
REGIME
Battery < Battery_low
nf=Nfd
INIT
OFF
2. Proposal2. Proposal
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114th Workshop COST289 – April 11th 2007
D-STAR: Discovery phaseD-STAR: Discovery phase
1. Duty cycle δ = 100% Listening mode for a time interval Tset-up
Beacon (HELLO) broadcasting: 1 beacon angular sector Node ID and Phase (φ) transmission (time to the next awakening)
Waiting for a fixed time duration τs in search of reply messages Switching to the following angular sector
Exit condition: (Tset-up is expired, i.e., Nfd frame periods)
2. Proposal2. Proposal
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124th Workshop COST289 – April 11th 2007
D-STAR: Discovery phaseD-STAR: Discovery phase
2. Proposal2. Proposal
δ = 100%
Tset-up
time
HELLO HELLO HELLO HELLO
HELLO
…
HELLO
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134th Workshop COST289 – April 11th 2007
D-STAR: Regime phaseD-STAR: Regime phase
Each node sends: HELLO messages to known neighbors belonging to different angular
sectors according to the phase transmitted in previous HELLO messages, several HELLO messages in background with the proper period to unknown
neighbors in the empty angular sector.
Upon the replying of a node, a logical channel is established: The channel access is managed by means of a CSMA/CA (Carrier Sense
Multiple Access with Collision Avoidance) approach.
Each node remains in the regime phase until there is at least one neighbor, otherwise if the number of empty angular sector is equal to Ns it re-enters the discovery phase in search of connectivity.
2. Proposal2. Proposal
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144th Workshop COST289 – April 11th 2007
D-STAR: Regime phaseD-STAR: Regime phase
2. Proposal2. Proposal
Tf
time
listening sleep
δ Tf
HELLO HELLO HELLO
…
HELLO + FWD
…
HELLO * FWD
HELLO
…HELLO HELLO
1 HELLO broadcasting
per sector
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154th Workshop COST289 – April 11th 2007
Operative hypothesisOperative hypothesis
FP6-IST-1-508744-IP ‘‘GoodFood’’ reference scenario Monitored area = 25 ∙ 25 [m2] Number of WSN nodes: [10…50] N = 1, 2 ,4, 6, 8 angular sectors HELLO pkt length = 8 bytes Bit rate = 250 kbps Packet Error Rate = 5% Number of channel sensing for CSMAC/CA algorithm = 6 Frame period: 10,25,50,75,93 s Duty-cycle: [1…5]%
3. Performance3. Performance
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164th Workshop COST289 – April 11th 2007
Università degli Studi di Firenze
Normalized Lifetime Gain (Tf=93 s d=3%)
0
5
10
15
20
25
10 15 20 25 30 35 40 45 50
Number of nodes
No
rma
lize
d L
ife
tim
e G
ain
omni
N=2/omni
N=4/omni
N=6/omni
N=8/omni
3. Performance3. Performance
Network lifetime vs nodesNetwork lifetime vs nodes
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174th Workshop COST289 – April 11th 2007
Normalized Lifetime Gain (Tf=93 s; 50 nodes)
0
5
10
15
20
25
0,01 0,02 0,03 0,04 0,05
Dutycycle
No
rma
lize
d L
ife
tim
e G
ain
omni
N=2/omni
N=4/omni
N=6/omni
N=8/omni
Network lifetime vs duty-cycleNetwork lifetime vs duty-cycle
3. Performance3. Performance
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184th Workshop COST289 – April 11th 2007
Normalized Lifetime Gain (d=3%; 50 nodes)
0
5
10
15
20
25
30
35
10 20 30 40 50 60 70 80 90
Frame period [s]
No
rma
lize
d L
ife
tim
e G
ain
omni
N=2/omni
N=4/omni
N=6/omni
N=8/omni
Network lifetime vs frame periodNetwork lifetime vs frame period
3. Performance3. Performance
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194th Workshop COST289 – April 11th 2007
Occupied Channel Probability (Tf=93s; d=3%)
0
0,01
0,02
0,03
0,04
0,05
0,06
10 15 20 25 30 35 40 45 50
omni
N=2
N=4
N=6
N=8
Number of nodes
Occ
up
ied
Ch
ann
el P
rob
abil
ity
Collision Probability (Tf=93 s; d=3%)
0
0,005
0,01
0,015
0,02
0,025
10 15 20 25 30 35 40 45 50
omni
N=2
N=4
N=6
N=8
Number of nodes
Co
llis
ion
Pro
bab
ilit
y
SS'
R
S S'
RR'
Hidden node analysisHidden node analysis
3. Performance3. Performance
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204th Workshop COST289 – April 11th 2007
Normalized Throughput (Tf=93 s; d=3%)
0,92
0,93
0,94
0,95
0,96
0,97
0,98
0,99
1
10 15 20 25 30 35 40 45 50
omni
N=2
N=4
N=6
N=8
Number of nodes
No
rma
lize
d T
hro
ug
hp
ut
Signaling Overhead (Tf=93 s; d=3%)
0
500
1000
1500
2000
2500
10 15 20 25 30 35 40 45 50
omni
N=2
N=4
N=6
N=8
Number of nodes
Ov
erh
ea
d [
pk
t/T
f]Signaling Overhead
Resource Utilization
Efficiency and complexityEfficiency and complexity
3. Performance3. Performance
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214th Workshop COST289 – April 11th 2007
ConclusionsConclusions
Energy efficient WSN protocol design Cross-layer approach (MAC+PHY) Performance:
Energetic consumption Lifetime Latency Collision probability Signaling overhead
Good tradeoff Easy to implement
4. Conclusions4. Conclusions