Power Consumption Analysis of Sensor Node According to Beacon Signal Interval in IEEE 802.15.4 Wireless Star Sensor Network 


Vol. 31,  No. 9, pp. 811-820, Sep.  2006


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  Abstract

In this paper, The correlation of the power consumption of sensor node is analyzed according to the analyze parameter in IEEE 802.15.4 star sensor network. And It is studied the influence on analysis parameter. The power consumption of sensor network in transmission process and average transmission power consumption drives to numerical formula. And CSEM WiseNET system measurement value is used. As a simulation result, The power consumption of sensor node in star network consist of 10 sensor nodes is more than 20 % that in single network in average. When beacon signal interval is 0.1 second in all frequency bands, the power consumption of sensor node in up-link is more than 2.5 times that in down-link in average. When beacon signal interval is 1 second and the number of sensor nodes increases to 100 and sensing data increases to 100 byte, the power consumption of sensor node increases to 2.3 times. And The superior performance of 2.4 ㎓ frequency band has than 868/915 ㎒ frequency band up to 6∼12 times.

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  Cite this article

[IEEE Style]

Y. Yoo, J. Choi, N. Kim, "Power Consumption Analysis of Sensor Node According to Beacon Signal Interval in IEEE 802.15.4 Wireless Star Sensor Network," The Journal of Korean Institute of Communications and Information Sciences, vol. 31, no. 9, pp. 811-820, 2006. DOI: .

[ACM Style]

Young-dae Yoo, Jung-hun Choi, and Nam Kim. 2006. Power Consumption Analysis of Sensor Node According to Beacon Signal Interval in IEEE 802.15.4 Wireless Star Sensor Network. The Journal of Korean Institute of Communications and Information Sciences, 31, 9, (2006), 811-820. DOI: .

[KICS Style]

Young-dae Yoo, Jung-hun Choi, Nam Kim, "Power Consumption Analysis of Sensor Node According to Beacon Signal Interval in IEEE 802.15.4 Wireless Star Sensor Network," The Journal of Korean Institute of Communications and Information Sciences, vol. 31, no. 9, pp. 811-820, 9. 2006.

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pISSN : 1226 - 4717
eISSN : 2287 - 3880