• Title/Summary/Keyword: levy

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Performance Evaluation of AODV and OLSR Routing Protocol According to Node's Mobility Model (노드 이동성 모델에 따른 AODV와 OLSR 라우팅 프로토콜의 성능 분석)

  • Kang, Mi-Seon;Kum, Dong-Won;Cho, You-Ze
    • The Journal of Korean Institute of Communications and Information Sciences
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    • v.36 no.7A
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    • pp.662-668
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    • 2011
  • This paper analyzes the performance of the Ad hoc On-demand Distance Vector (AODV) routing protocol and Optimized Link State Routing (OLSR) for Mobile Ad hoc Networks (MANETs) using node mobility models. Mobility affects the performance of a routing protocol as it causes changes to network topology. Thus, evaluating the performance of a MANET routing protocol requires mobility models that can accurately represent the movements of mobile nodes. Therefore, this paper evaluates the performance of the AODV and OLSR routing protocols using the random way point model and the Levy walk model by the ns-2 simulations.

Computerization, Occupational Choice and Job Polarization in the Korea Labor Market (컴퓨터화, 직업선택, 그리고 한국 노동시장에서의 고용의 양극화)

  • Kim, Sung-min
    • Journal of Labour Economics
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    • v.35 no.1
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    • pp.21-54
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    • 2012
  • This paper investigates how technological change and the consequential occupational choices do influence the recent Korea labor market. Following Autor, Levy and Murnane (2003) and Autor, Katz and Kearney (2006), it shows that decreasing price of computer assets raises relative wages for nonroutine tasks and the self-selected occupational choices with increasing demands for computerization in routine tasks would be a main cause for the job polarization in the labor market.

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OBSERVATION OF IMPACT SITES OF SHOEMAKER-LEVY 9 COMET (슈메이커-레비 9 혜성의 목성 충돌관측)

  • Lee, Si-Woo;Kim, Seung-Ri;Seong, Hwan-Gyeong;Pyo, Tae-Su
    • Publications of The Korean Astronomical Society
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    • v.10 no.1
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    • pp.1-14
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    • 1995
  • We observed impact spots on Jupiter which were formed by the collision with fragments of Shoemaker-Levy 9 comet during the period from 17 July to 13 August, by using the SNU 61cm reflector combined with CCD camera and DBVRI filters. In order to get more clear image of impact spots, the observed data were processed by the unsharp masking method, high-pass filtering method and Richardson-Lucy algorithm after the basic processing through IRAF package. The sizes of impact spots range from 2000km to 1000km, and from this size, the original size of comet fragments before collision with Jupiter is estimated to be less than ${\sim}3km$. From the observed rotating rate of impact spots, the rotational period of Jupiter is determined as $9^h$ $56^m$ $32^s$ at the southern latitude of $47^{\circ}{\sim}49^{\circ}$.

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