• 한국멀티미디어학회논문지
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• 제8권6호
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• pp.836-843
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• 2005

The Wireless Internet services widely spread out with the developments of CDMA(Code Division Multiple Access) networks and wireless units. In contrast to the telecommunication network, WPAN (Wireless Personal Area Network) enables to transmit data and voice in personal area. Although WPAN technologies are commercially utilized, the combined services with COMA network are not so poplar up to now. Various services can be provided using the combination between COMA and WPAN. This paper presents the practical and united model between COMA and WPAN. Specially, the main focus of this research lies on the design of the Middle-ware system of a handset which could be managing both COMA and WPAN. This system used Bluethooth by WPAN. For the devices with the proposed WPAN Middle-ware, service areas of the COMA network can be expanded to WPAN, various services can be realized by the transmission of data and voice, and consequently, the user computing environment could be improved.

• 천문학회보
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• 제43권1호
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• pp.72.3-72.3
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• 2018

Since there are two-different observational constraints for the lunar exosphere data, it is interesting to find the best exospheric model that can account for the observed characteristics of the lunar coma and tail simultaneously (Lee & Kim, 2017).The characteristics of the lunar exosphere can be constrained by comparing simulated models with observational data of the coma and tail. In this work, considering effects of triple sodium sources (two dayside sources: a low- and a high-velocity component; and an Isotropic source component), we present time-dependent simulations showing initial conditions around the lunar coma and the final stage of the lunar tail. Based on an updated 3-D lunar exosphere model (Lee & Kim, 2017), we are presenting the simulated images of the lunar sodium coma and its correlation with lunar tail's physical parameters.

• The Korean Journal of Pain
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• 제19권2호
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• pp.213-217
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• 2006

Although various treatments for complex regional pain syndrome (CRPS) have been proposed, no well recognized treatment for CRPS has been established. Herein, a case using barbiturate coma therapy for the refractory pain management of a 24-year-old male patient, who suffered from constant stabbing and burning pain, with severe touch allodynia in the left upper extremity following blunt trauma on his forearm is described. Interventional treatments, including permanent spinal cord stimulation and large doses of oral medications, were performed. However, the pain could not be controlled, which lead to frequent emergency room treatment for about 1 month prior to his therapy. He then underwent barbiturate coma therapy due to the uncontrollable pain, with repeated sedation therapy due to his outrageous behavior. His pain became increasingly tolerable and the allodynia was markedly decreased after 5 days of coma therapy.

• 천문학회보
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• 제46권2호
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• pp.41.3-42
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• 2021

Coma cluster (Abell 1656) is one of the most massive local galaxy clusters such as Virgo, Fornax, and Perseus, which holds a large collection of globular clusters. Globular cluster systems (GCSs) in a galaxy cluster tell us a history of hierarchical cluster assembly and intracluster GCs (ICGCs) are known to trace the gravitational potential of the galaxy cluster. Previous studies of GCSs in Coma mainly utilized data obtained using Hubble Space Telescope (HST) with high spatial resolution. However, most of the data were based on narrow-field pointing observations. In this study we present the widest survey of GCSs in the Coma cluster using the archival Subaru/Hyper Suprime-Cam (HSC) g and r images, supplemented with the archival HST images. The Coma GCSs are largely extended in E-W and SW direction, along the general direction of Coma-Abell 1367 filament. This global structure of the GCSs is consistent with the spatial distribution of the intracluster light (ICL). ICGC spatial distribution is largely extended to almost ~50% of the virial radius. Most of these ICGCs are blue and metal-poor, which supports the scenario that ICGCs are mainly originated from dwarf galaxies and some proportion from brighter galaxies. Implications of the results will be discussed.

• Clinical and Experimental Pediatrics
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• 제53권4호
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• pp.598-602
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• 2010

신생아 일과성 고암모니아혈증은 고암모니아혈증을 특징으로 하며 대부분 호흡곤란 치료를 받는 미숙아에서 발생한다. 발생원인은 정확히 알려져 있지 않으나 생후 2-3일에 호흡 곤란, 기면, 경련, 혼수 등의 임상 증상을 보이고, 생화학적 검사 상 혈중암모니아 농도가 현저히 증가하며 요소회로 효소 치는 정상을 보인다. 치료가 늦으면 사망에 이르는 응급을 요하는 질환이나 즉각적이고 적절한 치료 시 신경학적 손상을 남기지 않고 호전 가능하다. 저자들은 호흡곤란을 보여 호흡기 치료를 받던 35주 미숙아에서 48시간 내에 경련과 함께 혼수상태에 빠지고 검사상 고암모니아혈증을 보여 신투석 등의 치료 후 회복되었으며 2년 추적관찰에서 정상을 보인 환아를 보고하는 바이다.

• 한국통신학회논문지
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• 제21권3호
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• pp.713-720
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• 1996

최근에 이동 통신의 수요가 급속히 증가하는 반면에 무선자원은 제한되어 있으므로 이를 효율적으로 이용할 수 있는 적합한 프로토콜이 요구되고 있다. 기존에 연구된 CDMA_ALOHA 기법중에 MS_CDMA_ALOHA(Mini Slotted CDMA_ALOHA) 방식이 S_COMA_ALOHA(Slotted COMA_ALOHA)보다 성능이 우수한 것으로 나타났다. 또한 CDMA 디지탈 셀룰러 시스템의 CAI 프로토콜로서 IS-95 다중 엑세스 방식이 제안되었다. 하지만 기존의 연구에서는 무선통신 환경의 채널특성을 고려한 성능분석이 이루어지지 않았다. 본 논문에서는 DS/CDMA 셀룰러 환경에서 성능개선을 위한 새로운 기법을 제시하였으며, 이는 기존의 MS_ COMA_ALOHA 방식을 기반으로 한 것으로서 채널상태에 적용할 수 있는 기법이다. 또한 컴퓨터 시뮬레이션을 통하여 기존의 방식과 비교 분석 하였다. 그 결과 새로 제안한 NA_COMA_ALOHA(Noise Adaptation COMA ALOHA) 방식은 기존의 COMA_ALOHA 방식보다 시스템 처리율 및 평균 지연특성면에서 우수한 성능을 보였다. 이는 NA_COMA_ALOHA 방식이 시스템의 과부하 환경에서 채널상태에 따라 사용자의 액세스 시도를 제어 하기 때문이다.

• 대한간호
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• 제16권6호통권92호
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• pp.81-88
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• 1977

• 천문학회지
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• 제28권1호
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• pp.15-30
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• 1995

A velocity inhomogeneity, which is defined as a regional preponderence of either radial or tangential orbits, is searched with a new technique for the Coma cluster of galaxies. It is found within $\~2h^{-1}$ Mpc from the cluster center that the Coma shows conspicuous inhomogeneities in velocity and that the inhomogeneities are real at a $99\%$ level of confidence. Even in the central region (7' - 30' from the center), zones that are dominated by radial and tangential orbits are distinguishable. Defining the cluster's 'equator' as the direction defined by the Coma-A1367 supercluster, tangential orbits dominate the 'polar' zones in the central region. Galaxies that are located in 30'-100' also inhomogeneous in velocity in that the 'polar' zones are mostly radial while the rest is nearly homogeneous. These results indicate that the Coma galaxies are exceedingly more radial in orbit, implying that merging or infalls are either still going on or an earlier virialization is likely to have occurred preferentially near the 'equator'. Incorporating the velocity inhomogeneity into mass estimators, the most appropriate mass is turned out to be $0.4\times10^{15}h^{-1}M_\bigodot(R\;\leq\;0.6h^{-1} Mpc),\;and\;1.0\times10^{15}h^{-1} M_\bigodot(R\;\leq\;2.1h^{-1}Mpc)$. The corresponding mass to blue light ratio on the average is $\~$300h. These estimates are consistent with Merritt (1987) and Hughes (1989) and the MILE is seemed to favour the mass-follows-light models than the uniform spread of dark matter throughout the cluster.

• 한국콘텐츠학회:학술대회논문집
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• 한국콘텐츠학회 2012년도 춘계 종합학술대회 논문집
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• pp.343-344
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• 2012

본 연구는 중증도가 높은 신경계중환자를 대상으로 중환자 중증도 분류도구와 Glasgow coma scale 적용의 유용성을 검정하고자 하는데 있다. 본 연구에서 대상자의 일반적 특성 및 임상 관련 특성에 따른 사망률 확인, 중환자 중증도 분류도구(CPSCS)의 일반적 특성, 임상관련 특성에 따른 중증도 차이, GCS의 일반적 특성과 임상관련 특성에 따른 중증도 차이를 파악하고, 임상적 유용성을 검정하고자 한다.

• 한국정보과학회:학술대회논문집
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• 한국정보과학회 2003년도 봄 학술발표논문집 Vol.30 No.1 (C)
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• pp.262-264
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• 2003

본 논문에서는 광역 및 근거리 우선 접속을 지원하는 PDA상에서 각 무선접속들 간의 상호 연동 및 핸드오프 방안을 설계하고 제시한다. 즉, 근거리 망인 블루투스와 광역 망인 COMA간의 연동 및 핸드오프 방식을 설계 제안하며 이동성과 연결성을 보장한다. 또한 홈 네트워크 상에서 홈 서버와 PDA간의 상호연동 접속 및 핸드오프 방안을 적용하고 테스트한다.