• KSII Transactions on Internet and Information Systems (TIIS)
• /
• 제10권10호
• /
• pp.4661-4680
• /
• 2016

Cognitive radio (CR) technology is an effective solution to the spectrum scarcity issue. Collaborative spectrum sensing is known as a promising technique to improve the performance of spectrum sensing in cognitive radio networks (CRNs). However, collaborative spectrum sensing is vulnerable to spectrum data falsification (SSDF) attack, where malicious users (MUs) may send false sensing data to mislead other secondary users (SUs) to make an incorrect decision about primary user (PUs) activity, which is one of the key adversaries to the performance of CRNs. In this paper, we propose a coalition based malicious users detection (CMD) algorithm to detect the malicious user in CRNs. The proposed CMD algorithm can efficiently detect MUs base on the Geary'C theory and be modeled as a coalition formation game. Specifically, SSDF attack is one of the key issues to affect the resource allocation process. Focusing on the security issues, in this paper, we analyze the power allocation problem with MUs, and propose MUs detection based power allocation (MPA) algorithm. The MPA algorithm is divided into two steps: the MUs detection step and the optimal power allocation step. Firstly, in the MUs detection step, by the CMD algorithm we can obtain the MUs detection probability and the energy consumption of MUs detection. Secondly, in the optimal power allocation step, we use the Lagrange dual decomposition method to obtain the optimal transmission power of each SU and achieve the maximum utility of the whole CRN. Numerical simulation results show that the proposed CMD and MPA scheme can achieve a considerable performance improvement in MUs detection and power allocation.

• Journal of Astronomy and Space Sciences
• /
• 제31권2호
• /
• pp.121-130
• /
• 2014

Essential ideas, successes, and difficulties of Areal Density Analysis (ADA) for color-magnitude diagrams (CMD's) of resolved stellar populations are examined, with explanation of various algorithms and strategies for optimal performance. A CMD-generation program computes theoretical datasets with simulated observational error and a solution program inverts the problem by the method of Differential Corrections (DC) so as to compute parameter values from observed magnitudes and colors, with standard error estimates and correlation coefficients. ADA promises not only impersonal results, but also significant saving of labor, especially where a given dataset is analyzed with several evolution models. Observational errors and multiple star systems, along with various single star characteristics and phenomena, are modeled directly via the Functional Statistics Algorithm (FSA). Unlike Monte Carlo, FSA is not dependent on a random number generator. Discussions include difficulties and overall requirements, such as need for fast evolutionary computation and realization of goals within machine memory limits. Degradation of results due to influence of pixelization on derivatives, Initial Mass Function (IMF) quantization, IMF steepness, low Areal Densities ($\mathcal{A}$), and large variation in $\mathcal{A}$ are reduced or eliminated through a variety of schemes that are explained sufficiently for general application. The Levenberg-Marquardt and MMS algorithms for improvement of solution convergence are contained within the DC program. An example of convergence, which typically is very good, is shown in tabular form. A number of theoretical and practical solution issues are discussed, as are prospects for further development.

• ETRI Journal
• /
• 제37권6호
• /
• pp.1065-1076
• /
• 2015

Network densification is regarded as the dominant driver for wireless evolution into the era of 5G. However, in this context, interference-limited dense small cell deployments are facing technical challenges in mobility management. The recently announced results from an LTE field test conducted in a dense urban area show a handover failure (HOF) rate of over 21%. A major cause of HOFs is the transmission failure of handover command (HO CMD) messages. In this paper, we propose two enhancements to HO performance in LTE networks - radio link failure-proactive HO, which helps with the reliable transmission of HO CMD messages while the user equipment is under a poor radio link condition, and Early Handover Preparation with Ping-Pong Avoidance (EHOPPPA) HO, which assures reliable transmission of HO CMD under a good radio link condition. We analyze the HO performance of EHOPPPA HO theoretically, and perform simulations to compare the performance of the proposed schemes with that of standard LTE HO. We show that they can decrease the HOF rate to nearly zero through an analysis, and based on the simulation results, by over 70%, without increasing the ping-pong probability.

• Journal of Oral Medicine and Pain
• /
• 제18권1호
• /
• pp.31-43
• /
• 1993

To evaluate the correlationship between sign/symptoms of craniomandibular disorder(CMD) and possible contributing occlusal factors, the author analyzed craniomandibular index(CMI), clinical dysfunction index(CDI) and occlusal index(Oi) obtained from 88 subjects (32 males, 56 females, mean age 28.7) consisted of 49 CMD patients(15 males, 34 females, mean age 28.7) and 39 non-CMD patients (17 males, 22 females, mean age 24.5). The obtained results were as follows : 1. There was very high significant correlation bebween CMI and CDI in total subjects (r=0.83, p<0.01) 2. There was very low correlation between working-side interference and TMJ noise which was observed as a statistically significant value(p<0.05). And also there ws very low correlation between nonworking side interference and muscle tenderness, CDI, dysfunction index(DI), palpation index(PI) which were observed as statistically significant value (p<0.01) 3. There was very low correlation between as ymmetry of tetruded contact position(RCP)-intercuspal position(ICP) slide and muscle tenderness, TMJ tenderness, TMJ noise, CMI, DI, PI which were observed as statistically significant values(p<0.05) 4. In general there was low correlation between Oi and muscle tenderness, CDI, CMI, DI, PI which were observed as statistically significant values (p,0.05). But Oi had a relatively higher correlation with muscle tenderness, PI than whith CDI, DI.

• Journal of Oral Medicine and Pain
• /
• 제22권1호
• /
• pp.145-155
• /
• 1997

The purpose of this study was to compare differences in endurance time and EMG power spectral characteristics of the masticatory muscles during sustained isometric contraction between patients and controls. 15 CMD patients{8 women and 7 men, aged 15 to 38 years(24.1$\pm$7.5)}, and 15 healthy volunteers{8 women and 7 men, aged 15 to 30 years(24.7$\pm$3.4)} without past history or present symptoms of CMD were included in this study. Sustained isometric contractions of masticatory muscles were perfomeed as long as possible at 50% level of maximum voluntary contraction(MVC) of EMG activity via visual feedback, and the duration of sustained isometric contraction(endurance time) was examined. The author perfomed EMG power spectral analysis in the myoelectric signals of masseter and anterior temporal muscle during sustained isometric contraction in CMD patients with chronic muscle pain and healthy controls. The author came to following conclusions from the results. 1. The endurance time of the patient group was shorter than the control group in sustained isometric contraction of masticatory muscles(p<0.01). 2. MF values of masticatory muscles with sustained isometric contraction during endurance time were decreased following regression line in both groups(p<0.01, r>0.9). 3. The amount of MF shift to lower frequency range exhibited no significant differences between the patients and the control group in sustained isometric contraction during endurance time. 4. SMF to lower frequency range of the patient group was steeper than the control group in sustained isometric contraction during endurance time(p<0.05).

• 자원환경지질
• /
• 제56권2호
• /
• pp.125-138
• /
• 2023

수계 내 세슘(cesium: Cs)을 제거하기 위하여 개발된 대부분의 기존 Cs 흡착제들은 원재료 값이 고가라는 단점과, 해수와 같이 높은 이온 강도와 낮은 Cs 농도를 가지는 대규모의 오염수를 실질적으로 정화하는데 한계를 가지고 있었다. 본 연구에서는 석탄광산배수를 처리하는 과정에서 생성되는 슬러지(CMDS)에 Na와 S를 첨가하여 친환경적이고 높은 Cs 제거 효율을 가지는 Cs 흡착제를 개발하였다. Fe 및 Ca 함량이 풍부한 CMDS를 1차 소재로 사용하였고, 열처리 과정으로 Na와 S를 첨가하여 새로운 Cs 흡착제를 제조하였다(이하 본 연구에서 개발한 흡착제는 Na-S-CMDS라 명명함). Na-S-CMDS의 Cs 흡착능 및 흡착 기작을 평가하기 위해 실험실 규모의 실험과 흡착 동역학 및 등온 모델링 연구를 수행하였으며, XRF, XRD, SEM/EDS, XPS 등의 분석을 통해 Na-S-CMDS의 물리화학적, 광물학적 특성을 조사함으로써 Cs 흡착 기작을 규명하였다. 흡착 배치 실험 결과, Cs은 빠르게 Na-S-CMDS에 흡착되어 1시간 내 평형에 도달하였으며, 낮은 Cs 농도(0.5 mg/L) 조건에서도 높은 Cs 제거 효율(> 90.0%)을 보였다. 흡착 등온 모델링 결과, 단일 흡착을 가정하는 Langmuir 흡착 등온 모델에 대응되는 경향을 보였으며, 흡착 동역학 모델링 결과 흡착 경향이 유사 2차 속도(pseudo second order kinetic) 모델과 일치하는 경향을 보였고, 이러한 결과는 단순한 물리적 흡착보다 이온 교환과 같은 화학적 흡착이 우세함을 의미한다. 고농도의 Cs 용액으로 반응시킨 Na-S-CMDS의 XRF/XRD 분석 결과, Na-S-CMDS 내 Na 함량은 감소하고 흡착 전 존재하던 erdite (NaFeS₂·2(H₂O))가 관찰되지 않는 것을 통해, Na⁺과 Cs⁺ 사이에서 활발한 이온 교환 반응이 진행되었음을 알 수 있었다. XPS 분석 결과, Na-S-CMDS에서 Cs와 S 사이의 강한 결합 작용이 관찰되었으며, 이러한 Cs와 S(또는 S-복합체)내 결합에너지 감소도 Na-S-CMDS의 Cs 흡착능을 증가시키는 요인으로 판단되었다. 본 연구를 통해 기존에 폐기물로 처리되었던 석탄광산배수슬러지를 개량하여 제조한 Na-S-CMDS는 기존의 Cs 흡착제보다 제조 비용이 저렴하고, 해수 및 지하수와 같이 이온 강도는 높지만 Cs 농도가 낮은 대규모 오염 수계에서도 Cs 흡착능이 높게 유지되어, 현장에서 효과적인 Cs 흡착제로 사용할 수 있을 것으로 기대한다.

• 천문학회보
• /
• 제29권2호
• /
• pp.70.2-70.2
• /
• 2004

• Journal of Astronomy and Space Sciences
• /
• 제13권1호
• /
• pp.55-62
• /
• 1996

We present UBV CCD photomety of the metal-poor globular cluster M30. The data were obtained using the 40 inch telescope at Mt. Stromlo and Siding Spring Observatory (MSSSO). We used DAOPHOT CCD reduction package in order to obtain Color-Magnitude Diagram (CMD). We have derived some fundametal parameters of the globular cluster such as metal abundance ([Fe/H]), helium abundance (Y), and distance modulus (m-M) from the CMD. The derived parameters were [Fe/H]=-2.50, Y=0.28, and (m-M)=14.64. From the latter, the distance of 8.3kpc is obtained. Despite the photometric uncertainty near the main-sequence turnoff, we estimate the age of M30 to be 1.6${\pm}$3 Gyrs from the Revised Yale Isocyrones. If [O/Fe]=+0.4, this age will be reduced to 14.2${\pm}$3 Gyrs.

• 한국우주과학회:학술대회논문집(한국우주과학회보)
• /
• 한국우주과학회 1992년도 한국우주과학회보 제2권1호
• /
• pp.14.2-14
• /
• 1993

We present UBV CCD Photometry of the very metal-poor globular duster M3O,covering a region of r f 100 arcsec from the duster center. The data was obtained from the 40 inch telescope at Mt Soomlo Siding Spring Observator in August 1992. We used DAOPHOT CCD reudction package for data reduction to obtain Color-Magnitude Diagram(CMD). We have determined some fludamental parameters of the globular Ouster such as metal abundance, helium abundance and distance from the CMD. finally, we have attempted to determine the age of M3O using the revised Yale isochrones.

• 천문학회지
• /
• 제31권1호
• /
• pp.67-74
• /
• 1998

The VI CCD photometry is made for stars in the globular cluster M22 down to $V\approx19^m,\;I\approx18^m$. In the color-magnitude diagram (CMD), red giant branch (RGB), asymtotic giant branch (AGB) and blue horizontal branch (BHB) are well defined. The luminosity functions (LF) of RGB, AGB and BHB stars are derived, discussing deficient gaps and bumps in the CMD. The anomalously wide RGB seen in the BV photometric system is found to disappear in the VI photometric system.