• The Journal of Korean Institute of Electromagnetic Engineering and Science
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• v.13 no.8
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• pp.811-818
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• 2002

In this paper, a shorting pin and slot-loaded microstrip patch antenna is designed and fabricated. A shorting pin and slots are used for harmonic suppression on an inset fed antenna. A shorting pin and slot properties are analyzed by cavity model of the rectangular patch and the characteristics of the designed antenna are described. The designed antenna provides a gain of 7 dBi at the fundamental frequency, 5.8 GHz. In the second and third harmonic frequencies, the proposed antenna has gain suppression properties of -3.3 dB and -14.3 dB at each harmonic frequency, respectively.

• Standardization Trend in Telecommunications
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• s.24
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• pp.224-232
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• 1992

페이징 시스템의 발달과 시행은 오늘날 특정 영역 내에서의 진보가 다른 영역의 균형있는 발전에 얼마나 많이 의존하고 있는가를 보여주는 전형적인 예이다. 과거의 페이징 시스템은 한 공장의 근로자에게 혜택을 주었다. 위성을 이용하는 미래의 페이징 시스템은 전세계 모든 곳의 모든 사람에게 다양한 혜택을 제공해 줄 수 있게 된다. 점진적으로, 한 쌍의 킬로미터와 점선으로 연결된 전구와 벨은 처음으로 무선시스템으로 대체되어 한 국가라는 지역을 넘어서 서비스를 제공해 왔다. 디지털 기술의 개발을 포함해서, 무선 설비가 소형화 됨에 따라 이러한 일은 점차적으로 이루어져 왔다. 따라서 전기통신에 의한 우주 무선통신과 특히 정지위성 시스템의 엄청난 발전으로 전세계는 가까워지게 되었지만 거의 엄청난 비용과 이용자들이 갖춰야할 것들 때문에 이러한 영역에 접근하는 것은 거의 한정되어 방송용으로만 준비되어 왔다. 오랫동안 LEO 위성은 과학적, 군사적인 용도로만 이용되어 왔는데 그것은 이 위성이 원래 가지고 있는 문제점들로 하루마다 지평선 위의 아주 짧은 통행로와 관계된 것 때문이었다. 그러나 현재는 하나의 시스템을 형성하기 위해 수많은 LEO 위성들의 발사를 감당해 낼 수 있는 장치와 여러 영역에서의 공동작용(synergy) 덕분에, VHF대의 아주 저렴한 시설을 이용한 경제적, 기술적 장점을 인식하고, 혼신을 다하여 다이내믹 채널 활동지점 시스템(denamic channel activity assignment system)을 개발하였고, 마지막으로 말하지만 결코 가볍게 인식해서는 안될 WARC-92가 필요한 주파수대를 지정해야한다는 의도를 밝힌 것 등이 개인간의 통신을 전세계적으로 확대하는데 있어서 디딤돌이 될 것이다.

• Proceedings of the Korean Institute of Navigation and Port Research Conference
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• 2013.06a
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• pp.130-131
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• 2013

캐비테이션 현상은 고 유속 환경에서 발생(inception), 성장(growth), 붕괴(collapse) 및 소멸(disappearance) 과정이 반복적으로 일어나며 그 과정에서 기포붕괴에 따른 큰 충격압력을 방지하려는 분야와 이를 능동적으로 산업분야에 적용하려는 분야로 크게 대별된다. 본 연구에서는 캐비테이션의 붕괴거동을 수중 초음파 진동자에서 미세기포를 발생시켜 PIV기법을 이용하여 유동장을 계측하였다. 초음파 진동자는 직경 16 mm이며, 진동주파수는 20 kHz, 진폭은 $5{\mu}m$, $10{\mu}m$, $30{\mu}m$ 및 $50{\mu}m$를 각각 적용하였다. 유동구조, 난류강도, 레이놀즈 응력에 대한 통계적 유동정보를 계측한 결과 충격압력의 원인으로 알려진 캐비티 붕괴로 인해 유동특성을 확인하였다.

• Transactions of the Korean Society for Noise and Vibration Engineering
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• v.26 no.6_spc
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• pp.705-713
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• 2016

Underwater noise produced by ships has been becoming an increasing issue. A dominantly contributing noise source is a ship propeller. Therefore, it is important to predict the propeller noise at the propeller design stages. This study applied the acoustic analogy based on Ffowcs Williams equation for the prediction of the marine propeller BPF noise. A marine propeller BPF noise is investigated experimentally as well as numerically. Propeller BPF noise measurement and propeller cavitation observation tests are performed in the KRISO medium size cavitation tunnel. Numerical prediction schemes of marine propeller BPF noise are presented together with the noise measurement method. Propeller BPF noise predictions and experiments are performed under the various propeller operating conditions including non-cavitating and caveating conditions. Numerical and experimental results are compared and analyzed. It is shown that numerical prediction results are generally in good agreement with the measured data.

• Proceedings of the Korean Society for Noise and Vibration Engineering Conference
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• 2005.11a
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• pp.479-484
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• 2005

The test blasts were carried out by detonating some single blastholes at two upper sites of the underground storage cavern the crude oil. One was performed at the entrance site of the construction tunnel and the other at the middle part of the underground storage cavern. Based on the blast-induced vibration measured by the test blasts, we suggested the propagation equations of blasting vibration that were capable of estimating the peak particle velocity. In addition, in order to assess the stability of the nearest ground storage tank, we did the frequency analysis and the response spectrum analysis with the particle velocity-time history and the particle acceleration-time history that were measured by the test blast carried out on the entrance site of the construction tunnel. In result, it was predicted that the displacement on the highest part of the tank shell was less than the allowable displacement.

• Journal of Korean Tunnelling and Underground Space Association
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• v.9 no.4
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• pp.403-413
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• 2007

As rock bolts become one of the main support systems in tunnels and underground structures, the integrity of the rock bolts affects the safety of these types of structures. The purpose of this study is the evaluation of rock bolt integrity using Fourier and wavelet transforms of the guided ultrasonic waves. After five rock bolt specimens with various defect ratios are embedded into a large scale concrete block, guided waves are generated by a PZT (lead zirconate titanate) element and measured by an acoustic emission (AE) sensor. The captured signals are analyzed in the frequency domain using the Fourier transform, and in the time-frequency domain using the wavelet transform based on a Gabor wavelet. The spectrum obtained from the Fourier transform shows that a portion of high frequency contents increases with increase in the defect ratio. Peak values in the time-frequency domain represent the interval of travel time of each echo. The energy velocities of the guided waves increase with the defect ratio. This study shows that the spectrum ratio and the energy velocity may be indicators fur the evaluation of rock bolt integrity.

• Journal of the Korea Academia-Industrial cooperation Society
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• v.17 no.7
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• pp.334-341
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• 2016

In this paper, the study of a waveguide aperture-coupled feed-structured antenna has been conducted for the purpose of applying it to a wireless back-haul system sufficient for high-capacity gigabits-per-second data rates. For this study, a $32{\times}32$ waveguide slot sub-array antenna with a corporate-feed structure was designed and produced. Also, this antenna is used at 57 GHz to 66 GHz in the V-band. The construction of the antenna is a laminated form with radiating parts (outer groove and slot, cavity), a coupled aperture, and feeds in each. The antenna was designed with HFSS, which is based on 3D-FEM, produced with aluminum processed by a precision-controlled milling machine, and assembled after a silver-plating process. The measurement result from analysis of the characteristics of the antenna shows that return loss is less than -12 dB, VSWR < 2.0, and a wide bandwidth ranges up to 16%. An overall first side lobe level is less than -12.3 dB, and a 3 dB beam width is narrow at about $1.85^{\circ}$. Also, antenna gain is 38.5 dBi, offering high efficiency exceeding 90%.

• Journal of the Korean earth science society
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• v.27 no.6
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• pp.670-676
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• 2006

We present a B and V band time-series CCD photometry of ${\delta}$ Scuti type variable star HR 2707. The observation was carried out for 45 nights between November 13, 2001 and February 20, 2002 with a 40 cm telescope equipped with a 1K CCD camera at the Korea National University of Education Optical Astronomy Observatory. Through the time-series CCD photometry we obtained 3011 V band and 6562 B band CCD frames. In some of these data, the V band data obtained for seven nights in January of 2002, had been used as a part of a multi-site campaign by Lopez de Coca et al. (2003). To detect pulsational frequencies, we used Discrete Fourier Transformation (DFT) and linear least square method. We have detected eight resonable pulsational frequencies and compare to previous studies we determine $f_1,\;f_2,\;f_3,\;f_4,\;f_5$ of Lopez do Coca et al. (2003) and $f_4$ for derived from this study are real pulsational frequencies of HR 2707.

• Journal of the Korea institute for structural maintenance and inspection
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• v.21 no.4
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• pp.69-79
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• 2017

The purpose of this study is to reconsider the rating method for the floor impact sound insulation performance in current criterion. Although there are some arguments about proper standard heavy impact source with reproducibility of actual impact source in residence building, bang machine is adopted as the only standard heavy impact source in domestic criterion. To inspect the rating methods of evaluation criteria, this study conducted vibration test for both of standard heavy impact sources and actual impact sources. Using the test results, the floor impact sound insulation performance levels were assessed by each of several criteria. In addition, low frequency noise beyond current criteria was evaluated. Consequently, the floor impact sound levels have different performance levels according to adopted criteria, and measured floor impact sounds are bound to annoy the neighbors in the low frequency range. Current criteria does not consider the spectrum characteristics of floor impact sound according to impact sources and low frequency noise. This may cause the difference between the floor impact sound insulation performance level and human perception. Thus current criterion needs to be complemented to reflect the spectrum characteristics of floor impact sound levels according to impact sources and sound pressure levels in low frequency range.

• Journal of Astronomy and Space Sciences
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• v.14 no.2
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• pp.275-285
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• 1997

We have investigated Pi 2 pulsations which were observed both on ground magnetometer array and by satellites. On November 9th in 1994, Pi 2 pulsations appeared globally on the 190/210 magnetometer chain and Hermanus station when two satellites(EXOS-D and ETS-VI) were located near the magnetic meridian of the 210 array. The local time of measurements covers from morning(LT=8.47hr) to afternoon(LT=20.3hr) and the bandwidth of peak frequency is found relatively small. The signals of the electric field are highly coherent with ground-based observations with the out of phase oscillations. However, the magnetic field measurement on the ETS-VI in the outer magnetosphere(L=6.60) shows no signature of Pi 2 pulsations over the same time interval and the correlation with any of the ground-based stations is found to be very weak, even through both satellites and magnetometer chain are located close to each other in local time. We suggest that this event may be a direct evidence of Pi 2 pulsations as virtual resonant modes which are localized in the plasmasphere(Lee 1996). The results show that the cavity mode oscillations can occur in the inner magnetosphere with less spectral noise compared to the outer magnetospheric case.