• 대한전자공학회:학술대회논문집
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• 대한전자공학회 1999년도 하계종합학술대회 논문집
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• pp.305-308
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• 1999

In this paper, a transimpedance optical receiver based on PIN/P-HEMT with cascoded input stage and inductor peaking technique was designed for several giga bits optical communication. Analysis of the receiver shows that cascoded input stage with inductor peaking increase bandwidth without sacrificing low frequence gain. The receiver achieved a low noise characteristic and maximally flat frequence response. It is shown that the 3-dB bandwidth of the designed receiver is 8.3 ㎓ and input equivalent noise current is as low as 16pA/√Hz to 10㎓.

• Journal of Astronomy and Space Sciences
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• 제21권1호
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• pp.29-38
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• 2004

VLBI(Very Long Baseline Interferometer)에서 요구되는 고위상 안정도를 갖는 국부발진기를 사용하여 초저잡음 Q-band우주 전파 수신기를 개발하였다. 냉각용 HEMT 중폭기를 사용하여, 관측 주파수 범위인 420㎓에서 44㎓까지의 대역폭에서는 65K정도의 수신기 잡음 온도를 얻었으며, 390㎓ -46㎓의 대역폭에서는 l00k 이하의 잡음 온도를 얻었다. SiO분자선 관측이 주된 목적이며, 이 대역에서 얻어진 수신기 잡음온도는 독일$.$일본 전파천문대에서 개발된 수신기보다 우수한 성능을 나타낸다.

• 한국소음진동공학회:학술대회논문집
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• 한국소음진동공학회 2014년도 춘계학술대회 논문집
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• pp.90-95
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• 2014

In order to investigate low frequency swishing noise of wind turbines, singularity in circular motion with large radius is introduced as a noise source model. By employing Lowson's acoustic analogy, simple exact solution is obtained. The solution shows that time histories of acoustic pressure at receiver points varied significantly according to receiver's directional location, even when the retarded time distributions are similar. However, the corresponding spectra of sound pressure for the receiver locations where the retarded time distributions are almost the same are not significantly different. It can be inferred from these results that the time-averaged sound pressure spectra which cannot take into account the detailed difference in the time-variation of wind turbine noise may not represent the sound quality of wind turbines due to its swishing.

• 한국전자파학회:학술대회논문집
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• 한국전자파학회 2002년도 종합학술발표회 논문집 Vol.12 No.1
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• pp.69-73
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• 2002

We have designed and fabricated a low-cost, V-band CPW receiver chip set using GaAs PHEMT technology for the application of millimeter-wave wireless communication systems. Low noise amplifiers and down-converters were developed for this chip set. The fabricated low noise amplifier showed an S$\sub$21/ gain of 14.9 ㏈ at 60 ㎓ and a noise figure of 4.1 ㏈ at 52 ㎓. The down-converter exhibited a high conversion gain of 2 ㏈ at the low LO Power of 0 ㏈m. This work demonstrates that the GaAs PHEMT technology is a viable low-cost solution for V-band applications.

• 한국음향학회지
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• 제36권4호
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• pp.238-246
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• 2017

고주파수, 고해상도 초음파 영상을 획득하기 위해서는 고주파수 초음파 변환기가 가지는 작은 구경에 따른 낮은 민감도와 침투 깊이에 따른 높은 감쇠량을 극복하여야 한다. 이는 고주파수 초음파 변환기의 본질적인 한계점이므로 수신 시스템을 통하여 그 한계점을 극복하여야 한다. 본 논문은 고주파수, 고해상도 초음파 영상을 위하여 고주파수 초음파 변환기의 본질적인 한계인 낮은 민감도와 높은 감쇠량을 극복할 수 있는 저잡음 광대역 수신 시스템 개발과 특성 평가 결과에 관한 것이다. 개발한 저잡음 광대역 수신 시스템은 80 MHz 이상의 동작 주파수 대역에서 최대 73 dB의 증폭 이득과 48 dB의 가변 이득 범위를 만족하며 ${\pm}1dB$의 증폭 이득 평탄도 성능을 가진다. 또한 개발한 수신 시스템은 상용 리시버에 비하여 8.4 dB 이상의 신호대잡음비 성능과 3.7 dB 이상의 대조도 성능이 우수함을 확인하였다.

• 한국소음진동공학회논문집
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• 제24권7호
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• pp.569-574
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• 2014

In order to investigate low frequency swishing noise of wind turbines, acoustic source model using a singularity in circular motion is introduced to derive analytic solution of Lowson acoustic analogy in time domain. Results in time and frequency domains computed by the solution show apparent modulation of amplitude and frequency. The solution indicates that time histories of acoustic pressure at receiver points varied significantly according to receiver's directional location, even when the retarded time distributions are similar. However, the corresponding time-averaged spectra of sound pressure at the receiver locations where the retarded time distributions are almost same are not significantly different. It can be inferred from these results that the time-averaged sound pressure spectra which cannot take into account the detailed difference in the time-variation of wind turbine noise may not represent the sound quality of wind turbines due to its swishing. Finally, as an introduction of procedure to quantify low frequency swishing noise level, relative variation of overall sound pressure level is obtained using tonal low frequency noise model.

• Journal of Positioning, Navigation, and Timing
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• 제13권3호
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• pp.245-256
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• 2024

Following the introduction of civilian navigation, the commercial Global Navigation Satellite System (GNSS) receivers' market has been expanding in various fields such as autonomous driving and smart cities. With improved receiver performance and widespread use of GNSS, the configurations of base and rover receivers are becoming more complex. As a result, user must consider combinations of base stations with different qualities, costs, and performances. To address these issues, we conducted zero-baseline tests to analyze the double-differenced code-pseudorange noise of various receiver combinations, ranging from low- to high-cost. The results showed that the noise varied depending on the receiver combination. Notably, receivers from the same manufacturer exhibited similar noise and positioning errors despite significant price differences. We also found that the double-differenced noise of all receiver combinations was correlated with the Carrier-to-Noise Density Ratio (C/N0), the satellite elevation angle, and the Doppler shift, and it did not perfectly follow a normal distribution. Further analysis based on Modified Allan Deviation (MDEV) showed that different types of noise were observed for each receiver combination and the double-differenced noise and positioning errors have similar statistical characteristics. From this study, the importance of receiver combinations and their various characteristics can be better understood.

• 한국통신학회논문지
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• 제37권7A호
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• pp.545-551
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• 2012

본 논문에서는 K대역의 신호를 수신하여 저잡음 증폭 및 L대역으로 하향 변환하는 다채널 전단 수신기를 설계 및 제작하였다. 제작된 다채널 전단 수신기는 잡음지수 2.3 dB 이하의 특성을 가지는 GaAs-HEMT 기반의 저잡음 증폭소자, 이미지 성분의 억제를 위한 IR(Image Rejection) Filter, 이미지 성분 억제와 IMD (Intermodulation Distortion) 특성 개선을 위한 IR(Image rejection) 믹서를 포함한다. 제작된 다채널 전단 수신기의 시험결과, 3.8 dB 이하의 잡음지수와 27 dB 이상의 변환이득을 가지며 입력신호 기준 -9.5 dBm 이상의 P1dB(1dB Gain Compression Point) 특성을 나타내었다.

• Journal of electromagnetic engineering and science
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• 제18권3호
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• pp.188-198
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• 2018

In this study, we propose an approach for the design and satisfy the requirements of the fabrication of a small, lightweight, reliable, and stable ultra-wideband receiver for millimeter-wave bands and the contents of the approach. In this paper, we designed and fabricated a stable receiver with having low noise figure, flat gain characteristics, and low noise characteristics, suitable for millimeter-wave bands. The method uses the chip-and-wire process for the assembly and operation of a bare MMIC device. In order to compensate for the mismatch between the components used in the receiver, an amplifier, mixer, multiplier, and filter suitable for wideband frequency characteristics were designed and applied to the receiver. To improve the low frequency and narrow bandwidth of existing products, mathematical modeling of the wideband receiver was performed and based on this spurious signals generated from complex local oscillation signals were designed so as not to affect the RF path. In the ultra-wideband receiver, the gain was between 22.2 dB and 28.5 dB at Band A (input frequency, 18-26 GHz) with a flatness of approximately 6.3 dB, while the gain was between 21.9 dB and 26.0 dB at Band B (input frequency, 26-40 GHz) with a flatness of approximately 4.1 dB. The measured value of the noise figure at Band A was 7.92 dB and the maximum value of noise figure, measured at Band B was 8.58 dB. The leakage signal of the local oscillator (LO) was -97.3 dBm and -90 dBm at the 33 GHz and 44 GHz path, respectively. Measurement was made at the 15 GHz IF output of band A (LO, 33 GHz) and the suppression characteristic obtained through the measurement was approximately 30 dBc.

• 천문학논총
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• 제11권1호
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• pp.109-123
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• 1996

We have developed a 5GHz continuum receiver system. The receiver is a direct type receiver. In order to reduce the noise due to the fluctuation of the gain in the amplifiers, the system employs the Dicke switching method. We made the 5GHz low-noise amplifier and the bandpass filter. The low-noise amplifier gives ${\sim}35dB$ gain and has ${\sim}210K$ noise temperature. The bandpass filter has a passband between 4.3 and 5.4GHz. We also made switch driver, video amplifiers, phase detector, and integrator. Using a 1.8 meter offset parabolic antenna, we measured the efficiency of the system. Since the antenna does not have a driver to track objects, observations were performed with the antenna fixed. The measured noise temperature of the system is ${\sim}650K$. From the observation of the blank sky, noise level was measured. It was found that the systematic noise(${\sim}0.5K$: peak to peak value) is much larger than the thermal noise. The systematic noise is possibly related to the stability of the DC power supplied to the receiver system. Besides the noise of the system, it was found that the airplanes are the very serious noise sources. We measured the radio flux of the Sun using the developed system. The observed radio flux of the Sun is ${\sim}10^6Jy$, which is close to the known value of the quiet Sun. The test observation of the Sun shows that the angular beam size of the antenna is ${\sim}2.2^{\circ}$.