• Title/Summary/Keyword: Receiver performance

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A Novel Design of CDSK Receiver for Improving the BER Performance (BER 성능 향상을 위해 제안하는 새로운 CDSK 수신기)

  • Lee, Jun-Hyun;Ryu, Heung-Gyoon
    • The Journal of Korean Institute of Communications and Information Sciences
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    • v.38A no.8
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    • pp.638-643
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    • 2013
  • Chaos communication system has a sensitive characteristic to initial conditions, because completely another signal is generated when initial condition of chaos equation is changed subtly. Also, chaos communication systems have the characteristics of non-periodic, non-predictability, the broadband signal, such as ease of implementation. Due to these characteristics, security of chaos communication system generally is evaluated better than other systems. However, BER(Bit Error Rate) performance is evaluated worse than other digital system, because existing chaos communication system's transmitter and receiver are strong influence by interference signal and noise. So, research to improve the BER performance of the chaotic communication system is performed continuously. In this paper, We will propose a new CDSK(Correlation Delay Shift Keying) receiver for BER performance improvement. After we compare to the performance of existing CDSK receiver and proposed CDSK receiver, BER performance of proposed CDSK receiver evaluate. Also, when using the new CDSK receiver, we evaluate the BER performance according to the spreading factors and find an optimum spreading factor. If chaos communication system use a new CDSK receiver, BER performance is improved than existing CDSK receiver. Also, if spreading factor's value is increased, BER performance is improved, because it is not nearly affected by interference signal and noise.

Performance Analysis of FFH/MFSK System with Clipper Receiver in the Presence of Multitone Interference (다중톤 재밍 환경에서 clipper 수신기를 사용하는 FFH/MFSK 시스템의 성능 분석)

  • 전근표;곽진삼;권오주;박재돈;이재홍
    • Proceedings of the IEEK Conference
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    • 2003.11c
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    • pp.15-19
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    • 2003
  • In this paper, the bit error rate (BER) performance of the fast frequency hopping/M-ary frequency shift keying system using the clipper receiver is analyzed by using the characteristic function (CF) technique in the presence of n=1 band multitone jamming and additive white Gaussian noise environment. The CFs of the clipper receiver outputs are derived as a infinite series representation using Gamma function and Marcum's Q -function. The analytical results are validated with various simulation results. Performance comparisons with linear combining receiver are shown that the BER performance of the clipper receiver is much better than that of the linear combining receiver In addition, as the clipping level approaches to infinity, it is shown that the clipper receiver simply performs a linear combining without clipping and there exists an optimum value of diversity level (the number of hops per symbol) that maximizes the worst case BER performance of the clipper receiver.

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Thermal Performance of Air receiver with a Change of Flow direction for Dish Solar Collector (공기식 흡수기의 유동 방향에 따른 $5kW_t$급 접시형 태양열 집열기의 열성능 분석)

  • Seo, Joo-Hyun;Kang, Kyung-Moon;Lee, Ju-Han;Oh, Sang-June;Seo, Tae-Beom
    • 한국신재생에너지학회:학술대회논문집
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    • 2008.05a
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    • pp.182-185
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    • 2008
  • The thermal performance of air receiver with a change of flow direction for dish solar collector. This system is installed and operated in Incheon, Korea. The thermal capacity of the system is about 5 kW thermal. The aperture diameter of the cylindrical-shape receiver which is made of stainless steel is 100 mm, and the height is 210 mm. Experiments are being carried out to investigate the thermal performance variation of the receivers with several design parameters such as the shape of the receiver, the flow directions and the flow rate of air. First, air flows into the upper part of the receiver, which is the opposite side of the aperture. After the air flows through the inside receiver, that goes out of the receiver through 3 exits which are located near the aperture. Second, air flows into the backside of the receiver, Which is the forward side of the aperture. After the air flows through the inside receiver, that goes out of the receiver through 1 exit. The results show that the system efficiency and receiver efficiency increase as the volume flow rate increases as expected.

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A Novel Transmitter and Receiver Design of CDSK-Based Chaos Communication System (CDSK 방식의 카오스 통신 시스템의 새로운 송·수신기 설계)

  • Lee, Jun-Hyun;Ryu, Heung-Gyoon
    • The Journal of Korean Institute of Electromagnetic Engineering and Science
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    • v.24 no.10
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    • pp.987-993
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    • 2013
  • Chaos communication system has characteristics of non-periodic, non-predictability, broadband signal and easy implementation. Also, chaos communication system is sensitive to the initial value, because completely another signal is generated when initial value of chaos equation is changed subtly. By these characteristics, security of chaos communication system is generally evaluated better than other digital communication systems. However, BER(Bit Error Rate) performance is worse than other digital communication systems, because transmitter and receiver of existing chaos communication system are strongly influenced by reference signal and noise. So, studies in order to improve the BER performance of chaos communication system is continuously performed. In this paper, We will propose a new CDSK (Correlation Delay Shift Keying) receiver in order to improve the BER performance. After we compare to the performance of existing receiver and proposed receiver, BER performance of proposed receiver evaluate. A novel receiver has characteristic that BER performance is better than existing receiver. However, if existing transmitter is used, existing receiver is possible to recover information bits even though BER performance is bad. Therefore, we propose a novel CDSK transmitter in order to improve the security of proposed receiver. When information bits are transmitted by using proposed transmitter, existing receiver is impossible to recover information bits, and proposed receiver is possible to recover information bits.

DESIGN OF THE IF DISTRIBUTOR AND V/F CONVERTER FOR RECEIVER SYSTEM (우주전파 수신기를 위한 IF 분배기 및 V/F 컨버터 설계)

  • Kim, Kwang-Dong;Yim, In-Sung;Byun, Do-Young;Song, Min-Gyu
    • Publications of The Korean Astronomical Society
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    • v.22 no.3
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    • pp.83-87
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    • 2007
  • We designed the Intermediate Frequency(IF) distributor for multi beam backend system and manufactured Voltage to Frequency Converter(VFC) to measure the multi-beam receiver performance. Multi beam receiver has 15 channel receivers and can get 15 spectrums at once. The multi beam receiver has more observation efficiency than single beam receiver. We manufactured the 15 IF distributors to distribute IF signal for Autocorrelation spectrometer that is radio signal processor. Also, we manufactured the VF Converter to test the performance measurement of receiver for Korea VLBI Network(KVN) system which is under-construct in Seoul, Ulsan and Jeju. As a result of performance measurement, we could obtain linearity of 99.4% on the input power vs output frequency and measured the operating range of input frequency.

Performance Comparison of Dish Solar Collector With Mirror Arrays & Receiver Shapes (반사경 배치와 흡수기 형상에 따른 접시형 고온 태양열 시스템 성능비교)

  • Ma, Dae-Sung;Kim, Yong;Seo, Tae-Beom
    • Journal of the Korean Solar Energy Society
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    • v.27 no.1
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    • pp.29-38
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    • 2007
  • In order to analyze the performance comparison of dish solar collector with mirror arrays and receiver shapes, the radiative heat flux distribution inside the cavity receiver is numerically investigated. The solar irradiation reflected by dish solar collector is traced using the Monte-Carlo method. Five different dish solar collectors and three different cavity receivers are considered. A parabolic-shaped perfect mirror of which diameter is 1.5 m is considered as a reference dish solar collector and four different arrays of twelve identical parabolic-shaped mirror facets of which diameter are 0.4 m are used. Their reflecting areas, which are $1.5\;m^2$, are the same. Three different cavity receiver shapes are dome, conical, and cylindrical. In addition, the radiative properties of the concentrating surfaces can vary the thermal performance of the cavity receiver so that variation of the surface reflectivity of each mirror is considered. Based on the calculation, the design information of dish solar collector for producing the electric power can be obtained. The results show that the dome type has the best performance in receiver shapes and the 2AND4 INLINE has the best performance in mirror arrays except perfect mirror.

Performance Evaluation of Maritime GPS Attitude Finding Receiver

  • Choi, Byung-Moom;Lee, Heon;Park, Chan-Sik
    • 제어로봇시스템학회:학술대회논문집
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    • 2001.10a
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    • pp.113.4-113
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    • 2001
  • A 24 channel L1 C/A-code GPS attitude-finding receiver is designed and implemented. The performance of developed receiver is evaluated under the various environments. The results show that the performances from land and maritime test are almost same in the calm lake. And it follows the expected performance derived from an analysis. It is expected that the developed receiver can be used in not only maritime applications but also land and air applications where the heading is required.

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A study on the RF receiving system design and on the performance improvement for PCS mobile station (개인휴대통신을 위한 이동국 RF 수신시스템의 설계 및 성능개선에 관한 연구)

  • 오정일;천종훈
    • Journal of the Korean Institute of Telematics and Electronics C
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    • v.34C no.11
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    • pp.66-75
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    • 1997
  • We derive the system design parameters to implement the receiving system for the PCS mobile station to satisfy the J-sTD-018 which is the PCS mobile station(MS) minimum performance. Also we analyze the system performance and intermodulation spurious due to the values of a device cause the system performance degradation, is proposed. The simulation shows the receiver's maximum system noise figure to satisfy the receiver selectivity is approximately 11 dB. While the MS noise figure is 10dB with system margin 1 dB, the minimum selectivity is -71 dB at 1.25MHz frequency offset from the carrier frequency. And the input 3rd order intercept point of the MS class I and the MS class II~V is -9.5 dBm and -14dBm respectively. When the interference power level at the receiver is small, the receiver has better performance as we increase the gain of the LNA. However, when the interference level at the receiver is large, the receiver performance is heavily affected by the spurious as we increase the gain of the LNA. Thus, we proved the effectiveness of the LNA On/Off switching technique as to reduce the effect of the spurious.

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Performance Analysis of the RAKE Receiver over a Multipath Fading Channel (다경로 페이딩 채널에서 RAKE 수신기의 성능 분석)

  • 고영훈;박성경;홍대식;강창언
    • The Proceeding of the Korean Institute of Electromagnetic Engineering and Science
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    • v.4 no.3
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    • pp.30-36
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    • 1993
  • This paper presents the RAKE receiver over a multipath fading channel. This interference between the propagation paths in a multipath fading causes a serious degradation in the mobile communication environment. In order to derive the path interference and reduce the fading effect, the RAKE receiver is used. As a result, the RAKE receiver gives a better performance than the DS / SS receiver over a multipath fading channel.

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Analysis of Heat Loss with Mirror Array and Receiver Shapes on the Dish Solar Collector (반사경 배치 및 흡수기 형상에 따른 접시형 태양열 집열기의 열손실 해석)

  • Seo, Joo-Hyun;Ma, Dae-Sung;Kim, Yong;Kang, Yong-Heack;Seo, Tae-Beom
    • Korean Journal of Air-Conditioning and Refrigeration Engineering
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    • v.20 no.1
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    • pp.35-41
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    • 2008
  • The radiative heat loss from a receiver of a dish solar collector is numerically investigated. The dish solar collector considered in this paper consists of a receiver and multi-faceted mirrors. In order to investigate the performance comparison of dish solar collectors, six different mirror arrays and four different receivers are considered. A parabolic- shaped perfect mirror of which diameter is 1.40 m is considered as the reference for the mirror arrays. The other mirror arrays which consist of twelve identical parabolic-shaped mirror facets of which diameter are 0.405 m are suggested for comparison. Their reflecting areas, which are 1.545 $m^{2}$, are the same. Four different receiver shapes are a conical, a dome, a cylindrical, and a unicorn type. The radiative properties of the mirror surfaces and the receiver surfaces may vary the thermal performance of the dish solar collector so that various surface properties are considered. In order to calculate the radiative heat loss in the receiver, two kinds of methods are used. The Net Radiation Method that is based on the radiation heat balance on the surface is used to calculate the radiation heat transfer rate from the inside surface of the receiver to the environment. The Monte-Carlo Method that is the statistical approach is adopted to predict the radiation heat transfer rate from the reflector to the receiver. The collector efficiency is defined as the results of the optical efficiency and the receiver efficiency. Based on the calculation, the unicorn type has the best performance in receiver shapes and the STAR has the best performance in mirror arrays except the perfect mirror.