• Title/Summary/Keyword: sub-6 GHz

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A Design of Small PCB Antenna using Helical Structure for IMT-2000 Handsets (헬리컬 구조를 이용한 IMT-2000 단말기용 소형 인쇄기판형 안테나 설계)

  • 김성철;이중근;김혜광
    • The Journal of Korean Institute of Electromagnetic Engineering and Science
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    • v.14 no.5
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    • pp.444-449
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    • 2003
  • In this paper, a PCB(Printed Circuit Board) antenna for IMT-2000 is designed and analyzed. The antenna has a helical structure with via-holes and lines on FR-4($\varepsilon$$\sub$${\gamma}$/=4.6 ) PCB, and the type of feeding is GCPW(Grounded Co-Planar Waveguide). Using HFSS of Ansoft, the antenna was designed and the measured results of frequency and radiation characteristic,3 with VSWR<2.0 are satisfied within operating frequency band of 1.920∼2.170 GHz. And it has resonating frequency of 2.045 GHz and a bandwidth of 321 MHz. The radiation gain of the antenna was measured to be -1 dBi.

Complex organic molecules detected in twelve high mass star forming regions with ALMA

  • Baek, Giseon;Lee, Jeong-Eun;Hirota, Tomoya;Kim, Kee-Tae
    • The Bulletin of The Korean Astronomical Society
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    • v.46 no.2
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    • pp.37.3-38
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    • 2021
  • One of the key questions on star formation is how the organic molecules are synthesized and delivered to the planets and comets since they are the building blocks of prebiotic molecules such as amino acid, which is thought to contribute to bringing life on Earth. Recent astrochemical models and experiments have explained that complex organic molecules (COMs; molecules composed of six or more atoms) are produced on the dust grain mantles in cold and dense gas in prestellar cores. However, the chemical networks and the roles of physical conditions on chemistry are not still understood well. To address this question, hot (> 100 K) cores in high mass young stellar objects (M > 8 Msun) are great laboratories due to their strong emissions and larger samples than those of low-mass counterparts. In addition, CH3OH masers, which have been mostly found in high mass star forming regions, can provide constraints due to their very unique emerging mechanisms. We investigate twelve high mass star forming regions in ALMA band 6 observation. They are associated with 44/95 GHz Class I and 6.7 GHz Class II CH3OH masers, implying that the active accretion processes are ongoing. For these previously unresolved regions, 66 continuum peaks are detected. Among them, we found 28 cores emitting COMs and specified 10 cores associated with 6.7 GHz Class II CH3OH masers. The chemical diversity of COMs is found in cores in terms of richness and complexity; we identified up to 19 COMs including oxygen- and nitrogen-bearing molecules and their isotopologues in a core. Oxygen-bearing molecules appear to be abundant and more complex than nitrogen-bearing species. On the other hand, the COMs detection rate steeply grows with the gas column density, which can be attributed to the effective COMs formation in dense cores.

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Analysis of Interference Impact of UWB System on WiBro System (UWB 시스템에 의한 WiBro 시스템에서의 간섭영향에 관한 연구)

  • Yoon Young-Keun;Hong Heon-Jin;Lee Il-Kyoo;Choi Ik-Guen;Kwak Kyung-Sub
    • The Journal of Korean Institute of Communications and Information Sciences
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    • v.31 no.8A
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    • pp.814-819
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    • 2006
  • This paper presents the impacts of Ultra Wide-Band(UWB) system applied in Indoor and Handhold communications using frequency band from 3.1 GHz to 10.6 GHz on Wireless Broad-band(WiBro) system based on Orthogonal Frequency Division Multiplexing(OFDM) using frequency of 2.3 GHz. The Minimum Coupling Loss(MCL) method for the case of single interference and Monte Carlo(MC) simulation for multiple interference considering practical scenario were used to evaluate the interference effects of UWB system on WiBro system. As a result, the minimum separation distance between single interferer and the victim receiver required 34.4 m and above to guarantee the co-existence. Also, the UWB transmitting PSD of around - 81 dBm / MHz below should be required to meet the minimum throughput loss of WiBro mobile station in case of multiple UWB interference.

Phase Evolution, Thermal Expansion, and Microwave Dielectric Properties of Cordierite-Al2O3 Composite

  • Kim, Shin;Song, Eun-Doe;Hwang, Hae-Jin;Lee, Joo-sung;Yoon, Sang-Ok
    • Journal of the Korean Institute of Electrical and Electronic Material Engineers
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    • v.34 no.5
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    • pp.337-341
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    • 2021
  • Phase evolution, thermal and microwave dielectric properties of cordierite-Al2O3 composite were investigated. As the content of Al2O3 increased, mullite, sapphirine, and spinel were formed as secondary phases, implying that cordierite may be decomposed by the reaction with Al2O3. All sintered specimens exhibited dense microstructures. The densification occurred through liquid phase sintering. As the content of Al2O3 increased, the thermal expansion coefficient and the dielectric constant increased, whereas the quality factor decreased. The thermal expansion coefficient, the dielectric constant, and the quality factor of the 90 wt% cordierite 10 wt% Al2O3 composite sintered at 1,425℃ were 2.9×10-6 K-1, 5.1, and 34,844 GHz, respectively.

Microwave Dielectric Properties of (Ba1-2xNa2x)(Mg0.5-xZrxW0.5)O3 Ceramics ((Ba1-2xNa2x)(Mg0.5-xZrxW0.5)O3 세라믹스의 마이크로파 유전특성)

  • Yoon, Sang-Ok;Hong, Chang-Bae;Lee, Yun-Joong;Kim, Shin
    • Journal of the Korean Institute of Electrical and Electronic Material Engineers
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    • v.30 no.6
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    • pp.356-360
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    • 2017
  • We investigated the phase evolution, microstructure, and microwave dielectric properties of Na- and Zr-doped $Ba(Mg_{0.5}W_{0.5})O_3$ [i.e., ($Ba_{1-2x}Na_{2x})(Mg_{0.5-x}Zr_xW_{0.5})O_3$] ceramics. $BaWO_4$ as a secondary phase was observed in all compositions, and it increased as the dopant concentration increased. All specimens revealed a dense microstructure. For the composition of x=0.01, polyhedral grains were observed. As the dopant concentration increased, the densification and the grain growth were promoted by a liquid phase. The quality factor($Q{\times}f_0$) decreased remarkably, whereas the dielectric constant (${\varepsilon}_r$) tended to decrease as the dopant concentration increased. The dielectric constant, quality factor, and temperature coefficient of the resonant frequency of the composition of x=0.01 sintered at $1,700^{\circ}C$ for 1 h were 18.6, 216,275 GHz, and $-22.0ppm/^{\circ}C$, respectively.

Microwave Dielectric Properties of MgTiO3, MgTa2O6/Polytetrafluoroethylene Composite

  • Jeon, Chang-Jun;Kim, Eung-Soo
    • Journal of the Korean Ceramic Society
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    • v.49 no.3
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    • pp.272-278
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    • 2012
  • Effects of ceramics on the microwave dielectric properties of polytetrafluoroethylene (PTFE) composites filled with $MgTiO_3$ (MTi) and/or $MgTa_2O_6$ (MTa) were investigated. The dielectric constant ($K$), quality factor ($Qf$), and temperature coefficient of resonant frequency ($TCF$) of the composites were dependent on the type and volume fraction ($V_f$) of the ceramics. For the composites mixed with MTa and MTi, the $K$ and $TCF$ values decreased with increasing MTi content. The $Qf$ values of the composites were affected by relative density. The measured $K$ values of the composites were compared with those predicted by several theoretical models. Good microwave dielectric properties with values of $K$=3.6, $Qf$ = 7,788 GHz, and $TCF$ = -0.19 ppm/$^{\circ}C$ were obtained for the composites with 0.1 $V_f$ ceramics (mixed 0.025MTa and 0.075MTi).

Design of a Sub-micron Locking Time Integer-N PLL Using a Delay Locked-Loop (지연고정루프를 이용한 $1{\mu}s$ 아래의 위상고정시간을 가지는 Integer-N 방식의 위상고정루프 설계)

  • Choi, Hyek-Hwan;Kwon, Tae-Ha
    • Journal of the Korea Institute of Information and Communication Engineering
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    • v.13 no.11
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    • pp.2378-2384
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    • 2009
  • A novel phase-locked loop(PLL) architecture of sub-micron locking time has been proposed. Input frequency is multiplied by using a delay-locked loop(DLL). The input frequency of a PLL is multiplied while the PLL is out of lock. The multiplied input frequency makes the PLL having a wider loop bandwidth. It has been simulated with a $0.18{\mu}m$ 1.8V CMOS process. The simulated locking time is $0.9{\mu}s$ at 162.5MHz and 2.6GHz, input and output frequency, respectively.

Low Temperature Sintering of B2O3 -added (Zn0.8Mg0.2)TiO3 Microwave Dielectric Ceramics (B2O3 가 첨가된 (Zn0.8Mg0.2)TiO3 마이크로파 유전체 세라믹스의 저온소결)

  • Bang, Jae-Cheol
    • Journal of the Korean Institute of Electrical and Electronic Material Engineers
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    • v.19 no.1
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    • pp.29-34
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    • 2006
  • The effects of $B_2O_3$ addition on the low-temperature sintering behavior and microwave dielectric properties of $(Zn_{0.8}Mg_{0.2})TiO_3$ ceramic system were investigated. Highly dense samples were obtained at the sintering temperatures below $900^{\circ}C$. The $Q{\times}f_o$ values were determined by the microstructures and sintering shrinkages which are affected by the amount of $B_2O_3$ and sintering temperature. Temperature coefficient of resonance frequency($T_f$) changes to a positive value with increasing the amount of $B_2O_3$ due to the increased amount of rutile phase which is one of the reaction products between $(Zn_{0.8}Mg_{0.2})TiO_3$ and $B_2O_3$. For $6.19 moi.{\%}B_2O_3$-added $(Zn_{0.8}Mg_{0.2})TiO_3$ system, it exhibits ${\epsilon}_r$ = 23.5, $Q{\times}f_o$ = 53,000 GHz, and $T_f$ = 0 ppm/$^{\circ}C$ when sintered at $900^{\circ}C$ for 5 h.

Sub-Terahertz On-Chip Microstrip Patch Antenna in CMOS with Metal Dummy Structures (메탈 더미 구조를 포함하는 서브 테라헤르츠 CMOS 온칩 마이크로스트립 패치 안테나)

  • Shim, Dongha;Yang, Ji Hoon;Han, Seung Han;Lee, Hyounmin;Kim, Ki Hoon;Kim, Hokyung
    • The Journal of Korean Institute of Electromagnetic Engineering and Science
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    • v.28 no.6
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    • pp.505-508
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    • 2017
  • This paper analyzes the effect of metal dummy structures in CMOS on antenna performances of a sub-terahertz on-chip microstrip patch antenna. A 400-GHz on-chip antenna is designed in a 45-nm CMOS process, and the resonance frequency and efficiency of the antenna are analyzed depending on the density of metal dummy structures. Antennas integrated with an oscillator are designed and fabricated for verification, and measurements are performed using quasi-optical methods with an FTIR and bolometer. The measurement results shows that the radiated power drops from 420 nW to 90 nW by 6.8 dB due to the dummy structures with the density of 27 %.

Affecting factors on low-temperature sintering of 0.85CaWO4-0.15SmNbO4 ceramics

  • Kim, Su-Jung;Kim, Eung-Soo
    • Journal of the Korean Crystal Growth and Crystal Technology
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    • v.17 no.6
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    • pp.245-250
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    • 2007
  • This study was focused on the effect of sintering additive and particle size on the low temperature sintering of $0.85CaWO_4-0.15SmNbO_4$ ceramics. With an increase of $CaV_2O_6$ content, the sintering temperature of the specimens was reduced from $1150^{\circ}C\;to\;800^{\circ}C$. The dielectric constant (K) and Qf value were increased with $CaV_2O_6$ content. These results are due to the enhancement of the density by the liquid phase sintering. Temperature coefficient of resonant frequency (TCF) was slightly shifted to the positive value with $CaV_2O_6$ content. Typically, K of 12.64, Qf of 23,106 GHz, TCF of $-34ppm/^{\circ}C$ were obtained for the specimens with 7 wt.% $CaV_2O_6$ sintered at $900^{\circ}C$ for 3 h.