• 한국전자파학회논문지
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• 제19권10호
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• pp.1159-1165
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• 2008

본 논문에서는 다양한 방사 편파를 얻기 위하여 모서리가 잘린 정삼각형 마이크로스트립 안테나를 제안하였다. 제안한 안테나는 삼각형 패치의 빗변과 평행하게 놓여진 마이크로스트립 라인에 의해 급전된다. 동일한 크기를 갖는 삼각형 모서리의 제거 여부에 따라 정삼각형 마이크로스트립 안테나는 선형 편파, 왼손 원형 편파, 오른손 원형 편파 특성을 나타내었다. 이러한 특성을 바탕으로 정삼각형 마이크로스트립 안테나를 편파 변환이 가능한 재구성 안테나로 응용하였다. 정삼각형 패치와 작은 삼각형 기생 패치 사이에 PIN 다이오드를 적용하였다. 다이오드에 인가되는 바이어스 전압에 따라 안테나는 선형 편파 또는 오른손 원형 편파 특성을 나타내었다. 측정된 방사 패턴 결과를 통해 선형 편파의 경우 낮은 크로스폴을, 원형 편파의 경우 좋은 축비 특성을 나타냄을 알 수 있었다.

• 한국전자통신학회논문지
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• 제18권2호
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• pp.251-258
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• 2023

본 논문에서는 특화망에 적용 가능한 DLP(Dual Linear Polarization) 적층 안테나를 제안하였다. 제안된 안테나는 일반적인 적층구조를 갖고 최대이득을 얻을 수 있도록 공기 갭을 갖도록 설계하였다. 격리도를 개선하기 위해서 두 개의 급전포트를 각 층으로 분리하여 설계하였다. 각각 패치의 크기는 하위층, 17.80 mm×16.70 mm(W1×L1) 그리고 상위층 18.56 mm×18.73 mm(W2×L2)이며 적층 안테나의 전체 크기는 40.0 mm(W)×40.0 mm(L)이며, 모두 두께(h) 1.6 mm, 그리고 비유전율이 4.4인 FR-4 기판을 사용하였다. 제작 및 측정결과로부터, -10 dB 반사손실을 기준으로 입력포트 1에서 100.0 MHz (4.74~4.84 GHz), 입력포트 2에서 150.0 MHz (4.67~4.82 GHz)의 대역폭을 얻었으며 전달계수 S21은 -20 dB 이하의 값을 얻었다. 또한 각 급전포트에서의 편파분리도를 얻었다.

• 천문학회지
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• 제40권1호
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• pp.1-7
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• 2007

About 10 percent of quasars are known to exhibit deep broad absorption troughs blueward of prominent permitted emission lines, which are usually attributed to the existence of outflows slightly above he accretion disk around the supermassive black hole. Typical widths up to 0.2c of these absorption roughs indicate the velocity scales in which special relativistic effects may not be negligible. Under he assumption of the ubiquity of the broad absorption line region in quasars, the broad emission line flux will exhibit Thomson scattered components from these fast outflows. In this paper, we provide our Monte Carlo calculation of linear polarization of singly Thomson scattered line radiation with the careful considerations of special relativistic effects. The scattering region is approximated by a collection of rings that are moving outward with speeds ${\upsilon}=c{\beta}<0.2c$ near the equatorial plane, and the scattered line photons are collected according to its direction and wavelength in the observer's rest frame. We find that the significantly extended red tail appears in the scattered radiation. We also find that the linear degree of polarization of singly Thomson scattered line radiation is wavelength-dependent and hat there are significant differences in the linear degree of polarization from that computed from classical physics in the far red tail. We propose that the semi-forbidden broad emission line C III]1909 may be significantly contributed from Thomson scattering because this line has small resonance scattering optical depth in the broad absorption line region, which leads to distinct and significant polarized flux in this broad emission line.

• 한국전자통신학회논문지
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• 제16권6호
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• pp.1037-1044
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• 2021

본 논문에서는 3.5 GHz 대역에 적용 가능한 DLP(Dual Linear Polarization) 배열 안테나를 제안하였다. 제안된 안테나는 1×4 배열 안테나로 구성되어 있으며 두 개의 입력포트를 갖도록 설계하였다. 또한 임피던스매칭을 위해 십자가 구조가 패치 아래 부분과 연결하였다. 각 안테나는 18.85 mm(W1)×18.85 mm(L1)의 크기를 갖으며 1×4 배열 안테나 전체 구조는 236.0 mm(W)×60.2 mm(L)의 크기를 갖으며 두께(h) 1.6 mm, 그리고 비유전율이 4.3인 FR-4 기판 위에 설계하였다. 제작 및 측정결과로부터, -10 dB 반사손실을 기준으로 입력포트 1에서 70 MHz (3.54~3.61 GHz), 입력포트 2에서 75 MHz (3.55~3.625 GHz)의 대역폭을 얻었으며 전달계수 S21은 -20dB 이하의 값을 얻었다. 또한 두 입력단자 사이의 교차편파의 값을 얻었다.

• 한국세라믹학회지
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• 제50권1호
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• pp.82-86
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• 2013

A poled lead zirconate titanate (PZT) cube specimen is subjected to impulse-type compressive stress with increasing magnitude in parallel to the poling direction at four room and high temperatures. During the ferroelastic domain switching induced by the compressive stress, electric displacement in the poling direction and longitudinal and transverse strains are measured. Using the measured responses, linear material properties, namely, the piezoelectric and elastic compliance coefficients, are evaluated by a graphical method, and the effects of stress and temperature are analyzed. Finally, the dependency of the evaluated linear material properties on relative remnant polarization is analyzed and discussed.

• ETRI Journal
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• 제28권3호
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• pp.379-382
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• 2006

A novel reconfigurable microstrip patch antenna with frequency and polarization diversities is proposed. A U-slot is incorporated into a square patch, and a PIN diode is utilized to switch the slot on and off, which realizes the frequency diversity characteristic. The polarization diversities among linear polarization (LP), right-hand circular polarization (RHCP), and left-hand circular polarization (LHCP) are also obtained by switching three PIN diodes on the slot and the truncating corners of a square patch on and off. The antenna design and experimental results are presented.

• 한국정보통신학회논문지
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• 제4권1호
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• pp.59-65
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• 2000

This paper describes the characteristics of a one dimensional narrow-wall slotted waveguide array with a single-layer linear-to-circular polarization converter consisting of a dipole array. An external boundary value Problem of one slot and three dipoles, which approximates the mutual coupling between the dipole array and an edge slot extending over three faces of a rectangular waveguide, is formulated and analyzed by the method of moments; design of polarization conversion is conducted for this model as a unit element. If every unit element has perfect circular polarization, grating lobes appear in the array pattern due to the alternating slot angle: these are suppressed in this paper by changing the dipole angle and degrading the axial ratio of the unit element. The validity of the design is confirmed by the measurements. The dipole array has negligible effects upon slot impedance; the polarization conversion for existing narrow-wall slotted arrays is realized by add-on dipole array.

• Current Optics and Photonics
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• 제6권1호
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• pp.23-31
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• 2022

Heterodyne efficiency is an indicator to evaluate the performance of space coherent laser communication systems. It is affected by signal light and local oscillator (LO) light amplitude, phase and polarization state. In this paper, based on the common heterodyne efficiency, a heterodyne efficiency model that can reflect polarization aberration of optical system is proposed. The heterodyne efficiency is analyzed when the signal light and the LO light are linearly polarized or circularly polarized. For a coherent communication optical system, when the incident signal light is right-circularly polarized light and the incident LO light is 45° linear polarized light. Based on the three-dimensional ray tracing theory and the heterodyne efficiency proposed in this paper, the change of polarization states and the distribution of heterodyne efficiency of the signal light and LO light influenced by the optical system's polarization aberration are analyzed. Analysis shows that the heterodyne efficiency model proposed in this paper can be used to evaluate coherent communication systems and reflect the influence of optical system polarization aberration.

• 천문학회보
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• 제40권2호
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• pp.36.2-36.2
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• 2015

We report the first detection of linearly polarized emission at an observing wavelength of 350 mum from the radio-loud active galactic nucleus 3C 279. We conducted polarization observations for 3C 279 using the SHARP polarimeter in the Caltech Submillimeter Observatory on 2014 March 13 and 14. For the first time, we detected the linear polarization with the degree of polarization of $13.3%{\pm}3.4%$ (3.9sigma) and the electric vector position angle (EVPA) of $34.^{\circ}7{\pm}5.^{\circ}6$. We also observed 3C 279 simultaneously at 13, 7, and 3.5 mm in dual polarization with the Korean very long baseline interferometry (VLBI) Network on 2014 March 6 (single dish) and imaged in milliarcsecond (mas) scales at 13, 7, 3.5, and 2.3 mm on March 22 (VLBI). We found that the degree of linear polarization increases from 10% to 13% at 13 mm to 350 mum and the EVPAs at all observing frequencies are parallel within < $10^{\circ}$ to the direction of the jet at mas scale, implying that the integrated magnetic fields are perpendicular to the jet in the innermost regions. We also found that the Faraday rotation measures RM are in a range of $-6.5{\times}102{\sim}-2.7{\times}103$ rad m-2 between 13 and 3.5 mm, and are scaled as a function of wavelength:| {RM}| ${\backslash}propto$ {lambda }-2.2. These results indicate that the millimeter and sub-millimeter polarization emission are generated in the compact jet within 1 mas scale and affected by a Faraday screen in or in the close proximity of the jet.

• 한국전기전자재료학회:학술대회논문집
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• 한국전기전자재료학회 2000년도 하계학술대회 논문집
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• pp.299-302
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• 2000

In this study, we have made the large holographic surface relief gratings on amorphous chalcogenide $As_{40}$$Ge_{10}$$Se_{15}$$S_{35}$ films by two beam interference using a He-Ne laser(632.8nm) light. The film thickness was about 0.6$\mu\textrm{m}$, we could magnify beam size by using beam expander. We made use $90^{\circ}$ holder which was made of reflection mirror and sample. Formed the surface relief structures were investigated using optical microscope. The diffraction efficiency was obtained by measuring +lst order intensity. In addition we investigated grating formation and diffraction efficiency as a function of polarization states which is linear or circular polarization. The results indicate that the grating was formed by linear polarized beam is better clear than that by circular polarized beam.