• 한국통신학회논문지
• /
• 제23권7호
• /
• pp.1764-1769
• /
• 1998

임의의 각도로 틀어진 서로 다른 두 도파관 사이에 임의의 형상을 가진 다중 공동으로 결합되는 방향성 결합기의 특성을 요한 요소 경계 적분법으로 해석하였다. 이러한 구조를 해석하는데 있어서 보통의 유한 요소법과의 계산 시간을 비교하여 제시된 방법이 매우 효율적임을 보였다. 또한 Moreno couple에 대한 기존의 다른 논문들의 결과와 비교하여 잘 일치함을 보임으로써 본 논문에서 제시한 방법의 타당성을 입증하였다.

• 전자공학회논문지A
• /
• 제29A권2호
• /
• pp.24-32
• /
• 1992

The impedance matching properties of infinite planar arrays of rectangular waveguides with dielectric plug loading and sheath covering are studied here. The effects of several involved parameters on the impedance matching of the phased array antenna are investigated by calculating the reflection coefficients numerically. The improvement of impedance matching and the appearance of forced surface wave resonances are also discussed.

• 전자공학회논문지A
• /
• 제30A권1호
• /
• pp.1-7
• /
• 1993

The radiation characteristics of a phased array antenna consisted of rectangular waveguides with a slant grid are investigated here. In particular, the effects of the slant angle on the radiation patterns are calculated by solving numerically the integral equation to the electric field over the waveguide aperture in view of the modal analysis. And it is found that the blindness on the radiation pattern can be moved by inserting a dielectric plug or sheath properly.

• 대한전기학회논문지:전기물성ㆍ응용부문C
• /
• 제50권6호
• /
• pp.296-302
• /
• 2001

In this paper, the vector finite elements are adopted to calculate eigenvalues of RF and microwave components. Simulation results show that spurious are completely avoided because of the divergence free nature of the vector elements. This paper seeks to extend these low-order elements to higher orders to improve the accuracy of numerical solution. Investigation of numerical results for a rectangular waveguide was provided. A vector finite element program was implemented to allow propagation constants and electric field distributions to be directly computed in the rectangular and circular waveguides which are partially filled with the dielectric.

• 대한전자공학회논문지
• /
• 제23권4호
• /
• pp.522-528
• /
• 1986

Based on the modified effective index method, analysis of dielectric rectangular waveguides and directional couplers are presented. Aside from the effective index concept of channel region, the equivalent index concept of cladding region is proposed. The error problem of eigenvalues, which has been experienced when the effective index method is used, is improved. Our approxiamtions give similar accuracy when compared with the results of other regorous approxiamtion techiniques. The advantage of the modified effective index methods is utilized by replacing the directional coupler with the equivalent slab guides, and the coupling constant is calculated by the coupled mode theory. The effectiveness of the equivalent index concept is positively confirmed.

• 한국통신학회논문지
• /
• 제22권8호
• /
• pp.1833-1841
• /
• 1997

집적광학에서 가장 기본적이고 필수적인 소자인 구형 유전체 도파로는 근사적인 해석방법에서부터 수치계산방법까지 여러가지 방법으로 연구되어왔다. 본 논문에서는 구형 유전체도파로의 해석을 위해 연속적인 섭동궤환방법을 이용하여 최적 등가도파로모델을 선택하고, 시뮬레이션을 통한 비교, 분석 결과, 섭동궤환방법을 이용해서 구한 전파상수가 다른 방법에 의해 얻어진 결과보다 더욱 정확한 값에 일치함으로써 최적의 근사치를 얻을 수 있음을 확인하였고, 또한 여기서 구한 전파 상수를 이용하여 여러 가지 집적광학 소자의 설계에 유용한 필드 특성을 표현하였다.

• Journal of Astronomy and Space Sciences
• /
• 제26권3호
• /
• pp.345-354
• /
• 2009

A stepped septum polarizer has been designed and fabricated for the 43 GHz band KVN receiver system. The dual-circular polarizer converts left and right hand circularly polarized signals into linear polarizations in two separated rectangular waveguides. Measurements show that the performance of the designed septum polarizer covering 42-48 GHz frequency band is adequate to meet the requirement of KVN receivers. Especially, a polarizer for the KVN receiver of 85-95 GHz frequency band can be fabricated by scaling the dimensions of the septum polarizer developed in this paper.

• 한국전기전자재료학회논문지
• /
• 제16권12호
• /
• pp.1087-1090
• /
• 2003

The circular cavity resonator which can measure the dielectric properties of dielectrics in the V -band(50㎓∼75㎓) frequency range was designed and fabricated. Exciting and detecting of the resonator is performed by WR15 rectangular waveguides using Bethe's small hole coupling. GaAs and PTFE plate samples were used for the verification of the performance of the fabricated circular cavity resonator. In the measurement of GaAs and PTFE using that resonator, the permittivity were measured as I2.87 and 2.14, respectively.

• 전자공학회논문지A
• /
• 제32A권6호
• /
• pp.1-9
• /
• 1995

The structures of inductive irises are used commonly in waveguide filter, especially at highter frequencyies, due to low loss and high temperature stability. However, the iris thickness can not be neglected, as it could be at the lower frequencies. Approximate models assuming zero thickness fail to predict the exact behavior of the filter. And current thickness correction is introduced which is valid in the case of thick irises only. Account of the effect of round is normally not taken. So the necessity of finding a relation for the two factors-iris thickness and round-arises in the design of waveguide filters. This paper describes a mutual relation that considers the combined effect of finite thickness and round from the start. In order to test the validity of the changed relation, weveral examples are given. And the measured response of each case is then compared with the predicted reponse. And it is shown that the radius is of perceptible influence on the transmission coefficient through a thick iris.

• 천문학논총
• /
• 제8권1호
• /
• pp.1-15
• /
• 1993

We made a pyramidal horn antenna system for 21cm cosmic radio wave. The antenna system has a rectangular waveguide with $TE_{10}$ mode and a copper probe to detect the electromagnetic wave in waveguide. The parameters of the probe are obtained by experiments using two waveguides. Pyramidal horn antenna is designed to get a gain of 20dB. The size of the aperture of this horn is $94cm{\times}74cm$. The beam width of half power is about $14.7^{\circ}$ for the frequency of 1.4GHz. The horn is made of aluminum plate with a thickness of 2mm. The signal from horn and waveguide is amplified in a receiver system and is converted into DC in the detecter. The intensity of the signal is recorded on a chart recorder. We observed the sun using this simple radio telescope and obtained the brightness temperature of $2.2{\times}10^5K$, which indicates that the sun is quiet at 21cm.