• 천문학회보
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• 제39권2호
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• pp.64.2-64.2
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• 2014

Interacting galaxy pairs are important for study of galaxy evolution. We selected 8,542 interacting galaxy pairs out of 593,514 KIAS-VAGC galaxy sample with 0.02 < z < 0.047 and r_mag <17.6. We then classified by their interacting features into 6 types by visual inspection. We focused on two types whose spiral tidal features extend to the center of early type galaxy (ETG) or to the edge of ETG. We compared galactic parameters of these two types with those of entire 8,542 pairs as well as between the two types. Preliminary result shows both types are very close pairs (projected distance ~ 20 kpc). Spiral galaxies in the center type are more massive but less bright than those in edge type. ETGs in the edge type are brighter but not more massive than those in the center type. The center type has a mass ratio 3.4 times greater than the edge type, but the edge type has a higher angular momentum than the center type.

• 한국환경보건학회지
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• 제24권1호
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• pp.19-23
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• 1998

This study has designed to investigate the removal effect of sewage treatment effluent by ultrafilter membrane species and then to analyze the change of pH, bacteria and E. coli., the concentration of chlorides. Ultra filtration process did not effective to remove chloride, Ca and Mg. Spiral type ultrafiltration process was more effective to remove chemical oxygen demand of sewage treatment effluent than Hollow type ultrafiltration process. The flux of spiral wound ultrafilter was higher than the hollow fiber ultrafilter.

• 천문학회지
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• 제16권1호
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• pp.1-5
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• 1983

Four HII regions of the Sd galaxy NGC 7793 were observed using AAT/IPCS. From these spectra we determined abundances of the elements using observed emission lines and electron temperatures. The calculated abundances show that this galaxy does not show any significant radial abundance gradient. The mean oxygen abundance is very much like the Orion nebulae and the nitrogen abundance is similar to the late type barred spiral galaxy NGC 1313.

• 천문학회지
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• 제22권1호
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• pp.31-41
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• 1989

Luminosity profile of the late type spiral galaxy NGC 2403 was obtained using the PDS scan of the plate. Some physical parameters (scale length, total magnitude, central brightness, disk to bulge ratio and concentric indices) were calculated from the brightness distribution. Total mass and the mass to luminosity ratio were estimated from the fitting of various mass models.

• 천문학회지
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• 제15권1호
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• pp.41-48
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• 1982

PDS was used to get the structure of two barred spiral galaxies NGC 1313 and NGC 1365. The result shows that NGC 1365 has both a deep spheroidal component and an exponential disk, but NGC 1313 has only an prominent exponential component. The luminosity profiles indicate that KGC 1313 is in type I and NGC 1365 belongs to type II. The length scales $({\alpha}^{-1})$ were derived from the exponential luminosity distributions as 1.64 kpc for NGC 1313 and 2.49kpc for KGC 1365.

• 터널과지하공간
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• 제19권3호
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• pp.181-189
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• 2009

이 연구는 지보재로서 가장 널리 사용되고 있는 록 볼트와 새로운 지보 형태인 스파이럴 볼트에 대한 지보특성을 비교하여 두 지보재의 지보효과를 평가하는데 있다. 이를 위하여 시멘트-모르타르 그라우트의 양생기간이 7일과 28일에 대한 록 볼트와 스파이럴 볼트의 실내인발시험을 실시하였으며, 각 시험결과로부터 인발하중, 변위 그리고 구속압, 내부압, 전단응력 등을 각각 구하였다. 인발하중에 대한 변위의 관계를 보면 각각의 양생기간에 대해서 스파이럴 볼트의 변위가 록 볼트에 비해 크게 나타나는데, 이것은 록 볼트의 역학적 성질이 스파이럴 볼트보다 크기 때문인 것으로 사료된다. 또한 양생기간이 길 경우 두 지보재의 변위는 거의 동일하거나 감소하는 경향을 보이는데, 그 원인은 양생기간에 따라 그라우트의 압축강도가 증가하므로 지보재와 시멘트-모르타르 그라우트 사이의 부착력이 증가하기 때문으로 사료된다. 구속압을 비교한 결과 동일한 인발하중단계에서 스파이럴 볼트의 구속압이 록 볼트보다 크게 나타났다. 이러한 사실은 같은 조건하에 있는 지반이나 암반에 지보재를 설치 할 경우 시공성 측면에서 스파이럴 볼트가 록 볼트보다 지반이나 암반의 안정성을 확보하는데 더 효과적임을 지시한다. 이상의 결과를 종합해 볼 때 같은 조건하에 있는 지반이나 암반에 지보재를 설치할 경우 새로운 형태의 지보재인 스파이럴 볼트가 기존의 지보재인 록 볼트보다 인발하중과 구속압을 더 크게 발휘하는 것으로 사료된다. 아울러, 지보재에 있어서 경제성, 현장에서의 지보재 시공성 뿐만 아니라 지보재 설치 전후의 지반이나 암반의 안정성 측면 등을 고려할 때 스파이럴 볼트가 록 볼트에 비하여 더 효과적일 것으로 판단된다.

• 한국전기전자재료학회논문지
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• 제14권6호
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• pp.518-524
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• 2001

We report the current limiting properties of superconducting fault current limiters (SFCL). Our SFCL was patterned in a spiral type on a YB $a_2$C $u_3$$O_{7-x}$(YBCO) film deposited using rf sputtering techniques and was coated with a gold shunt layer in order to disperse the heat generated at hot spots in the YBCO film. Current increased up to 13.5 $A_{peak}$ at 60 Hz for the voltage of 13 $V_{peak}$, which is the minimum quench point, and increased up to 17.6 $A_{peak}$ at 60 Hz fo the voltage fo 141.4 $V_{peak}$. The quench completion time was 5 msec at 13 $V_{peak}$ and 4 msec at 141. $V_{peak}$ respectively. we think that this architecture using spiral-type SFCL can be useful for the protection of the power delivery systems from fault currents.s. currents.s.

• Radiation Oncology Journal
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• 제8권2호
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• pp.155-162
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• 1990

마이크로파온열요법은 피부 및 국소종양에 대한 방사선과 병행요법으로서 치료성과를 얻고 있다. 저자들은 가정용 전기오븐을 이용하여 온도측정 및 조절장치를 할 수 있는 마이크로파온열기를 개발하여 적용가능한 환자를 치료하여 왔다. 그러나 선형단극 안테나로 제작된 applicator는 가열 깊이가 2\~4\;cm$로 낮고 온도분포가 불균일하여 많은 어려움이 있었다. 저자들은 안테나의 길이를 마이크로파의 파장과 같거나 배수로 하여 효율을 높게 하고 모양을 나선형으로 한 applicator를 여러개 제작하여 온열분포를 측정하였다. 안테나 길이가 파장과 같은 12.2cm이고 직경 4 cm 의 나선형모양을 가진 applicator의 온열분포가 대칭적이고 넓으며 (FWHM =3.5 cm) 보다 깊이 가열할 수 있어 ($D_{eff}=4\;cm$) 온열치료에 많은 도움을 줄 수 있다고 사료된다.

• Journal of Biosystems Engineering
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• 제12권3호
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• pp.42-49
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• 1987

The threshing action of the head-fed type threshing unit occurs mainly by the impact between threshing tooth and grains. It may be therefore the most fundamental step to calculate the time and order of the occurrance of impact by the tooth for predicting the performance of threshing unit. The threshing teeth arrangement was defined by length and diameter of threshing dram, number of spiral arrays, number of threshing teeth by kind per one spiral array, number of windings of spiral array around the threshing drum, delay angle of impact line. The linear equations for locus of left and right margin of paddy bundle, spiral array, impact line on the development figure of the threshing drum were expressed by fastors of the threshing teeth arrangement. In the computer program, the teeth which inflict impact were searched successively along the impact line. Searching range and impact condition were defined by the relation between four linear equations. If the impacting tooth was found, time and the kind of threshing tooth was derived from the coordinate of the threshing tooth. At this time the unit torque curve was accumulated on the array of computer memory. At last the completed torque curve of threshing drum shaft was described on the computer screen. Remarkably the peack valae and fluctuation of torque curve was decreased by adopting the delay angle of impact line.

• 대한설비공학회:학술대회논문집
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• 대한설비공학회 2009년도 하계학술발표대회 논문집
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• pp.774-779
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• 2009

The purpose of this research is to develop the high performance of solar chemical reactor for producing hydrogen by methane reforming reaction with steam. Two shape of chemical reactor is suggested: first type is filled with porous material and second type is spiral type. These reactors is installed on the dish-type thermal system of Inha University, Inha Dish-1. Performance analysis of these two reactors is conducted from getting methane conversion.