• 한국정밀공학회지
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• 제25권2호
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• pp.43-48
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• 2008

This paper proposes a new method for measuring the power of spherical and cylindrical lens with 6 points light source, which is composed of a LED and six holes, and magnification ellipse fitting algorithm. Each measured diagonal length of 6 points light source is determined by the target lens power. After finding the center position of each light point with threshold method, 3 axis-diagonal lengths were calculated. The long axis and short axis power of cylindrical lens can be calculated by using magnification ellipse fitting algorithm with the magnification relationships between the initial diagonal lengths and the measured diagonal lengths changed by lens power.

• 치과방사선
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• 제12권1호
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• pp.115-121
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• 1982

In the study of the focal trough of panoramic radiograph, using the Moritta compony Panex-EC a series of 48 exposures were: taken with the 6-18 brass pins placed in the holes of the plastic model plate, then eveluated by 4 observers. The author analyzed the focal trough defined by the sharpness criteria and calcuated the vertical and horizontal magnification range in the corrected focal trough. The results were as follows; 1. Continuous focal trough was not defined in the anterior region using a very high degree of sharpness. 2. As degree of sharpness used in the analysis became less, focal trough was continuous in the anterior and posterior regions, symmetrized bilaterally, and the widths of the focal trough increased more in the posterior region. e. As sharpness criteria were reduced, the percentage range of image magnification increased on both vertical and horizontal magnification, and especially the percentage range of horizontal magnification was greater than that of vertical magnification.

• 치과방사선
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• 제24권1호
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• pp.129-135
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• 1994

This study was performed to evaluate the accuracy of orthopantomogram by measuring the actual and radiographic tooth length and by analyzing the vertical magnification rate. For this study, total 90 teeth of the maxilla and mandible teeth and a dry skull were used. This experiment was attached with metal balls of 1±0.02㎜ at the root and the crown cusp tips of central, 2nd premolar, 1st molar of the maxilla and mandible and the teeth were embedded in dry skull, and then orthopantomogram was taken. The obtained results were as follows: 1. The average of tooth length in orthopantomogram was longer than that of actual tooth length. 2. The average of vertical magnification rate in the orthopantomogram to actual tooth length was 17-26%. 3. Vertical magnification rate of the maxilla teeth was 18-26% and that of mandibular teeth was 17-23%, and the magnification of maxillary teeth was larger than that of mandible teeth(P<0.0l). 4. Vertical magnification rate of posterior area was 22-26% and that of anterior area was 17-18%, and the magnification of anterior area was less than that of posterior area(P<0.01).

• 치과방사선
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• 제21권1호
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• pp.119-125
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• 1991

In the study of magnification of image in the focal trough of panoramic radiography, (Yoshida company Panoura - Eight - s), a series of 63 x-ray films were taken with the 8-19 metal pins placed in the holes of the plastic plate, measured and evaluated by 4 observes. The author analyzed the vertical and horizontal magnification rate in the corrected focal trough. Results were as follows: 1. For vertial measurements, magnification rates were minimum 10% maximum 36% and the magnification for image of medial side was larger than that of image of lateral side from image layer. 2. For horizontal measurements, magnification rates were minimum-14% maximum 46% and images of medial side from focal trough were magnified and images of lateral side from focal trough were retrenched. 3. When moved 10㎜ downward occlusal layer, interspace was somewhat narrow between the pins and upper sides of pins were horizontally magnified but images of the end parts of pins showed tapered form. 4. When moved 10㎜ downward from the occlusal layer, opposite images showed overlapping.

• 천문학회보
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• 제37권2호
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• pp.109.2-109.2
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• 2012

Current microlensing follow-up observations focus on high-magnification events because of the high efficiency of planet detection. However, central perturbations of high-magnification events caused by a planet can also be produced by a very close or a very wide binary companion, and the two kinds of central perturbations are not generally distinguished without time consuming detailed modeling (a planet-binary degeneracy). Hence, it is important to resolve the planet-binary degeneracy that occurs in high-magnification events. In this paper, we investigate caustic-crossing high-magnification events caused by a planet and a wide binary companion. From this study, we find that because of the different magnification excess patterns inside the central caustics induced by the planet and the binary companion, the light curves of the caustic-crossing planetary-lensing events exhibit a feature that is discriminated from those of the caustic-crossing binary-lensing events, and the feature can be used to immediately distinguish between the planetary and binary companions.

• 구강회복응용과학지
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• 제30권1호
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• pp.1-8
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• 2014

목적: 이 연구는 파노라마방사선사진 촬영 시 환자의 머리 위치가 상방, 하방, 좌측 및 우측으로 회전됨에 따른 수평 및 수직 확대율의 변화를 비교 평가하는 것이었다. 연구 재료 및 방법: 직경 4 mm인 금속구 5개를 건조 두개골의 하악 전치부(2개)와 우측 대구치부(3개)의 치조골 상방에 위치시켰다. 상하 및 좌우 회전량을 조절할 수 있는 두개골 고정장치에 건조 두개골을 고정시킨 후, 기준 위치와 회전된 위치에서 파노라마방사선사진을 쵤영하였다. 결과: 기준 위치에서 평균 수평 확대율은 $1.22{\pm}0.01-1.44{\pm}0.01$이었고, 평균 수직 확대율은 $1.29{\pm}0.00-1.35{\pm}0.02$였다. 전치부와 구치부 비교시 수평 확대율은 전치부에서 $1.24{\pm}0.02-1.31{\pm}0.03$, 구치부에서 $1.40{\pm}0.03-1.33{\pm}0.02$로 유의한 차이가 있었고(P < 0.05), 수직 확대율은 차이가 없었다. 위치 변화에 따른 수평 확대율은 $0.88{\pm}0.03-3.73{\pm}0.16$으로 기준 위치와 비교 시 통계적으로 유의한 차이를 보인 반면 (P < 0.05), 수직 확대율은 $1.24{\pm}0.01-1.37{\pm}0.02$로 차이가 없었다. 결론: 회전된 머리위치에서 파노라마방사선사진 촬영 시 수평 확대율의 변화가 크다.

• Archives of Plastic Surgery
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• 제40권2호
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• pp.104-108
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• 2013

Background Microsurgical techniques are considered standard procedures in reconstructive surgery. Although microsurgery by itself is defined as surgery aided by optical magnification, there are no guidelines for determining in which clinical situations a microscope or loupe should be used. Therefore, we conducted standardized experiments to objectively assess the impact of optical magnification in microsurgery. Methods Sixteen participants of microsurgical training courses had to complete 2 sets of experiments. Each set had to be performed with an unaided eye, surgical loupes, and a regular operating microscope. The first set of experiments included coaptation of a chicken femoral nerve, and the second set consisted of anastomosing porcine coronary arteries. Evaluation of the sutured nerves and vessels were performed by 2 experienced microsurgeons using an operating microscope. Results The 16 participants of the study completed all of the experiments. The nerve coaptation and vascular anastomoses exercises showed a direct relationship of error frequency and lower optical magnification, meaning that the highest number of microsurgical errors occurred with the unaided eye. For nerve coaptation, there was a strong relationship (P<0.05) between the number of mistakes and magnification, and this relationship was very strong (P<0.01) for vascular anastomoses. Conclusions We were able to prove that microsurgical success is directly related to optical magnification. The human eye's ability to discriminate potentially important anatomical structures is limited, which might be detrimental for clinical results. Although not legally mandatory, surgeries such as reparative surgery after hand trauma should be conducted with magnifying devices for achieving optimal patient outcomes.

• 천문학회보
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• 제35권1호
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• pp.48.1-48.1
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• 2010

Four of nine exoplanets found by microlensing were detected by the resonant caustic, which represents the merging of the planetary and central caustics at the position when the projected separation of a host star and a bounded planet is s~1. One of the resonant caustic lensing events, OGLE-2005-BLG-169, was a caustic-crossing high-magnification event with A_max ~800 and the source star was much smaller than the caustic, nevertheless the perturbation was not obviously apparent on the light curve of the event. In this paper, we investigate the perturbation pattern of the resonant caustic to understand why the perturbations induced by the caustic do not leave strong traces on the light curves of high-magnification events despite a small source/caustic size ratio. From this study, we find that the regions with small magnification excess around the center of the resonant caustic are rather widely formed, and the event passing the small-excess region produces a high-magnification event with a weak perturbation that is small relative to the amplification caused by the star and thus does not noticeably appear on the light curve of the event. We also find that the positive excess of the inside edge of the resonant caustic and the negative excess inside the caustic become stronger and wider as q increases, and thus the resonant caustic-crossing high-magnification events with the weak perturbation occur in the range of q $\leq$ 10-4. We determine the probability of the occurrence of events with the small excess $|\varepsilon|{\leq}3%$ in high-magnification events induced by a resonant caustic. As a result, we find that for the Earth-mass planets with a separation of ~2.5 AU the resonant caustic high-magnification events with the weak perturbation can occur with a significant frequen.

• 대한방사선기술학회지:방사선기술과학
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• 제43권5호
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• pp.331-336
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• 2020

In this study, we would like to examine the effect of the location of the magnification marker and the change in the stitching range on the magnification marker and the expansion of the anatomical structure in the examination of femoral stitching radiation using the stitching technique, and to find out the usability of the femoral stitching radiation examination in the preoperative examination for THRA. The measured values measured by 5 researchers were summed and presented through descriptive statistics. When the position of the magnification marker was changed, the average value of the measured value was in the range of 113.54 to 113.90 mm. The anatomical structures of the femur were measured in the range of 57.24 to 57.78 mm, 27.20 to 27.56 mm, and 70.11 to 70.81 mm, respectively. This showed a similar deviation from the expansion rate of previous related papers using markers. Therefore, it is considered that femoral stitching X-ray examination using magnification markers can be used for preoperative examination for THRA.

• 한국안광학회지
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• 제17권4호
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• pp.435-440
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• 2012

목적: 본 연구는 $2{\times}$ 배율을 가지는 도트사이트 장치의 개발에 관한 것이다. 방법: 무배율 도트사이트로 먼 거리를 주시할 때 목표물을 확대해서 볼 수 있도록 하기 위해 기존 무배율 도트사이트에 착탈식으로 장착할 수 있는 새로운 광학계를 개발한다. 이는 기존 무배율($1{\times}$) 도트사이트를 $2{\times}$ 배율 도트사이트로의 전환을 필요에 따라 쉽게 할 수 있도록 하기위한 것이다. 결과: 배율이 없는 도트사이트에 착탈할 수 있는, doublet 렌즈가 쌍으로 구성되는, $2{\times}$ 배율 어포칼 광학계를 설계 제작하였다. 이를 사용하였을 때 우리는 외부 목표점을 2배 확대하여 조준할 수 있어서 조준의 정확성을 더욱 높일 수 있었다. 결론: 배율이 없는 일반 도트사이트에 착탈할 수 있는 $2{\times}$ 배율 어포칼 광학계를 설계 제작할 수 있었다. 이것에 의해 외부 목표점을 2배 확대하여 조준할 수 있도록 함으로서 조준의 정확성을 더욱 높일 수 있게 되었다.