• 한국해안·해양공학회논문집
• /
• 제22권6호
• /
• pp.374-386
• /
• 2010

최근 슬리트케이슨제와 같은 유공방파제의 파랑제어특성에 대한 이론적 실험적 연구가 활발히 진행되고 있다. 본 연구에서는 규칙파의 작용하에 슬리트케이슨에 의한 반사율의 특성과, 전면유공부 및 유수실의 내부벽면에 작용하는 파압을 2차원 및 3차원수치파동수로에서 각각 추정하고, 그 결과를 검토하였다. 수치실험에서는 주기 7초, 9초, 11초 및 13초와 각각의 주기에 대해 파형경사 0.02, 0.03 및 0.04를 갖는 입사파고의 수치실험안을 설정하였고, 본 연구에서 사용된 2차원 및 3차원의 수치해석은 Navier-Stokes운동방정식에 기초한 이상류(이상류(二相流)) 수치 모델로서, 이는 타해석기법에 비해 복잡한 수면변동에 대한 물리현상을 쉽게 재현할 수 있으며, 수치프로그램의 구성이 보다 간략하게 되는 장점이 있다. 실험결과에 의하면, 반사율에 있어서 주기가 짧은 경우에는 2차원해석이 상당히 큰 값을 나타내지만, 주기가 길어지고 파형경사가 큰 경우에는 2차원해석과 3차원해석의 결과가 거의 동일한 값을 나타낸다. 파압에 있어서 주기가 짧은 경우에는 두 해석법에서 차이는 작지만, 주기가 길어지고 파형경사가 큰 경우에는 차이가 크게 나타나는 경향을 확인할 수 있었다.

• 복식
• /
• 제61권7호
• /
• pp.67-79
• /
• 2011

This study is to design a ball-jointed doll costume with historical research in clay female doll's costume from Hwangsung-dong tomb of the Silla Dynasty[新羅] in 7C. This clay female doll's costume was characterized by slim silhouette, long sleeves, no neckline, side slit, high waistline, and bun on the back neck of representative of the early era. According to literature of 7-8C and textile relics, it is presumed that she wore short Jeogori[短衣, Dan-eui] with long sleeves and two layered skirt, and Dan-ryeong(團領) could be added as attachment that is reflective of the time era. For making design costume, Ra[羅, silk gauze] was used for long Dan-ryeong, plain silk and brocade[錦, Geum] for Dan-eui and skirt as a special textile of this period. Waist dart and small snap were added to the costume of ball-jointed doll because of hardness and curvy shape of doll's body, without contradicting traditional value. For better use of this study and cost reduction purposes, development of production system for traditional doll costumes should be considered.

• 한국의류산업학회지
• /
• 제19권4호
• /
• pp.385-399
• /
• 2017

This study will broaden the application of doll costume product with historical characteristics and the image of unlined cheollik in the $17^{th}$ century period of transition during the Joseon Dynasty. Historical design sources were extracted from old documents and precedent studies. Unlined cheollik of Shin Gyeong-yu, meritorious retainer, were selected as main reference-relic because of various fabric, preserved conditions and definite shape. 'Baby doll' was selected as main model because of consumer preferences and awareness. Design sources from unlined cheollik in the early $17^{th}$ century were about a 1:2 ratio of upper and under parts, removable separated doori-somae, knife-shaped collar (outside), projected square collar (inside), long pleats line, side slit, traditional flat fell seam sewing. Trapezoidal side line, round waistline, and thin fabric were applied in designs because of toddler-body of doll model. Three designs were produced in step 1: Cheollik A focusing on the historical remake (traditional type), Cheollik B with belt and side slit (crossover type), and Cheollik C with back- opening (modern type). In step 2, interview with fashion major student was conducted to increase the utility of designs. As a result, modern trend sources (frill, velcro, round armhole line, slope of sleeves, and floral pattern) were reflected in Cheollik B, C. Finally, three doll cheollik and cheollik-styled doll apron sample were produced. Various versions must be suggested in the study of doll costume products with traditional sources that balance historical characteristics and practicality to improve customer satisfaction.

• 천문학논총
• /
• 제21권2호
• /
• pp.51-59
• /
• 2006

We have successfully developed the KASI (Korea Astronomy and Space Science Institute) Solar Imaging Spectrograph (KSIS), which has been originally upgraded from the KASI solar spectrograph that was able to record solar spectra for a given slit region and to inspect the response function of narrow band filters. A prototype KSIS was developed in 2004 by using a scanning mirror in front of the spectrograph slit and a SBIG ST-8XE CCD camera. Its main disadvantage is that it took a long time (about 13 minutes) to scan a whole active region. In this work, we have upgraded the KSIS by installing a much faster Dalsa 1M15 CCD camera, which gives a data acquisition time of about 2.5 minutes. The software for KSIS was also improved for the new CCD camera on the basis of component-based development method. We have successfully made a test observation for a simple and small active region (AR10910) using the improved KSIS system. Our observations show that H-alpha images for several wavelengths have typical features in a sunspot as well as a H-alpha centerline image is quite similar to a BBSO H-alpha image, demonstrating the capability of the KSIS system.

• 복식문화연구
• /
• 제17권5호
• /
• pp.886-896
• /
• 2009

Acjurumpo is one of the most representatives daily outfit of Joseon Dynasty is a clothes which has a characteristic of having creases under the armhole and it has a lot of chance to use on modern clothes design. This study wants to provide a information on traditional clothes to the public and modernize traditional clothes by designing modern women clothes by adapting Acjurumpo, one of Joseon Dynasty's men' daily outfit which is not very well-known to publics as a link of traditional clothes modernization. Acjurumpo's characteristic is usually having a knife-shape collar and having two sup and one sup, but outside sup of having two sup was more common. There were tongsu, duri, as a example of shape of sleeve. For Mu the combinations were different from Acjurum starting with a shape of trapezoid, triangle to big Mu on a body of side line. For Gorum there were two pairs of long and short Gorum, two pairs of short Gorum or one pair of short or long Gorum. Slit of po was on both side or back. Acjurumpo which was adapted on modern clothes, it was usually used on Hanbok companies that used traditional shape or similar shape to design children' clothes. This study designed three summer one-piece and two winter jacket for women clothes adapting Acjurumpo. And it was designed by using modern material adapting Acjurumpo's characteristics, changing knife-shape collar, Acjurum, mu and Gorum. This study expects for popularization of many traditional clothes developed by modern design in future.

• Parasites, Hosts and Diseases
• /
• 제60권6호
• /
• pp.419-421
• /
• 2022

To improve our understanding of the migration of sparganum in humans, we report a case of ocular sparganosis having the migratory episode from the muscle cone to the subconjunctiva. A 34-year-old woman was admitted to the Hospital of Anhui Medical University (Hefei, China), in December 2019. She presented with conjunctival hemorrhage and recurrent pain in the left eye. A foreign body was found in the muscle cone of the eye. Two months later, a ribbon-like white material was found under the conjunctiva on slit-lamp examination. A long and slender, actively moving parasite was extracted by surgery. The extracted worm was approximately 8 cm long and 2 mm wide. The worm was whitish, wrinkled, ribbon shaped, and had a slightly enlarged scolex. The worm sample was morphologically identified as a plerocercoid larva (sparganum) of the Spirometra tapeworm. Her conjunctival blood suffusion and eye pain ceased within 1 week after operation. She has been in good health without any symptoms during the 2-year follow-up. A case of ocular sparganosis, in which larval worm migrated from the muscle cone to the subconjunctiva is reported from China.

• 천문학논총
• /
• 제12권1호
• /
• pp.167-172
• /
• 1997

Detailed low spectral resolution observations of the spectrum have been made for three early spectral type standard stars, HR718, HR1544, HR3454, respectively, for the wavelength region 4,300 A to 7,500 A, using the Bohyunsan Optical Astronomy Observatory (BOAO) Middle- Dispersion Spectrograph. These standard stars were chosen from well-known bright northern standard stars. All of the observed long slit spectral data has been reduced and analyzed using the IRAF reduction procedure. The derived extinction coefficients are compared with the other observatory result. The derived value can be used in the determination of flux calibration of BOAO spectroscopic observation. However, until the high quality data are secured from a new series of observation in the blue region and are re-analyzed together, the extinction coefficients below the 4,000 A wavelength remains unknown.

• 천문학회보
• /
• 제40권1호
• /
• pp.78.4-79
• /
• 2015

We present the spatially resolved kinematics of ionized gas and stars along the major axis of 9 pseudo bulge galaxies. Using the high quality long-slit spectra obtained with the FOCAS at the Subaru telescope, we measured the flux, velocity, and velocity dispersion of the [OIII] and $H{\beta}$ lines to determine the size of the narrow-line region, rotation curve, and the radial profile of velocity dispersions. We compare ionized gas kinematics and stellar kinematics to investigate whether ionized gas shows any signs of outflows and whether stars and ionized gas show the same sigma-dip feature (i.e., decrease of velocity dispersion) at the very center.

• 천문학논총
• /
• 제22권2호
• /
• pp.35-41
• /
• 2007

We present the result of radial velocity observation of a W UMa type binary star EX Leo. We observed the star on February 16, 2003, using Long-Slit spectrograph of BOAO(Bohyunsan Optical Astronomical Observatory). Since the spectral lines are broad due to its fast rotation, it is difficult to distinguish two radial velocities from cross correlation function. Instead of cross correlation function, we used broadening function to develop our own code which estimate the radial velocity of the broadened line spectra. With our own code, radial velocities of primary and secondary stars are derived simultaneously. From the radial velocity curve fit, we obtained $K_1=50.24{\pm}8.29km/s$ and $K_2=254.05{\pm}20.984km/s$ respectively.

• Journal of Astronomy and Space Sciences
• /
• 제12권1호
• /
• pp.1-13
• /
• 1995

We carried out photometric and spectroscopic observatious of the blue compact dwarf galaxy Haro 6 in the Virgo Cluster of Galaxies. The long-slit spectroscopy was employed at three position angles, $\Phi$=$0^{\circ}$, $\Phi$=$30^{\circ}$, and $\Phi$=$120^{\circ}$with CCD camera mounted on the Cassegrain Spectrograph. Based on the mean intrinsic axial ratio < $q_0$ >=0.3, we derived inclination I of the system as $44^{\circ}$using our composite V-band CCD image. Careful analysis on the velocity field of the system shows an asymptotically fiat rotation curve with the maximum rotational velocity $V(r)_{max}$ reaches about 12km/sec. The calculation of the dynamical mass of Haro 6 with a simple mass model is briefly discussed with emphasis on the mass to luminosity ratio. From the IRAS Point Source Cataloque, we derived dust-to-gas ratio which indicates relatively low dust content, thus tempting us to conjecture the youth of the system.