• Title/Summary/Keyword: Stars

Search Result 1,611, Processing Time 0.027 seconds

A Study on the Pop Music and Fashion (팝 음악과 패션에 관한 연구)

  • 김미정;이상례
    • Journal of the Korean Society of Costume
    • /
    • v.53 no.2
    • /
    • pp.101-118
    • /
    • 2003
  • This paper describes pop stars' fashion style by the changes of pop music from the 1950's of the formative Period of a rock-n-roll to the 1990's. The author could examine the features of pop music as follows : the 1950's rock-n-roll, the 1960's rock and Psychedelic rock. the 1970's punk rock, the 1980's new wave and the 1990's reggae·hip-hop. Based on the examination, the author could do sampling of the fashion style, on which current pop music had influence, by rock style, new wave style, and reggae hip-hop style. The rock style makes appearance again as a new style when it is recently accepted to be a fashion. The 1960's hippie, which contains long-cherished desire of antiwar and peace after September 11, 2001 Attack on America and the Afghan War. reappeared as luxurious hippie, and the hybrid punk has been made because barriers between cultures have been collapsed to mix items and combine contradicting components at fashion field. The new wave style destroys sex difference of clothes. and men's clothes style has introduced women's dress style, so that androgynous style, which has handsome boy image with womanlike hair style and makeup, and the lingerie style without distinction of underwear and outer garment has made appearance through new cloth wearing ways and overexposure. The reggae and hip-hop style makes appearance to overcome social strata, groups, ages, regions and gender, etc and become one of the 21s1 century culture codes. In conclusion, pop music have played very important roles until expansion and popularity of new fashion style, and has been quickly expanded by mass media development. When the pop music fashion styles are introduced to high fashion, fashion styles have become more polished and high-qualify to expand them at main fashion world again.

A Study on the Effect of Popular Culture in Modern Fashion -Focused on the Fashion Icon- (현대 패션에 나타나는 대중문화의 영향에 관한 연구 -Fashion Icon을 중심으로-)

  • Kim, Young-Sam
    • Journal of the Korean Society of Costume
    • /
    • v.56 no.7 s.107
    • /
    • pp.58-67
    • /
    • 2006
  • This study of popular culture is in based on an academic point of view and based thereon an investigation of popular culture from a fashion standpoint follows. This study is to suggest that the popular culture theory can be a basic framework to examine the characteristics of fashion Icon and to verify that the characteristics of Fashion Icon is similar to the codes of the popular culture of today, This study considers the characteristics of popular culture as commercialism, mass-media relationship and a symbolic interaction. The images of movie stars projected through diverse entertainment media are the very fashion icons and strong role models that are copied by consumers. Now, the public take the lead in cultural industry, and they create new images as positive receivers of the images of fashion icons, not as mere imitators or followers. Fashion irons have contributed to diversifying the styles of ideal feminine beauty, and their lift pattern and image are one of the major sources to stir up the imagination and inspiration of people. Thus, the times, fashion and entertainment media have continued to evolve, closely affecting one another, and fashion icons play a role of fashion leader, through entertainment media, who takes the initiative in mass fashion without just being confined to the field of entertainment. This study meaningful from the aspect that discussion of popular culture has been placed in a position that recognizes the entity of and interest in popular culture. through this study, I hope that the scope of interest in Fashion design will expand and that approaches to popular culture will become more diversified.

An Investigation in the Thermal Effect on a Low Earth Orbit Satellite under Yaw Motion for the Visibility of a Star Sensor (저궤도 위성에서 별센서의 가시성을 위한 Yaw Motion에 따른 열적 영향 고찰)

  • Kim, Hui-Kyung;Lee, Jang-Joon;Hyun, Bum-Seok
    • Journal of the Korean Society for Aeronautical & Space Sciences
    • /
    • v.37 no.7
    • /
    • pp.709-716
    • /
    • 2009
  • Thermal condition according to the operation attitude of a satellite in orbit would be essential to be known because the orbit attitude is a dominant factor to affect satellite thermal design. In this paper, the change in space thermal environment and the thermal effect in thermal design are studied for a low earth orbit satellite according to the yaw motion. The present satellite retains sun-pointing attitude during daylight due to the fixed type solar arrays. And it also moves along the orbit with constant yaw motion in a longitudinal axis so that a star tracker which is a star sensor for satellite's attitude control always looks into the deep space. This attitude is considered in its better visibility to the stars for a successful mission operation. Also, it is required to access the corresponding thermal effects due to the yaw motion. Therefore, we try to verify these by the thermal analysis for the satellite thermal model with the yaw motion.

A Comparison Study on the Effect Size According to the Type of Fandom Activities : Based on Meta-analysis (팬덤활동의 유형에 따른 효과크기 비교 연구: 메타분석 기반)

  • Kim, Jhong-Yun;Kim, Eun-Bee
    • Journal of the Korea Convergence Society
    • /
    • v.11 no.6
    • /
    • pp.259-268
    • /
    • 2020
  • The purpose of our study is to conduct a general·quantitative analysis of fandom activities and verify their organization types and effects. The results are as follows. With regard to the comparison of effect size, the variable related to the social and economic field showed the greatest effect size, which was followed by individual behavior and individual mentality. In terms of influential factors of fandom activities, the effect size of positive variables was intermediate level while the effect size of negative variables was low level. In addition, the effect size of fandom supporting idol groups was the greatest, which was followed by of fandoms supporting sports stars, and actors. In terms of the effect size with regard to the influence on fandom among the objects of study, the effect size of university students was the greatest, which was followed by the whole, adult, middle and high school student, and middle school student. Meanwhile, the result of the analysis according to the classification by country showed that China had the greatest effect size, and the US also showed quite a big effect size. On the other hand, South Korea showed a low level of effect size.

On the Application of the Islamic Patterns to the Textile Design (이슬람 예술에 표현된 패턴 특징과 텍스타일디자인에의 활용)

  • 김희선
    • Journal of the Korea Fashion and Costume Design Association
    • /
    • v.6 no.1
    • /
    • pp.13-24
    • /
    • 2004
  • This study was analyzed three basic patterns of the Islamic arts. These are natural flora, geometrical and calligraphy pattern. Islamic belief in Aniconism, doctrine of unity and worship of arabic language demanded delicate, decorative, and abstract patterns instead of patterns of real image. Natural flora pattern was classified into arabesque and various flower patterns. Muhammad commands that "The artist who fashions a representation of living things is competitor of God and therefore destined to eternal damnation, so if you want to represent living things, you should only depict flowers and trees". Then the natural flora patterns developed into main Islamic pattern. Geometric pattern was composed of geometrical elements like, circle, trigon, square, rectangle, pentagon, hexagon, octagon or other polygons, stars or motifs with straight or curved lines. Circle symbolized ′celestial′ sphere and crystal of the lower octagon symbolized ′earthly existence′. Therefore if the circle join with the octagons, it means fusion of celestial and earthly existence. Another important influence on the Islamic art was the calligraphy pattern, the writing of Arabic language. The major language of calligraphy pattern was Arabic script and often Persian script. Calligraphy pattern was composed of Kufic and Cursive script. The cursive script was developed various forms. The Islamic tenet prohibit depiction of sacred images, the sacred Arabic calligraphy such as ′Alla′ or ′Mohammad′ was substituted of them. And the content of calligraphy pattern was used with Quranic phrases. The aesthetics of Islamic patterns analyzed aesthetic of ′rhythmic lines′, aesthetic of ′unity in multiplicity′, aesthetic of tessellation and aesthetic of harmony. On the textiles of the Islamic culture, the arabesque, floral, geometric and calligraphy patterns were frequently used.

  • PDF

Characteristics of Korean Dramas Favored by Chinese Viewers -Focused on Internet Bulletin Boards- (중국인들이 선호하는 한국 드라마의 특성 -인터넷 게시판에 나타난 시청의견을 중심으로-)

  • Lee, Moon-Haeng
    • The Journal of the Korea Contents Association
    • /
    • v.11 no.6
    • /
    • pp.167-175
    • /
    • 2011
  • Increased numbers of Chinese are using the Internet as communications technology develops, and more Chinese are downloading and watching Korean dramas and movies. According to a survey conducted to assess the present state of Korean wave in China, most Chinese young people are watching Korean dramas by downloading them from the Internet. The objective of this study is to see the characteristics of Korean dramas preferred by Chinese viewers: the factors are years of production, diffusers(Broadcasters), types of drama, story topics, main actors, and directors. As a result, Chinese viewers tend to prefer to dramas recently diffused in Korea, miniseries, and comic dramas and romance. Otherwise, broadcasters, main actors, and directors do not influence directly on the choice of dramas of Chinese. Particularly, Korean wave stars in China do not always appear into the dramas favored by Chinese viewers.

SENSITIVITY CALIBRATION OF FAR-ULTRAVIOLET IMAGING SPECTROGRAPH (원자외선 분광기(FIMS)의 감도 측정)

  • Kim, I.J.;Seon, K.I.;Yuk, I.S.;Nam, U.W.;Jin, H.;Park, J.H.;Ryu, K.S.;Lee, D.H.;Han, W.;Min, K.W.;Edelstein Jerry;Korpela Eric
    • Journal of Astronomy and Space Sciences
    • /
    • v.21 no.4
    • /
    • pp.383-390
    • /
    • 2004
  • We describe the in-flight sensitivity calibration of the Far ultraviolet Imaging Spectrograph (FIMS, also known as SPEAR) onboard the first Korean science satellite, STSAT-1, which was launched in September 2003. The sensitivity calibration is based on a comparison of the FIMS observations of the hot white dwarf G191B2B, and two O-type stars Alpha-Cam, HD93521 with the HUT (Hopkins Ultraviolet Telescope) observations. The FIMS observations for the calibration targets have been conducted from November 2003 through May 2004. The effective areas calculated from the targets are compared with each other.

The BV Photometry of the RR Lyrae Star, BH Ursae Majoris: Light Curves and Period Study

  • Kim, Chun-Hwey;Jeong, Jang-Hae
    • Journal of Astronomy and Space Sciences
    • /
    • v.28 no.2
    • /
    • pp.109-116
    • /
    • 2011
  • The first presented BV light curves of BH UMa confirmed Krajci's (2005) result that BH UMa is an RR Lyr star that belongs to the RRc subgroup. The light curves showed a slight asymmetry of D = 0.453 with an amplitude of about $0.^m58$ in B, $0.^m47$ in V, and $0.^m11$ in B-V and with a small hump between $0.^p82$ and $0.^p86$. We determined nine new times of minimum light and eight times of maximum light. We also analyzed all of the available unanalyzed minimum timings and found for the first time that the period of BH UMa has varied dramatically in at least three independent sinusoidal ways superposed on a secularly downward parabola over 66 years. The secular period decreasing rate was obtained as $6.^d684{\times}10^{-8}y^{-1}$, corresponding to -0.58 s/century. The semi-amplitude and period for each of the three sinusoidal variations were ($0.^d058$, $14.^y44$), ($0.^d044$, $9.^y98$), and ($0.^d005$, $0.^y97$), respectively. It is uncertain whether the periodicity for the shortest period of $0.^y97$ is real or spurious. The secular period decrease, well consistent with those of the other RRc stars, could be considered as a natural result of the evolution of the BH UMa system. The two possible sinusoidal terms were interpreted as both two light-time effects due to two additional bodies orbiting BH UMa and combinations of random fluctuations in the pulsation period of BH UMa. Two interpretations were shortly discussed with related parameters.

An Analysis of the Social-Cultural Meaning of Korean Girl Groups' Appearances -Focusing on the Change of Girl Groups' Appearances across Generations- (국내 걸그룹 외모에 나타난 사회문화적 의미 분석 - 세대별 걸그룹 외모 변화를 중심으로 -)

  • Han, Cha-young
    • Journal of Fashion Business
    • /
    • v.21 no.1
    • /
    • pp.12-31
    • /
    • 2017
  • Korean commercial-organized girl groups were remarkable in the late 1990's. However, by the late 2000's, girl groups had an even more profound effect on Korean popular music compare to past influences. This study aimed to analyze the social-cultural meaning of the changing appearance of girl group between the first and second-generations. For this purpose, this study analyzed media image and text, based on a social-cultural context, about 13 girl groups. The results are as follows. First, while the first -generation girl group tended to maintain girlish/sexy images trying to the male desire, the second -generation girl group strategically showed various sexual identities such as femininity, masculinity, masculinity and androgyny along with contextual sexual images. The reason why girl groups increased the number of strategic images featuring various sexual identities was in order to appeal to a wide, diverse audience. Second, the second generation girl groups had - slim bodies with great athleticism, basically due to trainee system. Because of this, their semiotic body images have been commercially used to promote the consumption. Third, the second generation girl groups - were the bigger stars than first generation girl groups - because the members worked in many different fields. Therefore, the group members' images were successful consumed directly and then reproduced symbolically. Fourth, each member of the second -generation girl groups characterized by appearing in diverse, yet familiar images, through various media sources. Although the intention of this was to have recognition and popularity, it became difficult for them to change their image once one particular image was deemed popular.

Modeling Gamma-Ray Emission From the High-Mass X-Ray Binary LS 5039

  • Owocki, Stan;Okazaki, Atsuo;Romero, Gustavo
    • Journal of Astronomy and Space Sciences
    • /
    • v.29 no.1
    • /
    • pp.51-55
    • /
    • 2012
  • A few high-mass X-ray binaries-consisting of an OB star plus compact companion-have been observed by Fermi and ground-based Cerenkov telescopes like High Energy Stereoscopic System (HESS) to be sources of very high energy (VHE; up to 30 TeV) ${\gamma}$-rays. This paper focuses on the prominent ${\gamma}$-ray source, LS 5039, which consists of a massive O6.5V star in a 3.9-day-period, mildly elliptical ($e{\approx}0.24$) orbit with its companion, assumed here to be an unmagnetized compact object (e.g., black hole). Using three dimensional smoothed particle hydrodynamics simulations of the Bondi-Hoyle accretion of the O-star wind onto the companion, we find that the orbital phase variation of the accretion follows very closely the simple Bondi-Hoyle-Lyttleton (BHL) rate for the local radius and wind speed. Moreover, a simple model, wherein intrinsic emission of ${\gamma}$-rays is assumed to track this accretion rate, reproduces quite well Fermi observations of the phase variation of ${\gamma}$-rays in the energy range 0.1-10 GeV. However for the VHE (0.1-30 TeV) radiation observed by the HESS Cerenkov telescope, it is important to account also for photon-photon interactions between the ${\gamma}$-rays and the stellar optical/UV radiation, which effectively attenuates much of the strong emission near periastron. When this is included, we find that this simple BHL accretion model also quite naturally fits the HESS light curve, thus making it a strong alternative to the pulsar-wind-shock models commonly invoked to explain such VHE ${\gamma}$-ray emission in massive-star binaries.