戦後思想が残したものと消費社会の可能性 - 吉本隆明 · 埴谷雄高の『anan』をめぐる論争を通して-

貞包英之(Sadakane, Hideyuki) 동아시아일본학회 2024 일본문화연구 Vol.- No.90

본고는 요시모토 다카아키와 하니야 유타카라는 두 사상가가 일본 사회의 소비사회화에 어떻게 대응했는지를 살펴봄으로써, 패전으로 인해 형성된 일본의 전후 사상의 과제가 어떻게 해결되었는지, 어떻게 해결되지 않았는지에 대해 밝힐 것이다. 요시모토와 하니야는 국가의 극복을 전후 사상의 과제로 받아들인다. 우익적 지향이든 좌익적 지향이든 국가와 이를 구성하는 권력을 보존하며 20세기가 가져온 비참함에 대응할 수 없다고 본 것이다. 그러나 그러한 과제에 대해 요시모토는 1980년대 소비사회화로 해결의 길이 열렸다고 본 반면, 하니야는 그렇지 않다고 보고 두 사람은 결별한다. 특히 여성 패션잡지『anan』을 둘러싸고 문제가 되었는데, 하니야가 거기서 국가 자본주의의 작동을 본 반면, 요시모토는 국가의 틀을 넘어선 사적 욕망의 전개를 보았다고 평가한다. 하지만 요시모토도 그러한 사적 욕망의 전개 자체가 사람들을 여전히 사회적 권력 관계속에 묶어두는 것으로 보지는 않았다. 본론은 요시모토와 하니야의 사상의 한계와 가능성을 밝히는 것을 통해 전후 사상 속에서 어떤 문제가 현대에도 여전히 유효한지 살펴본다. This article clarifies how the issues of Japanese postwar thought shaped by the defeat in World War II were resolved and how they were not resolved by examining how two thinkers, Takaaki Yoshimoto and Yutaka Haniya, responded to the transformation of Japanese society into a consumer society. Yoshimoto and Haniya believed that postwar thought must aim above all else to transcend the state. They analyzed that neither the right nor the left could cope with the misery of the 20th century by preserving the state and its interwoven powers. However, while Yoshimoto believed that the “consumer society” of the 1980s had provided a solution to this problem, Haniya believed otherwise, and the two fell out. The issue was particularly related to the womens fashion magazine “anan”. While Haniya assumed that state capitalism was still in operation in that magazine, Yoshimoto saw in it the development of private desires that transcended the state and evaluated it highly. Yoshimoto, however, ignored the fact that the development of such private desire itself binds people to social power relations. This paper investigates what issues in postwar thought are still active today by clarifying the limits and possibilities of Yoshimotos and Haniyas thinking.

A Spectroscopic Abundance Study of Dwarf Cepheid V1719 Cygni

Kim, Chulhee,Kozo-Sadakane 한국우주과학회 1992 한국우주과학회보 Vol.1 No.1

DOUBLE PEAKED OUTBURSTS OF THE BLAZAR OJ 287 IN 1994 - 1996

ARIMOTO JUN'ICHI,SADAKANE Kozo,HONDA SATOSHI,TANABE KAZUHITO The Korean Astronomical Society 1996 Journal of The Korean Astronomical Society Vol.29 No.suppl1

VRI bands CCD photometric observations of the BL Lac object OJ 287 have been carried out during the period from October, 1994 to May, 1996. OJ 287 underwent two major outbursts during our observations. The first peak (V14.0 mag.) occurred in the first half of November, 1994 and faded out to 16.5 mag within 150 days. The second peak (14.0 mag.) was observed in late December, 1995. The latter peak continued at nearly the same brightness until May, 1996. Such a long lasting outburst has never been reported for OJ 287. Color indices (V - R and V-I) remained nearly constant during the outbursts.

PULSATIONAL CHARACTERISTICS OF V1719 CYGNI WITH PECULIAR LIGHT CURVE

KIM CHULHEE,KIM SEUNG-LI,SADAKANE KOZO The Korean Astronomical Society 1993 Journal of The Korean Astronomical Society Vol.26 No.2

The light curve and radial velocity curve of multiperiodic dwarf cepheid VI719 Cyg (HD200925) with peculiar light curve have been reanalyzed in order to identify the oscillation modes to confirm the helium settling within the envelope. To do these, through the period search for the photometric and radial velocity data from the literature, two different periods were determined and the oscillation modes corresponding to the first and second periods were identified as the fundamental and first radial overtones. Hence the helium settling within the envelope was confirmed from the period ratio. The color excess, metallicity, effective temperature, and surface gravity corresponding to two different modes were determined and it was found that these parameters almost do not depend upon different oscillation mode. By utilizing the surface brightness method, we investigated the variation of angular diameter and radial displacement and it was found that the angular variation is very peculiar. Also by referring to the stellar models, mass and age were determined as $2.7M_{\bigodot}$ and 0.42 Gyr respectively which make this variable star heavier and younger than other multimode dwarf cepheids. Preliminary spectroscopic CCD observations were carried out and it was found that Mg in VI719 Cygni is nearly solar abundent according to the analysis of $5172.68{\AA}MgI$ line which is inconsistent with the photometric result. It was suggested that VI719 Cyg may be classified as a $\rho$ Pup stars according to the photometric characteristics.

PULSATIONAL CHARACTERISTICS OF V1719 CYGNI WITH PECULIAR LIGHT CURVE

KIM, CHULHEE,KIM, SEUNG-LI,SADAKANE, KOZO 全北大學校 基礎科學硏究所 1994 基礎科學 Vol.16 No.-

The light curve and radial velocity curve of multiperiodic dwarf cepheid V1719 Cyg(HD200925) with peculiar light curve have reanalyzed in order to identify the oscillation modes to confirm the hellium sattling within the envelope. To do these, through the period search for the photmetric and radial velocity data from the literature, two different periods were determined and the oscillation modes corresponding to the first and second periods were identifed as the fundamental and first radial overtones. Hence the helium settling within the envelope was confirmed from the period ratio. The color excess, metallicity, effective temperature, and surface gravity corresponding to two different modes were determined and it was found that these parameters almost do not depend upon different oscillation mode. By utilizing the surface brightness method, we investigated the variation of angular diameter and radial displacement and it was found that the angular variation is very peculiar. Also by referring to the stellar models, mass and age were dtermined as 2.7M_?? and 0.42 Gyr respectively which make this variable star heavier and younger than other multimode dwarf cepheids. Preliminary spectroscopic CCD observations were carried out and it was found that Mg in V1719 Cygni is nearly solar abundent according to the analysis of 5172.68ÅMgI line which is inconsistent with the photometric result. It was suggested that V1719 Cyg may be classified as a ρ Pup stars according to the photometric characteristics.

Initial Report for the Radiation Effects Research Foundation F1 Mail Survey

Milder, CM,Sakata, R,Sugiyama, H,Sadakane, A,Utada, M,Cordova, KA,Hida, A,Ohishi, W,Ozasa, K,Grant, EJ Asian Pacific Journal of Cancer Prevention 2016 Asian Pacific journal of cancer prevention Vol.17 No.3

To study the full health effects of parental radiation exposure on the children of the atomic bomb survivors, the Radiation Effects Research Foundation developed a cohort of 76,814 children born to atomic bomb survivors (F1 generation) to assess cancer incidence and mortality from common adult diseases. In analyzing radiation-associated health information, it is important to be able to adjust for sociodemographic and lifestyle variations that may affect health. In order to gain this and other background information on the F1 cohort and to determine willingness to participate in a related clinical study, the F1 Mail Survey Questionnaire was designed with questions corresponding to relevant health, sociodemographic, and lifestyle indicators. Between the years 2000 and 2006, the survey was sent to a subset of the F1 Mortality Cohort. A total of 16,183 surveys were completed and returned: 10,980 surveys from Hiroshima residents and 5,203 from Nagasaki residents. The response rate was 65.6%, varying somewhat across parental exposure category, city, gender, and year of birth. Differences in health and lifestyle were noted in several variables on comparison across city and gender. No major differences in health, lifestyle, sociodemographics, or disease were seen across parental exposure categories, though statistically significant tests for heterogeneity and linear trend revealed some possible changes with dose. The data described herein provide a foundation for studies in the future.

Bladder cancer risk in the Life Span Study of atomic bomb survivors : An updated analysis

Jaeyoung Kim,Kotaro Ozasa,Dale Preston,Kiyohiko Mabuchi,Hiromi Sugiyama,Atsuko Sadakane,Ritsu Sakata,Eric Grant 대한방사선방어학회 2017 대한방사선방어학회 학술발표회 논문요약집 Vol.2017 No.11

PRIMARY BLACK HOLE SPIN IN OJ 287 AS DETERMINED BY THE GENERAL RELATIVITY CENTENARY FLARE

Valtonen, M. J.,Zola, S.,Ciprini, S.,Gopakumar, A.,Matsumoto, K.,Sadakane, K.,Kidger, M.,Gazeas, K.,Nilsson, K.,Berdyugin, A.,Piirola, V.,Jermak, H.,Baliyan, K. S.,Alicavus, F.,Boyd, D.,Torrent, M. Ca American Astronomical Society 2016 ASTROPHYSICAL JOURNAL LETTERS - Vol.819 No.2

<P>OJ 287 is a quasi-periodic quasar with roughly 12 year optical cycles. It displays prominent outbursts that are predictable in a binary black hole model. The model predicted a major optical outburst in 2015 December. We found that the outburst did occur within the expected time range, peaking on 2015 December 5 at magnitude 12.9 in the optical R-band. Based on Swift/XRT satellite measurements and optical polarization data, we find that it included a major thermal component. Its timing provides an accurate estimate for the spin of the primary black hole, chi = 0.313 +/- 0.01. The present outburst also confirms the established general relativistic properties of the system such as the loss of orbital energy to gravitational radiation at the 2% accuracy level, and it opens up the possibility of testing the black hole no-hair theorem with 10% accuracy during the present decade.</P>

선회중 전복한 저건현 내항 탱커의 복원성에 관한 연구 (1)

孔吉永(Gil-Young Kong),金喆承(Chol-Seong Kim),定兼廣行(Hiroyuki Sadakane) 한국항해항만학회 2002 한국항해항만학회지 Vol.26 No.1

전복한 저건현 내항 탱커의 사고 원인을 조사하기 위하여 복원성에 영향을 미치는 자유표면영향과 저건현 선박에서 발생하는 해수침입, 침수침하 현상에 대하여 알아보았다. 그리고 선회시에 발생하는 경사 모멘트를 계산하고 사고 선박의 경사 모멘트를 추정하였다. 이상의 결과로부터 사고 선박의 복원성 상실에 의한 전복 원인을 고찰하였다. A coastwise chemical tanker sailing at full speed has capsized in calm water and wile turing. We investigate reasons of the accident and demonstrate that a proper correction for the free surface effect of the liquid cargo has not been practiced in the initial design stage and that the bow-sinkage induced in sailing has weakened the form stability of the ship. It is also shown that the liquid cargo shift occurring in turning generated a significant outward heel moment.

Preliminary diagnosis of medial meniscus posterior root tears using the Rosenberg radiographic view

( Yuya Kodama ),( Takayuki Furumatsu ),( Yusuke Kamatsuki ),( Takaaki Hiranaka ),( Tomohiro Takahata ),( Masayuki Sadakane ),( Haruhiko Ikuta ),( Masaharu Yasumitsu ),( Toshifumi Ozaki ) 대한슬관절학회 2019 대한슬관절학회지 Vol.31 No.1

Purpose: To verify the effectiveness of detecting medial meniscus posterior root tears (MMPRTs) using weightbearing posterior-anterior (PA) radiographs. Materials and methods: Twenty-three patients were diagnosed with an MMPRT using magnetic resonance imaging (Group A), with 23 matched individuals forming the control group (Group B). The distance between medial tibial eminence and the lateral edge of the medial femoral condyle (MTE-MFC distance) and medial joint space (MJS) width were measured on weight-bearing PA radiographs, with the knee flexed at 45° (Rosenberg view). Absolute medial meniscus extrusion (MME) was measured on magnetic resonance images. Results: The MTE-MFC distance was greater and the MJS width was smaller in Group A than Group B (7.7 ± 1.7mm versus 6.0 ± 1.24mm and 3.2 ± 0.8mm versus 4.5 ± 0.7 mm, respectively; P < 0.05). The MTE-MFC distance and MJS width correlated with MME (r = 0.603 and 0.579, respectively; P < 0.05), and the extent of MME was greater in Group A than Group B (4.1 ± 1.1 mm versus 1.8 ± 1.5 mm, respectively; P < 0.05). Conclusions: MMPRTs increase the MTE-MFC distance and decrease the MJS width, with these measurements correlating to the MME. Therefore, measurement of the MTE-MFC distance and MJS width on the Rosenberg view could be a useful preliminary method for the diagnosis of an MMPRT. Level of evidence: IV