• 제목/요약/키워드: Paris T3 Project

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Paris Rive Gauche Project: (Re)developping the City on the City

  • Ernek, Benoit
    • 토지주택연구
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    • 제5권3호
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    • pp.123-129
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    • 2014
  • Paris hasn't experienced such excitement since the huge changes brought about by Baron Haussmann in the 19th century. Paris Rive Gauche project, started in 1991, is the largest urban project in city ever since, it represents about 1% of Paris territory. It takes place on a workshops, factories and warehouses area that prospered along the Seine river and the railways in the 19th century. Originally planned as a business quarter, Paris Rive Gauche, developed by SEMAPA for the City of Paris, fosters urban diversity through housing, offices, public facilities, shops, creating a stimulating neighbourhood where 18,000 residents, 30,000 students as well as 60,000 employees will soon croth paths. This project's main principles are urban and social diversity, deployment of public facilites, the development of new university campus inside the city, promotion of industrial patrimony and connecting the old 13th distict to the river and the opposite side. Half of the project is going to be built on a concrete slab that covers the railway tracks which is one of the major performances of this long-term project. This concrete slab represents the new level of the City, about 6 to 8 meters above the railway tracks. We distinguish three families of buildings on the cover : Classic buildings; Bridges buildings and Connection buildings, these last guarantee the linkage between old and new level of the City.

IS THE ANOMALOUS MICROWAVE EMISSION DUE TO THE ROTATION OF INTERSTELLAR PAHS? PLANCK RESULTS: PLANCK - AKARI PROJECT

  • Planck Collaboration, Planck Collaboration;Giard, M.;Berne, O.;Doi, Y.;Ishihara, D.;Joblin, Ch.;Kaneda, I.;Marshall, D.;Nakagawa, T.;Ohsawa, R.;Onaka, T.;Sakon, I.;Shibai, H.;Ysard, N.
    • 천문학논총
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    • 제27권4호
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    • pp.195-200
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    • 2012
  • We show how the rotation emission from isolated interstellar Polycyclic Aromatic Hydrocarbons (PAHs) can explain the so-called anomalous microwave emission (AME). AME has been discovered in the last decade as microwave interstellar emission (10 to 70 GHz) that is in excess compared to the classical emission processes: thermal dust, free-free and synchrotron. The PAHs are the interstellar planar nano-carbons responsible for the near infrared emission bands in the 3 to 15 micron range. Theoretical studies show that under the physical conditions of the interstellar medium (radiation and density) the PAHs adopt supra-thermal rotation velocities, and consequently they are responsible for emission in the microwave range. The first results from the PLANCK mission unexpectedly showed that the AME is not only emitted by specific galactic interstellar clouds, but it is present throughout the galactic plane, and is particularly strong in the cold molecular gas. The comparison of theory and observations shows that the measured emission is fully consistent with rotation emission from interstellar PAHs. We draw the main lines of our PLANCK-AKARI collaborative program which intends to progress on this question by direct comparison of the near infrared (AKARI) and microwave (PLANCK) emissions of the galactic plane.

A Monitoring Observation of Comet 17P/Holmes during 2014 Apparition

  • Kwon, Yuna;Ishiguro, Masateru;Hanayama, Hidekazu;Kuroda, Daisuke;Sarugaku, Yuki;Kim, Yoonyoung;Vaubaillon, Jeremie J.;Takahashi, Jun;Watanabe, Jun-Ichi
    • 천문학회보
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    • 제40권1호
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    • pp.61.1-61.1
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    • 2015
  • We performed a monitoring campaign of a Jupiter-Family comet 17P/Holmes, which underwent the dramatic outburst on 23.3 October 2007 at $r_h=2.44AU$, to investigate the secular change in activity and subsequent physical properties of the inner dust coma before and after the 2014 perihelion passage. The monitoring observation was carried out over two years: from May to July 2013, from July to November 2014, and January 2015 with ~weekly cadence. We conducted photometry monitoring in Rc band using four ground-based telescopes, which are the Ishigakijima Astronomical Observatory 105cm telescope, the Okayama Astrophysical Observatory 50cm telescope, the Nishi-Harima Astronomical Observatory 2m telescope, and the T30 51cm i-telescope, respectively. In order to examine the dust production rate, we put a constraint upon the physical distance from the center of the nucleus as rho=2500km and conducted aperture photometry. We found that the average absolute Rc magnitude over the period between July to November 2014 was mR(1,1,0)~12.29, which was approximately 1.5 magnitudes fainter than those of 2013 data. Accordingly, comet 17P/Holmes seemed to become dormant, although a minor eruption was detected on January 26, 2015. In this presentation, we will introduce our ongoing project for 17P/Holmes and discuss why the nucleus becomes dormant within one orbital period.

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음폐수 이용 기존 매립지 가스 발생 향상에 따른 온실가스 감축효과 (Greenhouse Gas Reduction Effect of Improvement of Existing Landfill Gas(LFG) Production by Using Food Waste Water)

  • 신경아;동종인;박대원;김재형;장원석
    • 에너지공학
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    • 제25권3호
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    • pp.104-113
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    • 2016
  • 본 연구에서는 신기후체제 대비를 위한 온실가스 감축 수단으로써 신재생에너지원인 매립가스의 에너지이용 확대를 위해 현장 매립폐기물을 적용하여 음폐수 주입에 따른 메탄가스 생산량 증대 및 이에 따른 온실가스 감축효과를 분석하고자 하였다. 메탄가스 생산량 증대를 위해 주입하는 음폐수는 $35^{\circ}C$, pH 6으로 전처리한 후 사용하였고, 전처리 반응조는 타공성 담체가 고정된 상향류식 고정층 반응기를 이용하였다. 실제 매립폐기물을 이용한 pilot-scale 바이오리액터 운전결과 음폐수 주입시 강우를 활용한 대조군에 비해 6배의 매립가스 증가율을 보였으며, 평균 매립가스 발생량은 $56{\ell}/day/m^3$으로 $1m^3$ 매립지용적에서 연간 약 $20m^3$의 메탄가스가 생산 가능함을 확인하였다. 이를 에너지원으로 활용할 경우 25만 $m^3$ 이상의 중규모 매립지에 적용시 사업성이 확보될 뿐만 아니라 기 등록되어 있는 매립가스 활용 CDM 사업 및 방법론을 기준으로 폐기물 처리용량 25만 $m^3$ 규모의 매립지를 대상으로 온실가스 감축량을 산출한 결과 연간 약 4~5만 톤의 온실가스 감축효과가 있음을 확인하였다.