新生SPICAの体制・観測系検討の現状
|
|
|
- そうりん ぜんじゅう
- 6 years ago
- Views:
Transcription
1 光赤天連スペース将来計画シンポジウム SPICA 現状報告 1. ESA-JAXA 共同技術検討 (CDF Study) とその後の技術検討 検討結果が確定し公開された その後 サイエンス検討を重ねた結果 検討のベースラインを望遠鏡口径 2.5m 温度 8K 以下に冷却する 横置き (Planck 型 ) 構造をベースラインとすることとした (8-11 ページ参照 ) 以下のチームが核となり ESA の技術検討結果および従来の SPICA の成果などを用いて 衛星全体の設計 冷却系 望遠鏡設計を進めている 来月には一次的な検討結果が得られる予定 2.SPICA CV M5 対応チーム設置 (6/4 所長決定 ) 宇宙研 (JAXA) の ΔMDR SRR のための作業 および ESA の Cosmic Vision 次回 M クラス公募への提案の作業を行うチームを組織し 設置した 宇宙研赤外 国内赤外線天文学研究者 宇宙研宇宙物理学研究系 宇宙研工学 研究開発本部 SE/PO 室 国際調整担当の合同チームチーム長 : 芝井 チーム長代理 : 小川博之 中川貴雄 プリプロジェクト再設置時までのチーム SPICA ステアリンググループ ( 所内外 ) と SPICA タスクフォース ( 所内 ) がチームの活動をウォッチ 1
2 3. SPICA チームの活動 3/25-27 SPICA(SAFARI?) コンソーシアム会議 (Utrecht) M5 提案に向けて最終決断 SAFARI チームが欧州 + カナダ + 米国 ( 一部研究者 ) に拡大 高分散中間赤外線分光機能 および系外惑星大気分光機能を搭載する方向で検討を進める (3 4 ページ参照 ) 3/31 SPICA 全体会 5/18 学術会議天文宇宙分科会にて状況報告 この間 サイエンス検討 深化を進めた (5-7 ページ参照 ) 6/3-5 米国遠赤外コミュニティーワークショップにて講演 6/19 SPICA 科学レビュー ( 宇宙研 ) 7/15 SPICA Science Case International Preview (Paris 宇宙研主催) (13ぺージ参照) 7/31 SPICA 全体会 9 月 SPICAコンソーシアム会議 (Bordeaux SAFARI 主催 ) (12ぺージ参照) 2
3 1. SPICA mission overview SPICA Space Infrared Telescope for Cosmology and Astrophysics SPICA is a space mission optimized for mid- and far-ir astronomy. SPICA unveils the dusty era in the Universe (evolution of galaxies), and finds a route to habitable planets (formation of planetary systems). SPICA is launched at ambient temperature, and cooled down in space. (The cryo-cooler system is a key heritage of JAXA from IRTS and AKARI.) Japanese SMI is a mid-ir spectrometer covering mm. European SAFARI is a far-ir spectrometer covering mm. SPICA is a joint mission of JAXA and ESA with other international partners. SPICA is now in its re-definition phase in JAXA, and will go to the open competition as an M-class mission of the ESA Cosmic Vision program. Baseline specifications Telescope : 2.5 m aperture, cooled below 8 K Core wavelength : mm (+ High-resolution spectrometer at mm, Exoplanet instrument at 5 20 mm) Orbit : S-E L2 Halo Orbit Launcher : JAXA H-3 Vehicle Launch Year :
4 Enrichment of the Universe with metal and dust leading to the formation of habitable worlds O H Mg Si O OO O H D HH H SPICA studies how stars have been formed in galaxies along the history of the Universe (Goal1: evolution of galaxies), and how planets have been formed in a disk around a forming star and evolved to be habitable (Goal2: formation of planetary systems). IR spectroscopy SPICA s unique probes λ (μm) Dust bands HRS (organic matter, mineral, ice) Extinction-free metal lines 3. Molecular hydrogen lines λ (μm) AKARI Mid-IR all-sky map 4
5 大目標 銀河成長と惑星系形成 : 多様で豊かな宇宙を生んだ二大過程の解明 目的 1. 銀河成長 物質進化過程の解明 - ダストに隠された銀河成長最盛期 ( 宇宙論的分光サーベイ 10 平方度 ) - 星生成と物質進化の相互作用 ( 近傍銀河 4000 個 ) 目的 2. 惑星系形成過程の解明 - ガスの精密定量による惑星形成シナリオの検証 - 惑星形成における水と氷の役割 - 惑星系外縁天体の起源
6 IR luminosity density (L / Mpc 3 ) 1. SPICA mission overview Space infrared astronomy: from IRTS, AKARI to SPICA IRTS (Japan) 1995 IRTS Goto+ 2010, A&A 514, 6 AKARI (Japan, Korea, Europe) 2006 ~2011 Spitzer (US) 2003 ~ AKARI survey mid-ir spectroscopy Herschel (Europe, US) far-ir spectroscopy Evolution of galaxies Photometry SPICA Exploration IR galaxy Luminous IR Ultra-luminous IR redshift z=3 Spectroscopy Physics 6
7 1. SPICA mission overview Work-sharing plan Telescope Payload Module Cryocooler Focal Plane Instrument Assembly FIR Spectrometer (SAFARI) NL + European countries + Canada & US MIR Instrument (SMI) SPICA Data Center (NAOJ) Bus Module Launcher Focal Plane Attitude Sensor Science Community JP, Europe, US, KR, TW,,, Exoplanet Spectroscopy (SPEChO) European countries 7
8 Current baseline configuration Planck-type PLM with a 2.5-m, <8K telescope Mirror M1 2.5 mf M2 Support Structure Telescope Baffle Mirror M2 PLM Metering Structure Cryo Warm Electronics SVM Top Panel Telescope Optical Bench Telescope Shield (20 K) Supporting Bipod V-Groove thermal shields AOC StarTracker 1K-JT Compressors 2ST Compressors 1K-JT Compressors 8
9 運用体制 ( 案 ) JAXA 宇宙科学研究所 Operational Ground Segment Science Ground Segment 国立天文台 JAXA JAXA Stations Mission Operation Center (MOC) Science Operation Center (SOC) Science Data Center (SDC) Non- European User Community (Japan) (East Asia) Instrument Control Centers (ICCs) ESA ESA Stations ESA ESA Science Center (ESC) European Data Archive Center (ESDC) TBD European User Community 研究は基本的に共同利用であり データが広い範囲の研究者に公開される 9
10 プロジェクト推進体制 - SPICA コンソーシアム 日本 欧州 M5 Proposal ESA NAOJ JAXA SRON SPICA-J Project SPICA Consortium SAFARI Consortium 遠赤外線観測装置 ( 欧州 +) SMI Consortium 中間赤外観測装置 ( 日本 ) 名大 東大他 Scientists (outside the instrument teams) 装置チーム外研究者 SPEChO Consortium 系外惑星大気分光装置 ( 検討中 ) 10
11 ( 参考 ) 国際評価委員会 目的 SPICA 計画について 科学的観点からの評価を得る 日時 場所 2015 年 7 月 15 日 Paris 評価委員 Michael Rowan-Robinson (UK), Martin Bureau (UK), Anthony Jones (FR) Peter Barthel (NL) Anthony Peter Jones (FR) Martin Harwit (US), George Helou (US) Kazuhisa Mitsuda (JP), ISAS Saku Tsuneta, Masaki Fujimoto, Munetaka Ueno, Ikko Funaki SPICA Hiroshi Shibai (PI), Takashi Onaka (PS), Hidehiro Kaneda (PI 補佐 ), Kotaro Kohno (PS 補佐 ) Daisuke Ishihara, Takehiko Wada, Naoki Isobe, Peter Roelfsema (NL), Bruce Sibthorpe (NL) 11
12 1. SPICA mission overview Space infrared astronomy: from IRTS, AKARI to SPICA IRTS (Japan) 1995 IRTS AKARI (Japan, Korea, Europe) 2006 AKARI survey ~2011 Spitzer (US) 2003 ~ mid-ir spectroscopy SPICA SPICA Formation of planetary systems Herschel (Europe, US) far-ir spectroscopy AU Case study ~1 AU Planet-forming disk Universality 12
13 1. SPICA mission overview Project schedule Reviews & Phases Model & Tests CY JAXA ESA JAXA Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Phase-A Phase-B Phase-C MDR SRR SDR Project Appr. Rev. pre-pdr Sys-PDR pre-cdr Sys-CDR PSR Launch Phase-A PRR Phase-B1 SRR Phase-B2 PDR Phase-C CDR Phase-D QR? AR margin Phase-E1 Phase-D Phase-E 2028 PLM Comp Dev. MCS Comp. Dev. PLM/CRYO Design manufacture MCS Design / Manufacture Manufacture PLM/CRYO-STM MCS FAS PLM/CRYO AI L Launch Operation FAS Design manufacture PLM PLM IVT ESA System IVT System IVT Caption SVM Design manufacture SVM FM SIA IV SIA IVT FPI Warm Elechtronics CQM (FPI) Design STA Manufacture AIV EM/STM STA Design / Manufacture Front Loading FPIA Design IOB-STM MCS-EM FPIA FPIA IVT SMI Consortium SMI Components Developmen SMI Design Manufacture manufacture Detector Modules SMI SMI-CQM SAFARI Consortium + SAFARI Components Devekopment SAFARI Design Manufacture Manufacture SAFARI SAFARI-CQM Operation: 3 Years (Nominal), 5 Years (Goal) 13
14 1. SPICA mission overview Importance of a cryogenically-cooled IR telescope K 10 5 reduction! SPICA (8K) SPICA 14
15 1. SPICA mission overview Dramatic improvement in the sensitivity SOFIA AKARI FIS-FTS Limiting Line Flux (5-1hr) / Wm AKARI IRC R=25000 JWST/MIRI R=3000 Spitzer SPICA 100 Improvement R=300 HERSCHEL SPICA/SAFARI 2010's 2020's ALMA Wavelength / mm 15
16 1. SPICA mission overview SPICA s uniqueness in extra-galactic astronomy Sensitivity (5, 1 hour) of ALMA, SPICA, JWST and TMT, plotted on spectra of typical star-forming galaxies at z = 3 with different dust extinction values (A V = 0.3, 3, 30 mag). SPICA provides unique spectral tools to study physics in dust-obscured galaxies. SPICA A V = 0.3 mag ALMA II Zw 96 TMT JWST SPICA fills the spectral gap between ALMA and JWST. 16
![of planetary systems Science objectives [SO1] Star formation of distant galaxies [SO4] Gas dissipation in PPDs](/docs-images/64/51423880/images/17-3.jpg "[SO2] AGN outflow [SO5] Debris disks to solar system [SO3] Star formation in nearby galaxies [SO6] Exoplanet")
17 2.1. Overview Science goals and objectives Top-level goal Enrichment of the Universe with metal and dust, leading to the formation of habitable worlds [SG1] Evolution of galaxies Science objectives SCIENCE GOALS [SG2] Formation of planetary systems Science objectives [SO1] Star formation of distant galaxies [SO4] Gas dissipation in PPDs [SO2] AGN outflow [SO5] Debris disks to solar system [SO3] Star formation in nearby galaxies [SO6] Exoplanet atmosphere 17
18 3.3. SPICA mission overview Baseline design payload module Planck-type PLM with a 2.5 m, 8 K telescope secondary mirror cryocooler system primary mirror telescope thermal shield V-groove thermal shields telescope baffle instrument optical bench service module Front view Side view 18
19 3.3. SPICA mission overview Telescope Optical design The 2.5 mφ optical design is scaled from the 2.0 mφ CDF study. Optical specifications Telescope type : Ritchey Chrétien Entrance Pupil Diameter : 2.5 m Field of View : 30 arcmin Wave Front Error : <1.4 mm rms Diffraction limited at 20 mm Temperature Launch: Room temperature Operation: < 8 K Fabrication ESA is in charge of the procurement of the telescope. Technical Heritage The mirrors are based on the AKARI and Herschel heritage (SiC mirrors). 19
20 3.3. Configuration and specifications Mechanical cryo-coolers Mechanical cryo-coolers in the baseline design have been developed in Japan. 20K-class two-stage Stirling cooler (2ST) 4K-class J-T cooler (4K-JT) 1K-class J-T cooler (1K-JT) Cooling objectives JT precooling STA + FPIA FPIA (SAFARI+SMI) Cooling power (EOL) 200 mw@20 K, 1000 mw@100 K 40 mw@4.5 K 10 mw@1.7 K Input power < 90 W < 90 W < 75 W Lifetime > 3 years (goal: 5 years) >3 years (goal: 5 years) >3 years (goal: 5 years) Heritage AKARI (2006), JEM/SMILES (2009) ASTRO-H (2015) JEM/SMILES (2009) ASTRO-H (2015) Based on 4 K-JT R&D status TRL6 (ASTRO-H) TRL6 (ASTRO-H) TRL5 Cooling performance & reliability have improved based on AKARI & SMILES (e.g., flexure bearings to support the piston and displacer, inner outgas control, microphonics control). Design lifetime of 1K-JT has improved based on ASTRO-H 4K-JT with enhanced contamination control. These technologies are reflected in the 2ST and 4K-JT coolers. 20
21 3.3. Configuration and specifications Focal-plane instruments SPICA Mid-IR Instrument: SMI (LRS) mm, Si:Sb, prism:10 slit x x10 slit viewer, high mapping speed (MRS) mm, Si:Sb, grating:1 slit + beam-steering mirror, high sensitivity (HRS) mm, Si:As, grating: 6 slit + beam-steering mirror, high resolution SPICA Far-IR Instrument: SAFARI mm, TES, grating: 4 beams + beam-steering mirror, high sensitivity EChO instrument on SPICA: SPEChO 5-20 mm, Si:As, grating, high-stability ( in one eclipse) monitoring Spectral Resolution Line Sensitivity JWST/MIRI-MRS JWST/MIRI-LRS Spitzer/IRS Spitzer/IRS R = R = 1000 SPICA/SMI SPICA/SAFARI R = 3000 R = 300 Wavelength (mm) Wavelength (mm) 21
22 3.3. Configuration and specifications Instrument configuration on the telescope optical bench SPEChO FAS (Focal attitude sensor) SMI SAFARI SMI 22
Wish list for US participation by SDR
次世代赤外線天文衛星 SPICA の概要 2011 年 1 月 6 日中川貴雄 (JAXA) SPICA team 企画セッション :SPICA の挑戦 概要 次世代赤外線天文衛星 SPICA の概要 ( 中川 JAXA ) SPICA 観測装置 ( 片坐 JAXA ) 科学目的 SPICA の目指すもの ( 松原 JAXA ) SPICA で探る太陽系科学 ( 渡部 天文台 ) SPICA による系外惑星研究
PowerPoint プレゼンテーション
日本天文学会春季年会 W213a 215-3-19 次世代赤外線天文衛星 SPICA: 日欧共同詳細検討結果芝井広 ( 大阪大 ) 中川貴雄 松原英雄 川勝康弘 (JAXA) 尾中敬 ( 東京大 ) 金田英宏 ( 名古屋大 ) 他 SPICA チーム ( 日本の中間赤外線観測装置については次の講演参照 ) 1 When and How did our Universe become Material-rich
Microsoft PowerPoint - ICRRseminar_AkariSpica_ pptx
SPICA 2010 7 16 ICRR ISAS,JAXA List of my talk Bright Source Catalog Science Highlights Warm Mission SPICA 2 地球大気の透過率 & 放射強度 3 地球大気の吸収を逃れる 地球大気の放射から逃れる なぜ宇宙へ? 4,000m 級の高山に上っても 大気の赤外線放射は 宇宙から来る赤外線の 100
PowerPoint プレゼンテーション
宇宙科学シンポジウム 2017-01-06 SPICA ミッション 進捗報告 芝井広 ( 阪大 /JAXA) 小川博之 (JAXA) 尾中敬 ( 東大 ) 金田英宏 ( 名大 ) 河野孝太郎 ( 東大 ) 中川貴雄 (JAXA) 松原英雄 (JAXA) 山田亨 (JAXA) 他 SPICA チームメンバー P-086: A SPICA far-ir instrument SAFARI 土井靖生 (
SPICA SE会議#2
宇電懇シンポジウム 2015-01-28 SPICA 計画の経緯 現状 芝井広 ( 阪大 ),SPICA チーム あかり 遠赤外全天マップ 2014/12 公開 科学目的 3: 最高感度の宇宙赤外線天文台の実現 微惑星帯 Henning & Semenov 2013 銀河成長と惑星系形成: 多様で豊かな宇宙を生んだ二大過程の解明 ~1500K 地球型惑星 ~300K ~150K 小惑星帯 巨大惑星
Wish list for US participation by SDR
The next-generation space infrared astronomy mission SPICA GOPIRA Symp August 2013 T. Nakagawa, H. Matsuhara, Y. Kawakatsu (ISAS/JAXA) for SPICA Team Institute of Space & Astronautical Science Japan Aerospace
1 (5) ISAS/JAXA for the SRG SXC working group
1 (5) ISAS/JAXA for the SRG SXC working group 14 2 calendar year NeXT & SRG cooler development schedules SRG 2007 2008 2009 2010 2011 2012 basic design EM design EM fabrication & test PFM design PFM fabrication
koukai-seminar2018-kaneda-s
国際協力で進める宇宙科学プロジェクト 1/24 金田英宏宇宙物理学研究室 (U 研 ) 赤外線グループ (Uir) 内容 : 1. 名大と宇宙科学プロジェクト 2. あかり における国際協力 3. SPICAの実現に向けて 4. 今後の宇宙科学プロジェクト 第 27 回公開セミナー 天文学の最前線 : 国際化する天文学研究 1. 名大と宇宙科学プロジェクト Tenma (1983) 物理 U 研 :1965
110 JAXA JAXA / /
109 JAXA 4 1 2015 3 31 15 40 27 82 / 7/13 6/2 9/13 22/28 13 8 12 8 8 7 10 9 1 1 21 20 19 17 1988 63 2000 15 5 2 26 5 1 10 0 10 3 8 4 6 4 8 13 2 110 JAXA JAXA 9 12 80 60 40 20 / 50 40 30 20 10 / 0 0 3 18
SFN
THE STAR FORMATION NEWSLETTER No.291-14 March 2017 2017/04/28 16-20 16. X-Shooter spectroscopy of young stellar objects in Lupus. Atmospheric parameters, membership and activity diagnostics 17. The evolution
Wish list for US participation by SDR
次世代赤外線天文衛星 SPICA 計画の現状と課題 ~ 大型衛星計画の先駆として ~ 宇宙科学シンポジウム 2013 年 1 月 8 日中川貴雄 松原英雄 川勝康弘 (ISAS/JAXA) for SPICA Team SPICA がめざすもの : 我々はなぜ かく在るのか? 宇宙を構成する銀河はどこで生まれたのか? 銀河誕生のドラマ 我々を作る物質はどこで生まれたのか? 宇宙の物質輪廻の解明 我々を育んだ惑星はどうやって生まれたのか
系外惑星大気
http://hubblesite.org/newscenter/archive/2001/38/ 2004 9 30 1781 1846 1930 50 2 3 radial velocity HDS 5m/s HD209458 HD209458+I 2 cell Subaru/HDS 4 (Mayor & Queloz 1995) 4.2 5 2 1.5% HST 4 orbits Brown
2. TMT TMT TMT 1 TMT 3 1 TMT TMT PI PI PI SA PI SA SA PI SA PI SA
TMT TMT 181 8588 2 21 1 e-mail: n.kashikawa@nao.ac.jp TMT TMT TMT * 1 TMT TMT TMT SAC Science Advisory Committee 2012 8 13 1 1. 1 2 3 20 * 1 609 2. TMT TMT TMT 1 TMT 3 1 TMT 8 3 4 TMT PI 1 10 50 2.1 PI
スライド 1
2004/12/25 HOP JTPF JASMINE ILOM JAXA) SPICA JELT Yerkes 1m (1897) Palomar 5m (1948) Subaru 8m (1999) 6.5m Large Binocular Telescope(LBT) 8.4m Mt.Graham 18 3m-6m 6.5m 3m Hubble Space Telescope 2.4m (0.115
遠くを見よう→赤外線へ
宇宙空間からの 宇宙物理学 天文学 中川貴雄宇宙航空研究開発機構宇宙科学研究本部 Feb 1, 2007 GOPIRA WS 目指すゴール 宇宙科学長期計画 (10 年 ) 宇宙の真の姿は? 宇宙の歴史は? 宇宙科学委員会 計画部会 宇宙科学長期 (10 年 ) 計画 宇宙空間からの天体物理学 :3 つの目標 宇宙の大規模構造とその成り立ちを解明し 暗黒物質 暗黒エネルギーを探る 太陽系外惑星の観測により惑星の形成過程を探る
SPICA の中間赤外線検出器
SPICA の遠中間赤外線検出器 和田武彦 鈴木仁研 (ISAS/JAXA) 内容 次世代赤外線天文衛星 SPICA 赤外線検出器 SPICA の中間赤外線検出器 Si:Sb BIB 1024x1024 Si:As BIB 1024x1024 熱設計 SPICA の遠赤外線検出器 ( 鈴木さん ) 次世代赤外線天文衛星 SPICA 大口径 :2.5m 冷却望遠鏡 : 8K 波長 17-210um の
Microsoft PowerPoint - subaru_um.pptx
WFIRST and Subaru in Middle 2020 s Euclid 0.4 1.8μm WISH 1 5μm Wide field Space Missions in 2020 s WFIRST 0.6 2μm (option 2.4μm) Wide-field Imaging Surveyor for High-redshift 超広視野初期宇宙探査衛星計画 ISAS Call for
Telescope aperture 1.5mφ Telescope length Fit within the H-IIA nose fairing Spatial resolution 0.1" in UV 0.16" in Vis/NIR (Diffraction limit of 1.5mφ
, (NAOJ) (Kyoto U.) Telescope aperture 1.5mφ Telescope length Fit within the H-IIA nose fairing Spatial resolution 0.1" in UV 0.16" in Vis/NIR (Diffraction limit of 1.5mφ at 1µm ) FOV ~200" x 200" to cover
資料1－3
WPT (2017) ( ) *JST Center of Innovation ( 13- ) Last 5X * 16 8, 15 7, 14 6 METLAB 16 20, 15 18 WPT * IEEE MTTS Wireless Power Transfer Conference ( 11-, ) MTTS TC-26 (Wireless Energy Transfer and Conversion
太陽系外惑星探査
http://hubblesite.org/newscenter/archive/2001/38/ Terra MODIS http://modarch.gsfc.nasa.gov/ http://www.nasa.gov/home/index.html / 2 Are we alone? Origins Where are they? (Fermi 1950) 3 4 0.5 arcsec 10pc
ISLE 2010/08/17
ISLE 2010/08/17 Talk plan 1. ISLE 2. 3. 4. 2011A 2010/8/17 OAOUM 2010 ISLE 2010/8/17 OAOUM 2010 ISLE OASIS HAWAII (HgCdTe 1024 1024) 4.2 4.2 arcmin 2, 0.25 arcsec/pix (13 Filters) 2006B FWHM = 0.75 arcsec
理論懇2014
Proposal for a project of high-precision stellar radial velocity work, Struve (1952)! But there seems to be no compelling reason why the hypothetical stellar planets should not, in some instances, be much
Contents 1. Ia? 2. Ia 3. WISH Ia cosmology 4. WISH Ia + rate 5.
Type Ia Supernova Survey w/ WISH Contents 1. Ia? 2. Ia 3. WISH Ia cosmology 4. WISH Ia + rate 5. Contents 1. Ia? 2. Ia 3. WISH Ia cosmology 4. WISH Ia + rate 5. Type Ia Supernova + +?? (single degenerate)?
2 2. 13 2 1 1 PBS: Post-Boost Stage 1.2 2 30 JAXA 49 2 108 4 205
252 5210 3 1 1 e-mail: morita.yasuhiro@jaxa.jp 9 1. 1 F1 1 204 2015 4 2 2. 13 2 1 1 PBS: Post-Boost Stage 1.2 2 30 JAXA 49 2 108 4 205 IT IT 3 2 JAXA 2 3 1 2 2 2 3 2 206 2015 4 C/C 2 3. 3.1 1 SRB-A H2A
J. Jpn. Inst. Light Met. 65(6): 224-228 (2015)
65 62015 224 228 ** Journal of The Japan Institute of Light Metals, Vol. 65, No. 6 (2015), 224 228 2015 The Japan Institute of Light Metals Investigation of heat flow behavior on die-casting core pin with
090423_EXCEED_Web版
A 3 B X 3 LEO (Flexible Standard Bus) C 2 3 kg SPICA ASTRO-H GEOTAIL GINGA YOHKOH AKEBONO NOZOMI ASCA HITEN ASTRO-G PLANET-C HAYABUSA SPRINT 5 JAXA NOTE 2009 3»»»»»» 22 302 200kg400kg 300W 1kW 3 1 4 DE
Table 1. Assumed performance of a water electrol ysis plant. Fig. 1. Structure of a proposed power generation system utilizing waste heat from factori
Proposal and Characteristics Evaluation of a Power Generation System Utilizing Waste Heat from Factories for Load Leveling Pyong Sik Pak, Member, Takashi Arima, Non-member (Osaka University) In this paper,
16_.....E...._.I.v2006
55 1 18 Bull. Nara Univ. Educ., Vol. 55, No.1 (Cult. & Soc.), 2006 165 2002 * 18 Collaboration Between a School Athletic Club and a Community Sports Club A Case Study of SOLESTRELLA NARA 2002 Rie TAKAMURA
(ASIAA)
2016.11.07 (ASIAA) Dogs.. Introduction Dust Obscured Galaxies IR-bright DOGs Introduction Dust Obscured Galaxies i - [22] > 7.0 (AB mag) (Toba, Nagao et al. 2015) This study IR-bright DOGs HSC+WISE (Final
Abstract 1 1 2 Abstract Fig. 1 Fig. 2 Fig. 3 Abstract 1 2 3 4 5 6 7 8 10 9 Abstract 1 1 2 3 4 5 6 7 8 9 Abstract 1 2 3 4 Abstract 1 1 2 2 3 4 5 6 3 7 8 9 4 Abstract 1 2 3 4 5 6 7 8 9 10
Microsoft PowerPoint - HiCIAOTamuraBerkeley070607f.ppt
HiCIAO and exoplanet/disk searches on Subaru 2007.6.7 @ Berkeley Motohide Tamura NAOJ, Extrasolar Planet Project Office in collaboration with University of Hawaii, Hilo Collaborators K. Hodapp 2, R. Suzuki
On the Wireless Beam of Short Electric Waves. (VII) (A New Electric Wave Projector.) By S. UDA, Member (Tohoku Imperial University.) Abstract. A new e
On the Wireless Beam of Short Electric Waves. (VII) (A New Electric Wave Projector.) By S. UDA, Member (Tohoku Imperial University.) Abstract. A new electric wave projector is proposed in this paper. The
Table 1. Reluctance equalization design. Fig. 2. Voltage vector of LSynRM. Fig. 4. Analytical model. Table 2. Specifications of analytical models. Fig
Mover Design and Performance Analysis of Linear Synchronous Reluctance Motor with Multi-flux Barrier Masayuki Sanada, Member, Mitsutoshi Asano, Student Member, Shigeo Morimoto, Member, Yoji Takeda, Member
Spacecraft Propulsion Using Solar Energy Spacecraft with Magnetic Field Light from the Sun Solar Wind Thrust Mirror Solar Sail Thrust production by li
2004.3.28 物理学会シンポジウム 磁気プラズマセイル の可能性と 深宇宙探査への挑戦 宇宙航空研究開発機構 船木一幸 Spacecraft Propulsion Using Solar Energy Spacecraft with Magnetic Field Light from the Sun Solar Wind Thrust Mirror Solar Sail Thrust production
スペースプラズマ研究会-赤星.ppt
14 1 1 1 1 Pauline Faure 1 1 2 3 (1: 2: JAXA 3: IHI) IHI (C)(No.21560819) ISAS(JAXA) ISO TC20/SC14 / (Spall) 60~90% 2 (Cone) 1% (Jetting) CDV11227 Committee Draft for Comments CDV11227 Witness plate Sabot
subaruUM2010_murayama
SuMIRe/PFS 村山斉 (IPMU & Berkeley) Subaru Users Meeting @ 国立天文台 2011.1.19 PFS HSC 5 PFS (FIRST) HSC PFS weak lensing BAO dark energy PFS cf. white paper UM UM PFS exciting SAC HSC UM Eric Prieto (Marseille)
地球観測衛星データの保存・配布システム
Earth Remote Sensing Data Archive and Distribution System NASAEOS Earth Observing SystemASTER Advanced Spaceborne Thermal Emission and Reflection Radiometer ASTERASTER EOS ASTER DADSData Archive and Distribution
XFEL/SPring-8
DEVELOPMENT STATUS OF RF SYSTEM OF INJECTOR SECTION FOR XFEL/SPRING-8 Takao Asaka 1,A), Takahiro Inagaki B), Hiroyasu Ego A), Toshiaki Kobayashi A), Kazuaki Togawa B), Shinsuke Suzuki A), Yuji Otake B),
untitled
1 2 3 4 5 130mm 32mm UV-irradiation UV-cationic cure UV-cationic cure UV-cationic cure Thermal cationic Reaction heat cure Thermal cationic Cation Reaction heat cure Cation (a) UV-curing of
パナソニック技報
Panasonic Technical Journal Vol. 64 No. 2 Nov. 2018 Optical Disc Archiving System with 100 Years Lifespan of Digital Data Takuto Yamazaki Yasushi Kobayashi Blu-ray Disc 1 Archival Disc 2 3300 GB 10012
<30345F90BC96EC90E690B65F E706466>
15 特集 国際宇宙ステーション日本実験棟 きぼう における流体実験 * Space Experiment on the Instability of Marangoni Convection in Liquid Bridge Koichi NISHINO, Department of Mechanical Engineering, Yokohama National University 1 thermocapillary
19 Figure-2 General Layout of Mahaica-Mahicony-Abary Lower River Basin Rural Development Plan Study Location Map of Cooperative Republic of Guyana PROJECT DIGEST 1. PROJECT TITLE : Mahaica-Mahaicony-Abary
MW鹿児島
NGC1068 Dark Matter Halo baryon gas stars SMBH SMBH 1 SMBHs? (AGN) AGN Seyfertization Taniguchi 1987, ApJ, 317, L57 AGN The dead quasar problem (Rees 1990, Science, 247, 817) T AGN ~ 10 8 yrs AGN AGN
SCR8-17XX Technical Data Optical Magnetic Brushless Coreless Encoder Motor Unitmm 5 Number of commutator segments Brushes Precious Metal Bearings Slee
CORELESS MOTOR SCR8-17 SCR10-17 SCR10-25 SCR12-13 SCR12-18 SCR12-26 SCR13-20 SCR13-28 NEW SCR16-25 SCR16-35 SCR17-25 SCR17-35 SCR18-37 SC21-37 SC24-32 Smaller and higher-performance motors realized by
Development of a Mine in Andes Mountains, Peru by Yumisaburo NURAI The development of Huanzala Mine was started in October 1966 after the completion of prospecting and production began at 500M.T./day crude
Fig. 1 KAMOME50-2 Table 1 Principal dimensions Fig.2 Configuration of the hydrofoils (Endurance and sprint foil) Fig. 3 Schematic view of the vortex l
A study on the simulation of the motion of personal full-submerged hydrofoil craft by Yutaka Terao, Member Summary A new energy utilization project developed by Tokai University was started in 1991. It
teionkogaku43_527
特集 : 振動流によるエネルギー変換 熱輸送現象と応用技術 * Oscillatory Flow in a Thermoacoustic Sound-wave Generator - Flow around the Resonance Tube Outlet - Masayasu HATAZAWA * Synopsis: This research describes the oscillatory
Development of Induction and Exhaust Systems for Third-Era Honda Formula One Engines Induction and exhaust systems determine the amount of air intake
Development of Induction and Exhaust Systems for Third-Era Honda Formula One Engines Induction and exhaust systems determine the amount of air intake supplied to the engine, and as such are critical elements
Pyo Jeonghyun 5 6 Component Separation of the Near-Infrared Diffuse Spectrum from the AKARI Archive Data Kohji TSUMURA 1, Itsuki SAKON 2,
1 2 3 4 3 3 Pyo Jeonghyun 5 6 Component Separation of the Near-Infrared Diffuse Spectrum from the AKARI Archive Data Kohji TSUMURA 1, Itsuki SAKON 2, Shuji MATSUURA 3, Toshio MATSUMOTO 4, 3, Takehiko WADA
Contents 1. Ia cosmology 2. Ia / rate 3.
WISH ( ) Contents 1. Ia cosmology 2. Ia / rate 3. supernova (CC SN) Ia (SN Ia) supernova classification supernova Ia (SN Ia) - : redshift z~1.5 - progenitor system: Single Degenerate? Double Degenerate?
2 3 12 13 6 7
2 8 17 42ZH700046ZH700052ZH7000 28 43 54 63 74 89 2 3 12 13 6 7 3 4 11 21 34 63 65 8 17 4 11 4 55 12 12 10 77 56 12 43 43 13 30 43 43 43 43 10 45 14 25 9 23 74 23 19 24 43 8 26 8 9 9 4 8 30 42 82 18 43
H8000操作編
8 26 35 32H800037H800042H8000 49 55 60 72 2 3 4 48 7 72 32 28 7 8 9 5 7 9 22 43 20 8 8 8 8 73 8 13 7 7 7 55 10 49 49 13 37 49 49 49 49 49 49 12 50 11 76 8 24 26 24 24 6 1 2 3 18 42 72 72 20 26 32 80 34
Phonetic Perception and Phonemic Percepition
No.7, 587-598 (2006) The Historical and Social Significance of Foreign Brides in the Uonuma Region of Niigata Prefecture (1) TAKEDA Satoko Nihon University, Graduate School of Social and Cultural Studies
2
8 23 26A800032A8000 31 37 42 51 2 3 23 37 10 11 51 4 26 7 28 7 8 7 9 8 5 6 7 9 8 17 7 7 7 37 10 13 12 23 21 21 8 53 8 8 8 8 1 2 3 17 11 51 51 18 23 29 69 30 39 22 22 22 22 21 56 8 9 12 53 12 56 43 35 27
2
8 22 19A800022A8000 30 37 42 49 2 3 22 37 10 11 49 4 24 27 7 49 7 8 7 9 8 5 6 7 9 8 16 7 7 7 37 10 11 20 22 20 20 8 51 8 8 9 17 1 2 3 16 11 49 49 17 22 28 48 29 33 21 21 21 21 20 8 10 9 28 9 53 37 36 25
COE
COE COOL05 MD @ @ @ @ n ν x, y 2 2 International Workshop on Beam Cooling and Related Topics ( COOL05) General Topics Overview. S-LSR Report from Lab Report from Lab Electron Cooling Muon Cooling
Ando_JournalClub_160708
Independent discoveries of a tidally disrupting dwarf galaxy around NGC 253! A Tidally Disrupting Dwarf Galaxy in the Halo of NGC 253 Toloba, E. et al. 2016, ApJL, 816, L5 (hereafter T16, accepted 2015.12.07)
光赤外将来計画検討書： 改訂の進捗
セッション 3: スペース班報告および関連状況 ~ 概要 2015 年度光学赤外線天文連絡会シンポジウム 光赤外将来計画 : 報告書の最終取りまとめと長期戦略への布石 2015 年 9 月 14 日 ( 月 ) ー 16 日 ( 水 ) 松原英雄 (ISAS, JAXA) セッション3: スペース班報告および関連状況 座長: 川端弘治 10:00 概要 松原英雄 (JAXA) 10:15 SPICAの進行状況報告
NIES ASEAN4.. NIES.....EU.. ASEAN4 NIES
NIES ASEAN4.. NIES.....EU.. ASEAN4 NIES NIES ASEAN4 EU NIES ASEAN4 EU On-line UN Comtrade Database NIES NIES.AEAN4..EU.NIESASEAN4 NIES NIES ASEAN4. EU NIES ASEAN4. TPS: Toyota Production System.... Dunning
千葉県における温泉地の地域的展開
1) 1999 11 50 1948 23) 2 2519 9 3) 2006 4) 151 47 37 1.2 l 40 3.6 15 240 21 9.2 l 7. 210 1972 5) 1.9 l 5 1 0.2 l 6 1 1972 1.9 0.4 210 40-17- 292006 34 6 l/min.42 6) 2006 1 1 2006 42 60% 5060 4050 3040
Nano Range Specification Stable & Stable Telescopic Resonators Model Nano S Nano S Nano S Nano S Nano L Nano L Nano L Nano L Nano L Nano L Nano L 130-
L i t r o n T o t a l L a s e r C a p a b i l i t y Nano Series Ultra Compact Pulsed Nd:YAG Lasers Product Range Specification Nano Range Specification Stable & Stable Telescopic Resonators Model Nano
はなしの概要 あかり 遠赤外線分光器FIS-FTS FIS-FTSによる観測 セレンディピタス分光サーベイ FIS-FTSのデータ解析 キャリブレーションと標準ツール 初期成果 銀河中心 Yasuda et al. 星形成領域 Okada et al. 今後の解析 LMC セレンディピタスサーベイ
あかり 遠赤外線分光観測の成果 宇宙物理学研究室 赤外線グループ UIR 川田光伸 ２００９ 宇宙ブロック研究発表会 2009/11/19-20 @ エコトピア はなしの概要 あかり 遠赤外線分光器FIS-FTS FIS-FTSによる観測 セレンディピタス分光サーベイ FIS-FTSのデータ解析 キャリブレーションと標準ツール 初期成果 銀河中心 Yasuda et al. 星形成領域 Okada
爆発的星形成? AGN関係を 生み出す物理機構の観測的示唆
Umemura, Fukue & Mineshige 1997, 1998 Ohsuga et al. 1998 R ring ~100pc dv r = v 2 ϕ dt r 1 dp ρ dr dφ 1 r d(rv ϕ ) dt = 3χE 2c typical timescale dr + χ c F r 3 2 Myr r R ring V ring 3χE 2c v ϕ Umemura,
5 7 3AS40AS 33 38 45 54 3 4 5 4 9 9 34 5 5 38 6 8 5 8 39 8 78 0 9 0 4 3 6 4 8 3 4 5 9 5 6 44 5 38 55 4 4 4 4 5 33 3 3 43 6 6 5 6 7 3 6 0 8 3 34 37 /78903 4 0 0 4 04 6 06 8 08 /7 AM 9:3 5 05 7 07 AM 9
* Meso- -scale Features of the Tokai Heavy Rainfall in September 2000 Shin-ichi SUZUKI Disaster Prevention Research Group, National R
38 2002 7 2000 9 * Meso- -scale Features of the Tokai Heavy Rainfall in September 2000 Shin-ichi SUZUKI Disaster Prevention Research Group, National Research Institute for Earth Science and Disaster Prevention,
Microsoft PowerPoint - TMTinst_ _summerschool_akiyama
1 2 3 4 5 6 7 8 9 10 590nm 2200nm 0 1.739 1.713 5 1.708 1.682 10 1.678 1.652 0-10 0.061061 0.061061 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 1.0 x1.0 0.5 x0.5 0.2 x0.2 0.1 x0.1 bg/30ms
untitled
ISO 26262 : 2011(E) Functional safety nal 2 Managem ment of functio safety 3 Con ncept phase Annex B Examples for evaluating a safety culture Annex C (informative) Aim of the confirmation measures 8 Functional
TAMA --> CLIO ---> LCGT TAMA 300m基線長 三鷹(NAOJ) CLIO 100m 神岡 低温鏡 年5月17日火曜日
LCGT LCGT 2011/5/17, 1 TAMA --> CLIO ---> LCGT TAMA 300m基線長 三鷹(NAOJ) CLIO 100m 神岡 低温鏡 2 2011年5月17日火曜日 LCGT (Large-scale Cryogenic Gravitational wave Telescope) Underground in Kamioka, Japan Silent & Stable
ELECTRONIC IMAGING IN ASTRONOMY Detectors and Instrumentation 4 The discovery power of modern astronomoical instruments 5 Instrumentation and dete
ELECTRONIC IMAGING IN ASTRONOMY Detectors and Instrumentation 4 The discovery power of modern astronomoical instruments 5 Instrumentation and detectors 4 2017/4/19 Contents 4.3 Polarization; transverse
.\..ol.eps
1 2007 2008 2008 88 38 NGO 44 1 1 18 33 2008 10 2 2008 30 1 2006 18 2006 11 24 12 2007 2007 2007 11 2008 101 1297 Dragutin Dado Kovacevic 34 111 15 14 16 2007 11 3 12 1 10 a b c d e 4 25 1950 2008 11 25
Trip Trip Trip
- - - - 1999 Leonid MAC Multi-Instrument Aircraft Campaign November 8-23, 1999 1998-2002 (2001 ) Predictions, Observational Plans and Results for Leonid 1998-2002. Photo Gallery taken by Photographic Camera
NKK NEWS 2012
2012Spring 42 CONTROLS SINGLE POINT OF CONTROL (S.P.O.C.) Introduction / Index INDEX Module Versions: C / D BECAUSE CONTROL IS LOGIC! www.42controls.com Introduction... 2 Console Desktop Version... 3
B
B07557 0 0 (AGN) AGN AGN X X AGN AGN Geant4 AGN X X X (AGN) AGN AGN X AGN. AGN AGN Seyfert Seyfert Seyfert AGN 94 Carl Seyfert Seyfert Seyfert z < 0. Seyfert I II I 000 km/s 00 km/s II AGN (BLR) (NLR)
Fig. 3 Flow diagram of image processing. Black rectangle in the photo indicates the processing area (128 x 32 pixels).
Fig. 1 The scheme of glottal area as a function of time Fig. 3 Flow diagram of image processing. Black rectangle in the photo indicates the processing area (128 x 32 pixels). Fig, 4 Parametric representation
28 Horizontal angle correction using straight line detection in an equirectangular image
28 Horizontal angle correction using straight line detection in an equirectangular image 1170283 2017 3 1 2 i Abstract Horizontal angle correction using straight line detection in an equirectangular image
すばる望遠鏡 次世代広視野 補償光学システム (GLAO) 研究代表者 : 有本信雄
すばる望遠鏡 次世代広視野 補償光学システム (GLAO) 研究代表者 : 有本信雄 HSC, PFSに続く TMT 時代のすばる望遠鏡の主力装置 HSC, PFSは暗夜に運用 明夜を担う基幹装置が必要 本装置と系外惑星探査用のPI 装置で明夜の観測を実施 TMTとのサイエンス 技術開発両面でのシナジー 2020 年代のすばるは広視野サーベイでTMTにサンプル供給 典型的なすばる望遠鏡スケジュール
シラバス政治学H18.PDF
- 58 - Introduction to Politics (1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13) (14) (15) (16) (17) (18) (19) (20) (21) http://member.social.tsukuba.ac.jp/tujinaka/ Political Thought http://member.social.tsukuba.ac.jp/kondo/
1 Credit: NASA/JPL-Caltech/R. Hurt SSC-Caltech ,
397 0101 10762 30 e-mail: matsunaga@ioa.s.u-tokyo.ac.jp 8 3 20 2 3 3 7 2 3 1. 100 1912 1 1 4 12 10 3 1 20 2,500 2 1 3 4 374 2012 6 1 Credit: NASA/JPL-Caltech/R. Hurt SSC-Caltech 3 2. 5 3 6 100 7 8, 9 10
2
8 24 32C800037C800042C8000 32 40 45 54 2 3 24 40 10 11 54 4 7 54 30 26 7 9 8 5 6 7 9 8 18 7 7 7 40 10 13 12 24 22 22 8 55 8 8 8 8 1 2 3 18 11 54 54 19 24 30 69 31 40 57 23 23 22 23 22 57 8 9 30 12 12 56
系外惑星大気
transiting planet http://hubblesite.org/newscenter/archive/2001/38/ 2004 6 17 HDS 2 3 (Mayor & Queloz 1995) 4.2 4 (Charbonneau et al. 2000, Henry et al. 2000) HST HST Brown et al. (2001) 5 6 Radial velocity
1 Visible spectroscopy for student Spectrometer and optical spectrum phys/ishikawa/class/index.html
1 Visible spectroscopy for student Spectrometer and optical spectrum http://www.sci.u-hyogo.ac.jp/material/photo phys/ishikawa/class/index.html 1 2 2 2 2.1................................................
untitled
CAPEC, 2009 6 16 June 16, 2009 Page 1 CAPEC EMS 1. EMS USA EU 2. EMS 3. EMS 4. EMS 5. CAPEC 6. EMS June 16, 2009 Page 2 EMS EC 3 EMS EMS EMS EMS CAPEC EMS CAPEC EMS EMS June 16, 2009 Page 3 EU EU EC 1997/67/EC
レーザ誘起蛍光法( LIF法) によるピストンの油膜挙動の解析
Analysis of Piston Oil Film Behavior by Using Laser Induced Fluorescence Method Shuzou Sanda, Akinori Saito ( Laser Induced Fluorescence Method LIF ) LIF Scanning -LIF Abstract Analysis of the oil film
1 [1, 2, 3, 4, 5, 8, 9, 10, 12, 15] The Boston Public Schools system, BPS (Deferred Acceptance system, DA) (Top Trading Cycles system, TTC) cf. [13] [
![1 [1, 2, 3, 4, 5, 8, 9, 10, 12, 15] The Boston Public Schools system, BPS (Deferred Acceptance system, DA) (Top Trading Cycles system, TTC) cf. [13] [](/thumbs/91/106628466.jpg "1 [1, 2, 3, 4, 5, 8, 9, 10, 12, 15] The Boston Public Schools system, BPS (Deferred Acceptance system, DA) (Top Trading Cycles system, TTC) cf. [13] [")
Vol.2, No.x, April 2015, pp.xx-xx ISSN xxxx-xxxx 2015 4 30 2015 5 25 253-8550 1100 Tel 0467-53-2111( ) Fax 0467-54-3734 http://www.bunkyo.ac.jp/faculty/business/ 1 [1, 2, 3, 4, 5, 8, 9, 10, 12, 15] The
Journal of Geography 116 (6) Configuration of Rapid Digital Mapping System Using Tablet PC and its Application to Obtaining Ground Truth
Journal of Geography 116 (6) 749-758 2007 Configuration of Rapid Digital Mapping System Using Tablet PC and its Application to Obtaining Ground Truth Data: A Case Study of a Snow Survey in Chuetsu District,
The History of Marine Machinery before World War II (Part 1. Deck Machinery and etc.) By The Editorial Committee for Marine Engineering History in Japan This paper is an excert from the manuscripts written
Study on Application of the cos a Method to Neutron Stress Measurement Toshihiko SASAKI*3 and Yukio HIROSE Department of Materials Science and Enginee
Study on Application of the cos a Method to Neutron Stress Measurement Toshihiko SASAKI*3 and Yukio HIROSE Department of Materials Science and Engineering, Kanazawa University, Kakuma-machi, Kanazawa-shi,
CONTENTS National Institute of Technology, Nara College 1 Outline of History 2 National Institute of Technology, Nara College 3 4 Organization 5 National Institute of Technology, Nara College Regular courses
Instability of Aerostatic Journal Bearings with Porous Floating Bush at High Speeds Masaaki MIYATAKE *4, Shigeka YOSHIMOTO, Tomoaki CHIBA and Akira CH
Instability of Aerostatic Journal Bearings with Porous Floating Bush at High Speeds Masaaki MIYATAKE *4, Shigeka YOSHIMOTO, Tomoaki CHIBA and Akira CHIBA Department of Mechanical Engineering, Tokyo University
第６２巻 第１号 平成２４年４月／石こうを用いた木材ペレット
Bulletin of Japan Association for Fire Science and Engineering Vol. 62. No. 1 (2012) Development of Two-Dimensional Simple Simulation Model and Evaluation of Discharge Ability for Water Discharge of Firefighting
2
8 23 32A950S 30 38 43 52 2 3 23 40 10 33 33 11 52 4 52 7 28 26 7 8 8 18 5 6 7 9 8 17 7 7 7 38 10 12 9 23 22 22 8 53 8 8 8 8 1 2 3 17 11 52 52 19 23 29 71 29 41 55 22 22 22 22 22 55 8 18 31 9 9 54 71 44
燃焼圧センサ
49 Combustion Pressure Sensor Kouji Tsukada, Masaharu Takeuchi, Sanae Tokumitsu, Yoshiteru Ohmura, Kazuyoshi Kawaguchi π 1000N 150 225N 1 F.S Abstract A new combustion pressure sensor capable of measuring
0810_UIT250_soto
UIT UNIMETER SERIES 250 201 Accumulated UV Meter Digital UV Intensity Meter Research & Development CD Medical Biotech Sterilization Exposure Bonding Manufacturing Curing Production Electronic Components
RTM RTM Risk terrain terrain RTM RTM 48
Risk Terrain Model I Risk Terrain Model RTM,,, 47 RTM RTM Risk terrain terrain RTM RTM 48 II, RTM CSV,,, RTM Caplan and Kennedy RTM Risk Terrain Modeling Diagnostics RTMDx RTMDx RTMDx III 49 - SNS 50 0
<95DB8C9288E397C389C88A E696E6462>
2011 Vol.60 No.2 p.138 147 Performance of the Japanese long-term care benefit: An International comparison based on OECD health data Mie MORIKAWA[1] Takako TSUTSUI[2] [1]National Institute of Public Health,
Title < 論文 > 公立学校における在日韓国 朝鮮人教育の位置に関する社会学的考察 : 大阪と京都における 民族学級 の事例から Author(s) 金, 兌恩 Citation 京都社会学年報 : KJS = Kyoto journal of so 14: 21-41 Issue Date 2006-12-25 URL http://hdl.handle.net/2433/192679 Right
ERINA Report
The Current Status of and Future Prospects for the Automobile Industry in the Central Liaoning City Cluster (with a focus on the core city of Shenyang) (Part One) YASUGI Osamu Deputy Senior Researcher,
宇宙環境利用蛋白質結晶生成応用利用実証プロジェクトのご案内
16 8 23 1. 14 17 ISS JEM (JAXA) 2. JAXA 14 6 1 4 1 02/02/2003 29/08/2003 29/01/2004 11/08/2004 Baikonur Kazakhstan Progress 03/05/2003 28/10/2003 29/04/2004 19/10/2004 Kazakhstan Soyuz 13 weeks 9 weeks
チョークコイル・リアクタ
THIN TRNSORMRS (MPT TYP) OMSTI(JPN) U S I TYP MPT MPT series are available for the thinner-sized sets and suit to I standard. H MPT I KS5535 KS6435 KS7235 KS7250 KS7270 KS9640 KS9660 KS9680 KS00 75.0 67.0
The Phase Behavior of Monooleoylglycerol-Water Systems Mivoshi Oil & Fat Co.. Ltd. Faculty of Science and Technology, Science University of Tokyo Inst
The Phase Behavior of Monooleoylglycerol-Water Systems Mivoshi Oil & Fat Co.. Ltd. Faculty of Science and Technology, Science University of Tokyo Institute of Colloid and Interface Science, Science University