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Conceptual Model of Aquifers in th. Bedrock Zone of th. Marah.uéw.tersh.d (Centre-w.st of Ivory Coast)

Journal of Geoscience and Environment Protection 2022年第7期10卷 229-256页

作者： Kouassi Désiré Bouatrin Innocent Kouassi Kouame Aristide Gountôh.Douagui Kouamé Auguste Kouassi Bi Tié Albert Goula Geosciences and Environment Laboratory Department of Environmental Sciences and Management Nangui University Abrogoua Abidjan Ivory Coast

Marah.ué w.tersh.d, located in th. Center w.st of Côte d’Ivoire, h.s experienced significant population grow.h.in recent decades. And a major economic boom linked to intense agricultural activity and th. presence of certain industries. Th.s population grow.h.is also accompanied by seasonal w.ter sh.rtages. h.nce it needs to better manage th. basin’s groundw.ter, w.ich.is a permanent resource and more resistant th.n surface w.ter to climatic h.zards. Th. objective of th.s study is th.refore to propose a conceptual model of h.drogeological flow.for th. sustainable exploitation of groundw.ter resources in th. Marah.ué w.tersh.d. Th. establish.ent of th. conceptual model w.s carried out in tw. stages. Th. first step consisted in defining th. stratigraph.c units. For th.s purpose, th.ee units h.ve been defined. Th.se are th. layer of alterite, th. useful fissured h.rizon and th. sound basement. Th. th.ckness of th. layer of alterite varies from 0 to 80 m w.th.an average of 26 m. As for th. useful fissured h.rizon, its th.ckness is betw.en 43 and 46.5 w.th.an average of 45 m. In addition, th. roof of th. basement presents a sligh.ly uneven morph.logy w.th.a North.w.st, South.East dip and th. altitudes are betw.en 150 and 390 m. Th. second step corresponds to th. ph.se of determining th. h.drodynamic parameters. During th.s ph.se, th. crack porosity, th. transmissivity, th. conductivity, th. storage coefficient, th. h.drological balance and th. piezometric map w.re determined. Indeed, th.se parameters (th. crack porosity, th. transmissivity, th. conductivity and th. storage coefficient) confirm not only th. h.terogeneity of th. medium but th.t th. cracked h.rizon is sufficiently porous to be assimilated to an equivalent continuous medium during th. simulation.

关键词： Marah.ué w.tersh.d Conceptual Model Ivory Coast

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用于纺制粘胶纱线的新式TB转杯

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国际纺织导报 2007年第6期35卷 22-23页

作者： w.Jansen I．Biermann 刘肖燕（译）李毓陵（校）苏拉集团赐来福公司德国不详

技术设备简化纱线生产,目前采用新式装置的Autocoro粘胶纺纱厂在全球范围内粘胶的蓬勃发展中大大受益。粘胶纺纱的革新大大改善了粘胶纺织品的物理性能、外观和手感。不过一些参数像切断长度也在纺织生产的各流程中发挥着重要的作用。

关键词：粘胶纱线纺纱转杯

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加拉帕戈斯群岛移民和海参危机实例研究

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AMBIO－人类环境杂志 2002年第4期31卷 306-310页

作者： Jason Bremner M.P.h.Jaime Perez 章任群北卡罗莱纳大学

加拉帕戈斯海参捕捞危机是由于大量的移民涌入、激烈的经济竞争以及软弱无力的管理机构所造成的一个典型例子。短时期内,海参捕捞已经成为加拉帕戈斯地区最有煽动性的争议问题。就对新的海洋资源进行高效捕捞来说关键因素并不是渔民本身... 详细信息

加拉帕戈斯海参捕捞危机是由于大量的移民涌入、激烈的经济竞争以及软弱无力的管理机构所造成的一个典型例子。短时期内,海参捕捞已经成为加拉帕戈斯地区最有煽动性的争议问题。就对新的海洋资源进行高效捕捞来说关键因素并不是渔民本身,而是新的捕捞技术、银行贷款和水产市场。这说明造成每年海参捕捞危机的原因非常复杂而不仅仅因为不断增多的渔民加大了海参的捕捞量。本文通过人口普查数据和渔民注册登记数据分析了该群岛人口的增长情况。还通过一项民意调查来确定人们对海参捕捞和有关规定的态度。定性的采访揭示了海参繁荣的历史,同时海参监测信息也提供了年海参捕捞量的估计值。

关键词：捕捞业资源危机加拉帕戈斯群岛移民海参

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伴有皮质下梗死和脑白质病变的常染色体显性遗传性脑血管病MR异常表现的进程:前瞻性7年随访研究

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国际医学放射学杂志 2009年第1期32卷 78-78页

作者： M.K. Liem S.A. Lesnik Oberstein J. h.an I.L. van der Neut R. van den boom M.D. Ferrari 陈仁彪 Department of Radiology Leiden University Medical Center Albinusdreef 2 2333 ZA Leiden the Netherlands

目的对伴有皮质下梗死和脑白质病变的常染色体显性遗传性脑血管病病人的MRI异常表现进展的方式和比率进行了基线后7年的前瞻性研究，确定影响进展方式和比率的预后因素。材料和方法当地的伦理委员会批准了该项研究．并获得了所有参... 详细信息

目的对伴有皮质下梗死和脑白质病变的常染色体显性遗传性脑血管病病人的MRI异常表现进展的方式和比率进行了基线后7年的前瞻性研究，确定影响进展方式和比率的预后因素。材料和方法当地的伦理委员会批准了该项研究．并获得了所有参与者的知情同意。来自12个互不相关的家庭的25例NOTCh.突变携带者以及13例非突变携带者在基线年以及基线后7年均进行了临床检查和标准化MMR成像。

关键词：常染色体显性遗传性显性遗传性脑血管病脑白质病变皮质下梗死 MRI 随访研究脑血管病病人伦理委员会

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炼厂烷基化技术的未来:安全与辛烷值之间的平衡

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中外能源 2015年第5期20卷 80-84页

作者： Patrick J.Ch.istensen 杨永泰美国烃出版公司美国宾夕法尼亚19399

因汽油池中的乙醇用量越来越多,为了平衡乙醇较高的RVP值,生产商必须寻找低RVP值的调和组分。持续的页岩热潮带来了充足且廉价的丁烷,同时由于致密油中含大量链烷烃,通常会使FCC汽油的辛烷值平均降低8~10个单位,这就造成了对高辛烷值汽... 详细信息

因汽油池中的乙醇用量越来越多,为了平衡乙醇较高的RVP值,生产商必须寻找低RVP值的调和组分。持续的页岩热潮带来了充足且廉价的丁烷,同时由于致密油中含大量链烷烃,通常会使FCC汽油的辛烷值平均降低8~10个单位,这就造成了对高辛烷值汽油调和组分的需求。这些因素为烷基化运营商带来了巨大的机遇。世界已建的烷基化产能和商业技术中,液体酸（h.SO4和h.）烷基化技术一直占主导地位,因该技术有安全隐患,北美和欧洲的新建装置基本上已停止使用这种工艺技术。技术许可商已致力于开发烷基化技术的替代方案。UOP的间接烷基化工艺（InALKTM）既适用于新建装置,也适合于对现有MTBE装置改造后应用。有的炼厂对现有h.装置进行改造,再用固体酸替代h.。离子液体（ILS）在烷基化反应体系中既可作为溶剂也可作为催化剂,而且催化性能更好。Uh.e公司将STAR工艺与齐聚技术整合为完整的丁烷转化为烷基化油的工艺方案。预计固体酸烷基化和离子液体烷基化技术未来的研发工作将集中于如何更长期地保持催化剂的活性和选择性,同时提高催化剂的再生能力。利用烷基化装置生产中间馏分油是最具吸引力的选择。

关键词：烷基化技术乙醇烷基化油 FCC汽油液体酸固体酸离子液体辛烷值

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重型采矿设备的疲劳寿命预测第一部分:疲劳荷载评估和裂纹发展速度试验

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钢结构 2008年第6期23卷 88-88页

作者： G.Y. Grondin K.h. Obaia A.E. Elw.

重型采矿设备的疲劳寿命预测十分重要。首先,对早已存在有慢性疲劳裂纹的铲矿机起动臂进行现场监测,从监测数据中归纳了吊杆的载荷范围。针对试验数据,建立吊杆的有限元模型来预测其压应力和应变。进行了8个裂纹发展速度试验,获得使用... 详细信息

重型采矿设备的疲劳寿命预测十分重要。首先,对早已存在有慢性疲劳裂纹的铲矿机起动臂进行现场监测,从监测数据中归纳了吊杆的载荷范围。针对试验数据,建立吊杆的有限元模型来预测其压应力和应变。进行了8个裂纹发展速度试验,获得使用材料的疲劳特性。基于Palmgren-Miner’s累积损坏原则和裂纹发展速度的试验结果,计算出恒振幅的换算应力范围。

关键词：重型采矿设备疲劳现场试验裂纹发展速度试验疲劳载荷范围换算应力范围

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Feasibility and ph.sics potential of detecting ^(8)B solar neutrinos at JUNO

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Ch.nese Ph.sics C 2021年第2期45卷 93-110页

作者： Angel Abusleme Th.mas Adam Sh.keel Ah.ad Sebastiano Aiello Muh.mmad Akram Naw.b Ali Fengpeng An Guangpeng An Qi An Giuseppe Andronico Nikolay Anfimov Vito Antonelli Tatiana Antosh.ina Burin Asavapibh.p João Pedro Ath.yde Marcondes de André Didier Auguste Andrej Babic w.nder Baldini Andrea Barresi Eric Baussan Marco Bellato Antonio Bergnoli Enrico Bernieri David Biare Th.lo Birkenfeld Sylvie Blin David Blum Simon Blyth.Anastasia Bolsh.kova Math.eu Bongrand Clément Bordereau Dominique Breton Augusto Brigatti Riccardo Brugnera Riccardo Bruno Antonio Budano Max Buesken Mario Buscemi Jose Busto Ilya Butorov Anatael Cabrera h.o Cai Xiao Cai Yanke Cai Zh.yan Cai Antonio Cammi Agustin Campeny Ch.anya Cao Guofu Cao Jun Cao Rossella Caruso Cédric Cerna Jinfan Ch.ng Yun Ch.ng Pingping Ch.n Po-An Ch.n Sh.omin Ch.n Sh.njian Ch.n Xurong Ch.n Yi-w.n Ch.n Yixue Ch.n Yu Ch.n Zh.ng Ch.n Jie Ch.ng Yaping Ch.ng Alexander Ch.purnov Davide Ch.esa Pietro Ch.menti Artem Ch.kanov Anna Ch.vash.va Gérard Claverie Catia Clementi Barbara Clerbaux Selma Conforti Di Lorenzo Daniele Corti Salvatore Costa Flavio Dal Corso Ch.istoph. De La Taille Jiaw.i Deng Zh. Deng Ziyan Deng w.lfried Depnering Marco Diaz Xuefeng Ding Yayun Ding Bayu Dirgantara Sergey Dmitrievsky Tadeas Doh.al Georgy Donch.nko Jianmeng Dong Damien Dornic Evgeny Dorosh.evich.Marcos Dracos Frédéric Druillole Sh.xian Du Stefano Dusini Martin Dvorak Timo Enqvist h.ike Enzmann Andrea Fabbri Lukas Fajt Dongh.a Fan Lei Fan Can Fang Jian Fang Marco Fargetta Anna Fatkina Dmitry Fedoseev Vladko Fekete Li-Ch.ng Feng Qich.n Feng Rich.rd Ford Andrey Formozov Amélie Fournier h.onan Gan Feng Gao Alberto Garfagnini Alexandre Göttel Ch.istoph.Genster Marco Giammarch. Agnese Giaz Nunzio Giudice Franco Giuliani Maxim Gonch.r Guangh.a Gong h.i Gong Oleg Gorch.kov Yuri Gornush.in Marco Grassi Ch.istian Grew.ng Maxim Gromov Vasily Gromov Mingh.o Gu Xiaofei Gu Yu Gu Mengyun Guan Nunzio Guardone Maria Gul Cong Guo Jingyuan Guo w.nlei Guo Xinh.ng Guo Yuh.ng Guo Paul h.ckspach.r Caren h.gner Ran h.n Yan Yerevan Ph.sics Institute YerevanArmenia UniversitéLibre de Bruxelles BrusselsBelgium Universidade Estadual de Londrina LondrinaBrazil Pontificia Universidade Catolica do Rio de Janeiro RioBrazil Pontificia Universidad Católica de Ch.le SantiagoChile Universidad Tecnica Federico Santa Maria ValparaisoChile Beijing Institute of Spacecraft Environment Engineering BeijingChina Beijing Normal University BeijingChina Ch.na Institute of Atomic Energy BeijingChina Institute of h.gh.Energy Ph.sics BeijingChina North.Ch.na Electric Pow.r University BeijingChina Sch.ol of Ph.sics Peking UniversityBeijingChina Tsingh.a University BeijingChina University of Ch.nese Academy of Sciences BeijingChina Jilin University ChangchunChina College of Electronic Science and Engineering National University of Defense TechnologyChangshaChina Ch.ngqing University ChongqingChina Dongguan University of Tech.ology DongguanChina Jinan University GuangzhouChina Sun Yat-Sen University GuangzhouChina h.rbin Institute of Tech.ology HarbinChina University of Science and Tech.ology of Ch.na HefeiChina Th. Radioch.mistry and Nuclear Ch.mistry Group in University of South.Ch.na HengyangChina w.yi University JiangmenChina Sh.ndong University JinanChina Institute of Modern Ph.sics Chinese Academy of SciencesLanzhouChina Nanjing University NanjingChina Guangxi University NanningChina East Ch.na University of Science and Tech.ology ShanghaiChina Sch.ol of Ph.sics and Astronomy Shanghai Jiao Tong UniversityShanghaiChina Tsung-Dao Lee Institute Shanghai Jiao Tong UniversityShanghaiChina Institute of h.drogeology and Environmental Geology Chinese Academy of Geological SciencesShijiazhuangChina Nankai University TianjinChina w.h.n University WuhanChina Xi’an Jiaotong University Xi’anChina Xiamen University XiamenChina Sch.ol of Ph.sics and Microelectronics Zhengzhou UniversityZhengzhouChina Institute of Ph.sics National Ch.ao-Tung University Hsinchu National United University Miao-Li Department of Ph.sics National T

Th. Jiangmen Underground Neutrino Observatory(JUNO)features a 20 kt multi-purpose underground liquid scintillator sph.re as its main *** of JUNO's features make it an excellent location for^8B solar neutrino measurements,such.as its low.energy th.esh.ld,h.gh.energy resolution compared w.th.w.ter Ch.renkov detectors,and much.larger target mass compared w.th.previous liquid scintillator *** th.s paper,w. present a compreh.nsive assessment of JUNO's potential for detecting^8B solar neutrinos via th. neutrino-electron elastic scattering process.A reduced 2 MeV th.esh.ld for th. recoil electron energy is found to be ach.evable,assuming th.t th. intrinsic radioactive background^(238)U and^(232)Th.in th. liquid scintillator can be controlled to 10^(-17)g/*** ten years of data acquisition,approximately 60,000 signal and 30,000 background events are *** large sample w.ll enable an examination of th. distortion of th. recoil electron spectrum th.t is dominated by th. neutrino flavor transformation in th. dense solar matter,w.ich.w.ll sh.d new.ligh. on th. inconsistency betw.en th. measured electron spectra and th. predictions of th. standard th.ee-flavor neutrino oscillation *** m^(2)_(21)=4.8times10^(-5);(7.5times10^(-5))eV^(2),JUNO can provide evidence of neutrino oscillation in th. Earth.at approximately th. 3sigma(2sigma)level by measuring th. non-zero signal rate variation w.th.respect to th. solar zenith.***,JUNO can simultaneously measureDelta m^2_(21)using^8B solar neutrinos to a precision of 20% or better,depending on th. central value,and to sub-percent precision using reactor antineutrinos.A comparison of th.se tw. measurements from th. same detector w.ll h.lp understand th. current mild inconsistency betw.en th. value of Delta m^2_(21)reported by solar neutrino experiments and th. KamLAND experiment.

关键词： neutrino oscillation solar neutrino JUNO

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JUNO sensitivity on proton decay p→νK^(+)search.s

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Ch.nese Ph.sics C 2023年第11期47卷 7-22页

作者： Angel Abusleme Th.mas Adam Sh.keel Ah.ad Rizw.n Ah.ed Sebastiano Aiello Muh.mmad Akram 安丰鹏安琪 Giuseppe Andronico Nikolay Anfimov Vito Antonelli Tatiana Antosh.ina Burin Asavapibh.p João Pedro Ath.yde Marcondes de André Didier Auguste Nikita Balash.v w.nder Baldini Andrea Barresi Davide Basilico Eric Baussan Marco Bellato Antonio Bergnoli Th.lo Birkenfeld Sylvie Blin David Blum Simon Blyth.Anastasia Bolsh.kova Math.eu Bongrand Clément Bordereau Dominique Breton Augusto Brigatti Riccardo Brugnera Riccardo Bruno Antonio Budano Mario Buscemi Jose Busto Ilya Butorov Anatael Cabrera Barbara Caccianiga 蔡浩蔡啸蔡严克蔡志岩 Riccardo Callegari Antonio Cammi Agustin Campeny 曹传亚曹国富曹俊 Rossella Caruso Cédric Cerna 常劲帆 Yun Ch.ng 陈平平 Po-An Ch.n 陈少敏陈旭荣 Yi-w.n Ch.n 陈义学陈羽陈长程捷程雅苹 Alexey Ch.tverikov Davide Ch.esa Pietro Ch.menti Artem Ch.kanov Gérard Claverie Catia Clementi Barbara Clerbaux Selma Conforti Di Lorenzo Daniele Corti Flavio Dal Corso Olivia Dalager Ch.istoph. De La Taille 邓智邓子艳 w.lfried Depnering Marco Diaz Xuefeng Ding 丁雅韵 Bayu Dirgantara Sergey Dmitrievsky Tadeas Doh.al Dmitry Dolzh.kov Georgy Donch.nko 董建蒙 Evgeny Dorosh.evich.Marcos Dracos Frédéric Druillole 杜然杜书先 Stefano Dusini Martin Dvorak Timo Enqvist h.ike Enzmann Andrea Fabbri Ulrike Fah.endh.lz 范东华樊磊方建方文兴 Marco Fargetta Dmitry Fedoseev Li-Ch.ng Feng 冯启春 Rich.rd Ford Amélie Fournier 甘浩男 Feng Gao Alberto Garfagnini Arsenii Gavrikov Marco Giammarch. Agnese Giaz Nunzio Giudice Maxim Gonch.r 龚光华宫辉 Yuri Gornush.in Alexandre Göttel Marco Grassi Ch.istian Grew.ng Vasily Gromov 顾旻皓谷肖飞古宇关梦云 Nunzio Guardone Maria Gul 郭聪郭竞渊郭万磊郭新恒郭宇航 Paul h.ckspach.r Caren h.gner 韩然 Yang h.n Muh.mmad Soh.ib h.ssan 何苗何伟 Tobias h.inz Patrick h.llmuth.衡月昆 Rafael h.rrera 贺远强侯少静 Yee h.iung Bei-Zh.n h. 胡航胡健润胡俊胡守扬胡涛胡宇翔胡焯钧黄春豪黄桂鸿黄翰雄黄文昊黄鑫黄性涛黄永波惠加琪霍雷霍文驹 Cédric h.ss Safeer h.ssain Ara Ioannisian Roberto Isocrate Beatrice Jelmini Kuo-Lun Jen Ignacio Jeria 季筱璐吉星曌贾慧慧贾俊基蹇司玉蒋荻蒋炜江晓山金如意荆小平 Cécile Jollet Jari Joutsenvaara Sirich.k Jungth.w.n Leonidas Kalousis Ph.lipp Ka Pontificia Universidad Católica de Ch.le SantiagoChile IPh. Universitéde StrasbourgCNRS/IN2P3F-67037 StrasbourgFrance Pakistan Institute of Nuclear Science and Tech.ology IslamabadPakistan INFN Catania and Dipartimento di Fisica e Astronomia dell Universitàdi Catania CataniaItaly East Ch.na University of Science and Tech.ology ShanghaiChina University of Science and Tech.ology of Ch.na HefeiChina Joint Institute for Nuclear Research DubnaRussia INFN Sezione di Milano and Dipartimento di Fisica dell Universitàdi Milano MilanoItaly Department of Ph.sics Faculty of ScienceChulalongkorn UniversityBangkokThailand IJCLab UniversitéParis-SaclayCNRS/IN2P391405 OrsayFrance Department of Ph.sics and Earth.Science University of Ferrara and INFN Sezione di FerraraFerraraItaly INFN Milano Bicocca and University of Milano Bicocca MilanoItaly INFN Sezione di Padova PadovaItaly III.Ph.sikalisch.s Institut B RWTH Aachen UniversityAachenGermany Eberh.rd Karls Universität Tübingen Physikalisches InstitutTübingenGermany Institute of h.gh.Energy Ph.sics BeijingChina SUBATECh Universitéde NantesIMT AtlantiqueCNRS-IN2P3NantesFrance Univ.Bordeaux CNRSLP2IUMR 5797F-33170 GradignanFrance Department of Ph.sics National Taiwan UniversityTaipei Dipartimento di Fisica e Astronomia dell’Universitàdi Padova and INFN Sezione di Padova PadovaItaly University of Roma Tre and INFN Sezione Roma Tre RomaItaly Aix Marseille Univ CNRS/IN2P3CPPMMarseilleFrance w.h.n University WuhanChina INFN Milano Bicocca and Politecnico of Milano MilanoItaly National United University Miao-Li Dongguan University of Tech.ology DongguanChina Tsingh.a University BeijingChina Institute of Modern Ph.sics Chinese Academy of SciencesLanzhouChina Institute of Ph.sics National Yang Ming Chiao Tung UniversityHsinchu North.Ch.na Electric Pow.r University BeijingChina Sun Yat-Sen University GuangzhouChina Beijing Institute of Spacecraft Environment Engineering BeijingChina Universidade Estadual de Londrina LondrinaBrazil INFN Sez

Th. Jiangmen Underground Neutrino Observatory(JUNO)is a large liquid scintillator detector designed to explore many topics in fundamental *** th.s study,th. potential of search.ng for proton decay in th. p→νK^(+)mode w.th.JUNO is *** kaon and its decay particles feature a clear th.ee-fold coincidence signature th.t results in a h.gh.efficiency for ***,th. excellent energy resolution of JUNO permits suppression of th. sizable background caused by oth.r delayed *** on th.se advantages,th. detection efficiency for th. proton decay via p→νK^(+)is 36.9%±4.9%w.th.a background level of 0.2±0.05(syst)±0.2(stat)events after 10 years of data *** estimated sensitivity based on 200 kton-years of exposure is 9.6×1033 years,w.ich.is competitive w.th.th. current best limits on th. proton lifetime in th.s ch.nnel and complements th. use of different detection tech.ologies.

关键词： proton decay grand unified th.ories JUNO liquid scintillator detector

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