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CEPC Technical Design Report

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Radiation Detection Technology and Methods 2024年第1期8卷 I0003-I0016,1-1091页

作者： Waleed Abdallah Tiago Carlos Adorno de Freitas Konstantin Afanaciev Shakeel Ahmad Ijaz Ahmed xiaocong Ai Abid Aleem Wolfgang Altmannshofer Fabio Alves Weiming An Rui An Daniele Paolo Anderle Stefan Antusch Yasuo Arai Andrej Arbuzov Abdesslam Arhrib Mustafa Ashry Sha Bai Yu Bai yang Bai Vipul Bairathi Csaba Balazs Philip Bambade yong Ban Tripamo Bandyopadhyay Shou-Shan Bao Desmond P.Barber Ayse Bat Varvara Batozskaya Subash Chandra Behera Alexander Belyaev Michele Bertucci xiao-Jun Bi Yuanjie Bi tianjian Bian Fabrizio Bianchi Thomas Biekotter Michela Biglietti Shalva Bilanishvili Deng binglin Denis Bodrov Anton Bogomyagkov Serge Bondarenko Stewart Boogert Maarten Boonekamp Marcello Borri Angelo Bosotti Vincent Boudry Mohammed Boukidi Igor Boyko Ivanka Bozovic Giuseppe Bozzi Jean-Claude Brient Anastasiia Budzinskaya Masroor Bukhari Vladimir Bytev Giacomo Cacciapaglia Hua cai wenyong cai Wujun cai Yijian cai Yizhou cai Yuchen cai Haiying cai Huacheng cai Lorenzo Calibbi Junsong Cang Guofu Cao Jianshe Cao Antoine Chance xuejun Chang Yue Chang Zhe Chang Xinyuan Chang Wei Chao Auttakit Chatrabhuti Yimin Che Yuzhi Che bin Chen Danping Chen Fuqing Chen Fusan Chen Gang Chen Guoming Chen Hua-Xing Chen Huirun Chen Jinhui Chen Ji-Yuan Chen Kai Chen Mali Chen mingjun Chen mingshui Chen Ning Chen Shanhong Chen Shanzhen Chen Shao-Long Chen Shaomin Chen shiqiang Chen tianlu Chen Wei Chen xiang Chen xiaoyu Chen Xin Chen Xun Chen Xurong Chen Ye Chen ying Chen Yukai Chen Zelin Chen Zilin Chen Gang Chen Boping Chen Chunhui Chen Hok Chuen Cheng Huajie Cheng Shan Cheng Tongguang Cheng Yunlong Chi Pietro Chimenti wen han Chiu Guk Cho ming-Chung Chu xiaotong Chu Ziliang Chu Guglielmo Coloretti Andreas Crivellin hanhua cui xiaohao cui zhaoyuan cui Brunella D'Anzi Ling-Yun Dai Xinchen Dai Xuwen Dai Antonio De Maria Nicola De Filippis Christophe De La Taille Francesca De Mori Chiara De Sio Elisa Del Core Shuangxue Deng Wei-tian Deng Zhi Deng Ziyan Deng Bhupal Dev Tang Dewen Biagio Di Micco Ran Ding Siqin Dingl Yadong Ding Haiyi Dong Jianin AGH University of Science and Technology Faculty of Physics and Applied Computer ScienceKrakow Anhui University HefeiAnhui Applied Physics Department Federal Urdu University of ArtsScience and TechnologyIslamabad Banaras Hindu University Institute of ScienceVaranasi Bandirma Onyedi Eylul University Bandirma Beihang University Beijing Beijing Computational Science Research Center Beijing Beijing Conveyi LTD Beijing Beijing Glass Research Institute Co. LtdBeijing Beijing Institute of Technology Beijing Beijing Normal University Beijing Brown University ProvidenceRI Budker Institute of Nuclear Physics Novosibirsk Cadi Ayyad University Laboratory of Fundamental and Applied PhysicsPolydisciplinary FacultyMarrakech cairo University Giza Center for Theory and Computation National Tsing Hua UniversityHsinchu Central China Normal University WuhanHubei Central South University ChangshaHunan Centro de Fisica Teorica de Particulas Universidade Tecnica de LisboaLisboa Chengdu KaitengSifang Digital Radio&TV Equipment Co. LtdChengduSichuan China academy of engineering physics MianyangSichuan China building materials academy Beijing China Center of Advanced Science and Technology Beijing China Institute of Atomic Energy Beijing China Jiliang University HangzhouZhejiang China Nuclear Instrument CO. LTDBeijing China University of Geosciences Beijing China University of Geosciences WuhanHubei China University of Mining and Technology XuzhouJiangsu China West Normal University NanchongSichuan Chongqing University Department of PhysicsChongqing Chulalongkorn University Bangkok City University of Hong Kong Department of PhysicsHong Kong Cockcroft Institute Daresbury Cornell University IthacaNY CPPM(AMU/IPhU&CNRS/INP) Marseille Dalian Minzu University DalianLiaoning Dalian University of Technology Department of PhysicsDalian Deutsches Elektronen-Synchrotron DESY Hamburg Dzhelepov Laboratory of Nuclear Problems of Joint Institute for Nuclear Research(DLNP JINR) Dubna East China University Of Science And Technol

The Circular Electron Positron Collider(CEPC)is a large scientific project initiated and hosted by China,fostered through extensive collaboration with international *** complex comprises four accelerators:a 30 GeV Linac,a 1.1 GeV Damping Ring,a Booster capable of achieving energies up to 180 GeV,and a Collider operating at varying energy modes(Z,W,H,and tt).The Linac and Damping Ring are situated on the surface,while the subterranean Booster and Collider are housed in a 100 km circumference underground tunnel,strategically accommodating future expansion with provisions for a potential Super Proton Proton Collider(SPPC).The CEPC primarily serves as a Higgs *** its baseline design with synchrotron radiation(SR)power of 30 MW per beam,it can achieve a luminosity of 5×10^(34)cm^(-2)s^(-1)per interaction point(IP),resulting in an integrated luminosity of 13 ab^(-1)for two IPs over a decade,producing 2.6 million Higgs *** the SR power to 50 MW per beam expands the CEPC's capability to generate 4.3 million Higgs bosons,facilitating precise measurements of Higgs coupling at sub-percent levels,exceeding the precision expected from the HL-LHC by an order of *** Technical Design Report(TDR)follows the Preliminary Conceptual Design Report(Pre-CDR,2015)and the Conceptual Design Report(CDR,2018),comprehensively detailing the machine's layout,performance metrics,physical design and analysis,technical systems design,R&D and prototyping efforts,and associated civil engineering ***,it includes a cost estimate and a preliminary construction timeline,establishing a framework for forthcoming engineering design phase and site selection *** is anticipated to begin around 2027-2028,pending government approval,with an estimated duration of 8 *** commencement of experiments and data collection could potentially be initiated in the mid-2030s.

关键词： initiated exceeding precise

Data release of the LAMOST pilot survey

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Research in Astronomy and Astrophysics 2012年第9期12卷 1243-1246页

作者： A-Li luo Hao-Tong zhang yong-Heng zhao Gang zhao xiang-Qun cui Guo-Ping Li Yao-Quan Chu Jian-rong shi Gang wang Jian-Nan zhang Zhong-Rui Bai xiao-yan Chen Feng-Fei wang yan-Xin Guo Jian-Jun Chen bing Du xiao Kong Ya-Juan Lei yin-Bi Li Yi-han Song Yue Wu yan-xia zhang Xin-Lin zhou Fang Zuo Peng Du Lin He wen Hou Yi-Qiao Dong Jian Li Guang-Wei Li Shuang Li Jing Song Yuan tian Meng-Xin wang yong-Hui Hou Zhi-ying Huo Hong-Zhuan Hu Ning-Sheng Hu Zhong-wen Hu Lei Jia Fang-Hua jiang xiang jiang Zi-Bo jiang Ge Jin Ai-Hua Li Qi Li yin-Dun Mao Zheng-Hong Tang qing-Sheng Tao Liang-Ping Tu Da-qing wang Dan wang Jian-Ping wang Lei wang Shou-Guan wang Shu-qing wang Ya-Nan wang You wang Yue-Fei wang ming-Zhi Wei xiang-xiang xue xiao-Zheng Xing Ling-Zhe Xu Xin-Qi Xu yan Xu De-Hua yang shi-Hai yang Zheng-Qiu Yao yong Yu Hui Yuan Chao Zhai En-Peng zhang Jing zhang Li-Ping zhang Weizhang yong zhang Zhen-Chao zhang ming zhao Fang zhou yong-tian Zhu Jie Zhu Si-Cheng Zou National Astronomical Observatories Chinese Academy of Sciences Beijing 100012 China lal @ lamost o rg Nanjing Institute of Astronomical Optics and Technology National Astronomical ObservatoriesChinese Academy of Sciences Nanjing 210042 China University of Science and Technologyof China Hefei 230026 China Shanghai Astronomical Observatory Chinese Academy of Sciences Shanghai 200030 China Institute of Architecture Design and Research Chinese Academy of Sciences Beijing 100190China

This paper describes the data release of the LAMOST pilot survey, which includes data reduction, calibration, spectral analysis, data products and data access. The accuracy of the released data and the information about the FITS headers of spectra are also introduced. The released data set includes 319 000 spectra and a catalog of these objects.

关键词： techniques: spectroscopic survey — data reduction — data release

The first data release(DR1) of the LAMOST regular survey

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Research in Astronomy and Astrophysics 2015年第8期15卷 1095-1124页

作者： A-Li luo yong-Heng zhao Gang zhao Li-cai Deng xiao-Wei Liu Yi-Peng Jing Gang wang Hao-Tong zhang Jian-rong shi xiang-Qun cui Yao-Quan Chu Guo-Ping Li Zhong-Rui Bai Yue Wu yan cai Shu-Yun Cao Zi-Huang Cao Jeffrey L.Carlin Hai-Yuan Chen Jian-Jun Chen Kun-Xin Chen Li Chen xue-Lei Chen xiao-yan Chen ying Chen Norbert Christlieb Jia-Ru Chu Chen-zhou cui Yi-Qiao Dong bing Du Dong-Wei Fan Lei Feng Jian-Ning Fu Peng Gao xue-Fei Gong Bo-Zhong Gu yan-Xin Guo Zhan-wen han Bo-Liang He Jin-Liang Hou yong-Hui Hou wen Hou Hong-Zhuan Hu Ning-Sheng Hu Zhong-wen Hu Zhi-ying Huo Lei Jia Fang-Hua jiang xiang jiang Zhi-Bo jiang Ge Jin xiao Kong Xu Kong Ya-Juan Lei Ai-Hua Li Chang-Hua Li Guang-Wei Li Hai-Ning Li Jian Li Qi Li Shuang Li Sha-Sha Li Xin-Nan Li yan Li yin-Bi Li Ye-Ping Li Yuan Liang Chien-Cheng Lin Chao Liu Gen-rong Liu Guan-Qun Liu Zhi-Gang Liu wen-Zhi Lu Yu luo yin-Dun Mao Heidi Newberg Ji-Jun Ni zhao-xiang Qi yong-Jun Qi shi-yin Shen Huo-ming shi Jing Song Yi-han Song Ding-Qiang Su Hong-Jun Su Zheng-Hong Tang qing-Sheng Tao Yuan tian Dan wang Da-Qi wang Feng-Fei wang Guo-Min wang Hai wang Hong-Chi wang Jian wang Jia-Ning wang Jian-Ling wang Jian-Ping wang Jun-xian wang Lei wang Meng-Xin wang Shou-Guan wang Shu-qing wang xia wang Ya-Nan wang You wang Yue-Fei wang You-Fen wang Peng Wei ming-Zhi Wei Hong Wu Ke-Fei Wu xue-bing Wu Yu-Zhong Wu xiao-Zheng Xing Ling-Zhe Xu Xin-Qi Xu yan Xu Tai-Sheng yan De-Hua yang Hai-Feng yang Hui-Qin yang ming yang Zheng-Qiu Yao yong Yu Hui Yuan Hai-Bo Yuan Hai-Long Yuan Wei-Min Yuan Chao Zhai En-Peng zhang Hua-Wei zhang Jian-Nan zhang Li-Pin zhang Wei zhang yong zhang yan-xia zhang Zheng-Chao zhang ming zhao Fang zhou Xu zhou Jie Zhu yong-tian Zhu Si-Cheng Zou Fang Zuo National Astronomical Observatories Chinese Academy of Sciences Department of Astronomy Peking University Shanghai Astronomical Observatory Chinese Academy of Sciences Nanjing Institute of Astronomical Optics & Technology National Astronomical ObservatoriesChinese Academy of Sciences University of Science and Technology of China Department of Physics Applied Physics and AstronomyRensselaer Polytechnic InstituteTroyNY 12180USA Department of Physics and Astronomy Earlham CollegeRichmondIN 47374USA Universitt Heidelberg Zentrum für AstronomieLandessternwarteKnigstuhl 1269117 HeidelbergGermany Department of Astronomy Beijing Normal University Yunnan Observatories Chinese Academy of Sciences Purple Mountain Observatory Chinese Academy of Sciences

The Large sky Area Multi-Object Fiber Spectroscopic Telescope（LAMOST） general survey is a spectroscopic survey that will eventually cover approximately half of the celestial sphere and collect 10 million spectra of stars, galaxies and QSOs. Objects in both the pilot survey and the first year regular survey are included in the LAMOST DR1. The pilot survey started in October 2011 and ended in June 2012, and the data have been released to the public as the LAMOST Pilot Data Release in August 2012. The regular survey started in September 2012, and completed its first year of operation in June 2013. The LAMOST DR1 includes a total of 1202 plates containing 2 955 336 spectra, of which 1 790 879 spectra have observed signalto-noise ratio（SNR） ≥ 10. All data with SNR ≥ 2 are formally released as LAMOST DR1 under the LAMOST data policy. This data release contains a total of 2 204 696 spectra, of which 1 944 329 are stellar spectra, 12 082 are galaxy spectra and 5017 are quasars. The DR1 not only includes spectra, but also three stellar catalogs with measured parameters： late A,FGK-type stars with high quality spectra（1 061 918 entries）, A-type stars（100 073 entries）, and M-type stars（121 522 entries）. This paper introduces the survey design, the observational and instrumental limitations, data reduction and analysis, and some caveats. A description of the FITS structure of spectral files and parameter catalogs is also provided.

关键词： techniques: spectroscopic survey—data release—catalog

Timing analysis of the black hole candidate EXO 1846–031 with Insight-HXMT monitoring

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Research in Astronomy and Astrophysics 2021年第3期21卷 193-204页

作者： He-Xin Liu Yue Huang Guang-Cheng xiao qing-cui Bu Jin-Lu Qu Shu zhang Shuang-Nan zhang Shu-Mei Jia Fang-Jun Lu xiang Ma Lian Tao Wei zhang Li Chen Li-ming Song Ti-Pei Li Yu-Peng Xu xue-Lei Cao yong Chen Cong-Zhan Liu Ce cai Zhi Chang Gang Chen tian-xiang Chen Yi-Bao Chen Yu-Peng Chen Wei cui Wei-Wei cui Jing-Kang Deng yong-Wei Dong Yuan-Yuan Du Min-xue Fu Guan-Hua Gao He Gao Min Gao ming-Yu Ge Yu-Dong Gu Ju Guan Cheng-Cheng Guo Da-Wei han Jia Huo Lu-Hua jiang Wei-Chun jiang Jing Jin yong-Jie Jin Ling-Da Kong bing Li Cheng-Kui Li Gang Li Mao-Shun Li Wei Li xian Li xiao-Bo Li Xu-Fang Li yang-Guo Li Zheng-Wei Li xiao-Hua Liang Jing-Yuan Liao Bai-Sheng Liu Guo-qing Liu Hong-Wei Liu xiao-Jing Liu Yi-Nong Liu Bo Lu xue-Feng Lu Qi luo Tao luo bin Meng Yi Nang Jian-yin Nie Ge Ou Na Sai Ren-Cheng Shang Xin-ying Song Liang Sun ying Tan You-Li Tuo Chen wang Guo-Feng wang Juan wang Ling-Jun wang weng-Shuai wang Yu-Sa wang xiang-yang wen Bai-yang Wu Bo-bing Wu Mei Wu Shuo xiao Shao-Lin Xiong He Xu Jia-Wei yang Sheng yang yan-Ji yang Yi-Jung yang Qi-bin Yi Qian-qing yin Yuan You Ai-Mei zhang Cheng-Mo zhang Fan zhang Hong-Mei zhang Juan zhang Tong zhang Wan-Chang zhang wen-zhao zhang Yi zhang Yi-Fei zhang yong-Jie zhang Yuan-hang zhang Yue zhang zhao zhang Zhi zhang Zi-Liang zhang Hai-Sheng zhao xiao-Fan zhao shi-Jie Zheng Yao-Guang Zheng Deng-Ke zhou Jian-Feng zhou Yu-Xuan Zhu Ren-Lin Zhuang Yue Zhu Key Laboratory of Particle Astrophysics Institute of High Energy PhysicsChinese Academy of SciencesBeijing 100049China University of Chinese Academy of Sciences Chinese Academy of SciencesBeijing 100049China Institut fur Astronomie und Astrophysik Kepler Center for Astro and Particle PhysicsEberhard Karls Universität72076 TubingenGermany Department of Astronomy Beijing Normal UniversityBeijing 100088China Department of Astronomy Tsinghua UniversityBeijing 100084China Department of Physics Tsinghua UniversityBeijing 100084China Department of Engineering Physics Tsinghua UniversityBeijing 100084China Key Laboratory of Space Astronomy and Technology National Astronomical ObservatoriesChinese Academy of SciencesBeijing 100101China College of Physics Sciences&Technology Hebei UniversityBaoding 071002Hebei ProvinceChina

We present the observational results from a detailed timing analysis of the black hole candidate EXO 1846-031 during its outburst in 2019 with the observations of Insight-HXMT,NICER and *** outburst can be classified roughly into four different ***-C quasi-periodic oscillations(QPOs)observed by NICER(about 0.1-6 Hz)and Insight-HXMT(about 0.7-8 Hz)are also reported in this ***,we study various physical quantities related to QPO *** QPO rms-frequency relationship in the energy band 1-10 keV indicates that there is a turning pointing in frequency around2 Hz,which is similar to that of GRS 1915+105.A possible hypothesis for the relationship above may be related to the inclination of the source,which may require a high inclination to explain *** relationships between QPO frequency and QPO rms,hardness,total fractional rms and count rate have also been found in other transient sources,which can indicate that the origin of type-C QPOs is non-thermal.

关键词： X-ray binaries black hole candidate QPO EXO 1846–031

Consensus statement on layout and delivery of automatic external defibrillator in China

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Journal of Hainan Medical University 2020年第15期26卷 18-23页

作者： Yu Cao Song Chen yan-Fen Chai xiao-Hui Chen Yu-Guo Chen Shao-wen Cheng wen-Wei Cheng Bang-han Ding yang Deng Jie Fu Bang-jiang Fang Mai-ying Fan Li Gui Ping Gong Wei Guo Shu-bin Guo Liang Huang Ji-Yuan han Zhong Ji xian-Fei Ji Xin-cai Ji Hong-Xu Jin Xin-Jun jiang wang-xiang jiang Jia-Liang Liu xiao-Ran Liu Zhi Liu Chuan-Zhu Lv Feng Lu Tan-shi Li Xin Li yong Li Shang-Lun Li Shuang-ming Li xiao-Gang Li Bao-Jun Li Pei-Wu Li Chun-Sheng Li Zhi-Jun Li Chang-luo Li xiang-Min Li yin-Ping Li zong-Jun Lu Zu-Xun Lu Zhong-Qiu Lu Zhi-Qian luo xiao-Xing Liao Jian-Bo Lei Tao Ma Yu Ma Yue-Feng Ma qing-Bian Ma Lin-Hao Ma Jun-Qi Ma shi-Nan Nie Jie-Miao Ou-yang Peng Peng Qiao Pei Shu-ming Pan Guo-Zhong qing Li-Jie Qin Wu-ying Qiao Fei Shao Wei Song Xing-Yue Song Zhen-Ju Song rong-Ju Sun De-Ya Shang Du-Juan Sha Gui-Lan Tao Guo-Gang tian ying-Ping tian Jian-Guang tian Chao-yang Tong Zi-Ren Tang Meng-Xiong Tang Guo-Ping Wu Zhi Wan Tao wang Xin wang Peng wang Zhong wang Tong wang Ri-Xing wang Yi-Xin wang xiao-Dan wang Ling Wu Wei Wei Hua xiang Feng Xu Jun Xu Jie Xu Miao-rong Xie Shuo-Gui Xu Tie Xu Feng Yu wen Yi Li-Shan yang shi-Jiao yan Jin-Jian Yao Shou-Chun yan xue-Zhong Yu xian-Zhi Ye xian-Liang yan Fu-bing zhou rong-bin zhou ming zhou Qiang zhou Jin zhou Ping zhou Chang-Ju Zhu Hua-Dong Zhu Ji-Hong Zhu Hong zhang Mao zhang Hua zhang Na zhang Guo-Qiang zhang Guo-Xiu zhang Jin-Song zhang wen-Wu zhang wen-Zhong zhang Jian-Feng zhang Yi-Min Zhu Jun Zeng Yuan Zheng Zhi-Jie Zheng Shen zhao yan zhao Min zhao bin zhao xiao-Dong zhao xiao-Jing zhao Hong-Ke Zeng Sheng-Qiang Zou The Chinese Society of Emergency Medicine Research Unit of Island Emergency Medicine Chinese Academy of Medical SciencesHainan Medical University Key Laboratory of Emergency and Trauma of Ministry of Education Hainan Medical UniversityHaikouHainanChina Emergency and Trauma College Hainan Medical UniversityHaikouHainanChina Department of Emergency Hainan Clinical Research Center for Acute and Critical DiseasesThe Second Affiliated Hospital of Hainan Medical UniversityHaikouHainanChina Key Laboratory of Hainan Trauma and Disaster Rescue Key Laboratory of Trauma of Hainan Medical University

*** Sudden cardiac death(SCD)refers to sudden death due to a variety of cardiac *** is manifested as a sudden loss of consciousness,cardiac arrest,and respiratory arrest and generally shows early symptoms that are atypical and not easily detected[1].According to a recent study,nearly 544000 patients suffer from SCD every year in China[2].

关键词： cardiac death respiratory

四川省一起伴中毒性休克综合征的人感染猪链球菌2型暴发

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中华流行病学杂志 2006年第3期27卷 185-191页

作者：杨维中余宏杰景怀琦徐建国陈志海祝小平汪华刘学成王世文刘伦光祖荣强罗隆泽向妮娟刘红露钟文君刘莉孟玲袁珩高永军杜化茂欧阳宾叶长芸金冬吕强崔志刚黄燕张守印安向东黄婷周兴余冯燎庞启迪舒跃龙王宇中国疾病预防控制中心北京100050 中国疾病预防控制中心传染病预防控制所北京地坛医院四川省疾病预防控制中心江苏省疾病预防控制中心中国疾病预防控制中心中国现场流行病学培训项目中国疾病预防控制中心病毒病预防控制所

目的调查2005年7月中旬四川省资阳市一家医院报告5例以败血症休克为主要临床表现的聚集性病例的病因。方法建立了病例主动发现、报告的加强监测系统,根据病例的流行病学暴露史和临床表现进行临床诊断;采集患者标本进行细菌分离培养和生... 详细信息

目的调查2005年7月中旬四川省资阳市一家医院报告5例以败血症休克为主要临床表现的聚集性病例的病因。方法建立了病例主动发现、报告的加强监测系统,根据病例的流行病学暴露史和临床表现进行临床诊断;采集患者标本进行细菌分离培养和生化反应鉴定,应用PCR方法对猪链球菌2型的种属和毒力基因进行检测和序列测定;与当地往年报告的流行性脑脊髓膜炎发病数进行比较。结果2005年6月10日至8月21日,四川省共报告了68例实验室确诊人感染猪链球菌病例,发病前都有屠宰、洗切、加工等病(死)猪的直接暴露史。其中26例(38%)表现为中毒性休克综合征,15例(58%)死亡。其他病例临床表现为轻型败血症或脑膜炎。分离菌株应用PCR方法检测猪链球菌2型的种属和毒力基因(tuf、16S rRNA、cps2J、mrp、sly、ef)均为阳性。同期还报告了136例有相似暴露史,但缺乏实验室确诊依据的临床诊断病例。结论证实该起发生在四川省部分农村地区直接暴露于病(死)猪后的疾病为猪链球菌2型感染暴发。推测这种罕见的、表现为高病死率的中毒性休克综合征可能是由于感染某种高致病性菌株循环所致。

关键词：猪链球菌中毒性休克综合征

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论“植物医学”学科与专业的建设

植物医生 2021年第3期34卷 1-6页

作者：刘同先丁伟沈佐锐杨忠岐许永玉李洪连原雪峰马德英文才艺董金皋刘芳邱宝利王源超张正光黄丽丽黄国华操海群潘月敏韩强黄金光刘会香刘怀侯有明王宗华刘长仲缪卫国刘国坤郭永霞罗朝喜梁广文曾玲李华平顾爱星左豫虎李向东张大羽吴元华段玉玺尹建潘洪玉钟国华张跃进赵中华陈根强林晓民张友军万方浩高希武李世东褚栋赵洪海梁文星王森山张世泽李俊凯谭辉华王文明周洪友赵思峰王兰芦光新崔汝强李会平尚巧霞赵晓燕青岛农业大学植物医学学院山东青岛266109 西南大学植物保护学院重庆400715 中国农业大学植物保护学院北京100193 中国林业科学院北京100091 山东农业大学植物保护学院山东泰安271001 河南农业大学植物保护学院郑州450002 新疆农业大学农学院乌鲁木齐830052 河北农业大学植物保护学院河北保定071001 扬州大学园艺与植物保护学院江苏扬州225009 华南农业大学植物保护学院广州510642 南京农业大学植物保护学院南京210014 西北农林科技大学植物保护学院陕西杨凌712100 湖南农业大学植物保护学院长沙410128 安徽农业大学植物保护学院合肥230036 福建农林大学植物保护学院福州350002 甘肃农业大学植物保护学院兰州730070 海南大学植物保护学院海口570228 黑龙江八一农垦大学农学院黑龙江大庆163319 华中农业大学植物科技学院武汉430070 浙江农林大学农学院杭州311300 沈阳农业大学植物保护学院沈阳110161 信阳农林学院农学院河南信阳464006 吉林大学植物科技学院长春130012 全国农业技术推广服务中心北京100026 河南科技大学园艺与植保学院河南洛阳471023 中国农业科学院蔬菜花卉研究所北京100081 中国农业科学院植物保护研究所北京100193 长江大学农学院湖北荆州434020 广西大学农学院南宁530004 四川农业大学农学院四川雅安625014 内蒙古农业大学园艺与植保学院呼和浩特010018 石河子大学农学院新疆石河子832003 塔里木大学植物科学学院新疆阿拉尔843300 青海大学农牧学院西宁810016 江西农业大学农学院南昌330045 河北农业大学林学院河北保定071001 北京农学院生物与资源环境学院北京102206

1952年以前我国涉农高校设有植物病理学、昆虫学学科与专业,没有“植物保护”这一名称.在1952年全国高校院系调整时,因学习和借鉴原苏联的教育体系而引入并设立“植物保护”学科与专业.目前我国至少有62所高校设有“植物保护”学科和本... 详细信息

1952年以前我国涉农高校设有植物病理学、昆虫学学科与专业,没有“植物保护”这一名称.在1952年全国高校院系调整时,因学习和借鉴原苏联的教育体系而引入并设立“植物保护”学科与专业.目前我国至少有62所高校设有“植物保护”学科和本、专科专业.无论从专业名称、专业侧重或专业理念上看,“植物保护”都远远不能满足新农科背景下学科专业建设和高素质人才培养及“三农”发展的需求.在原植物保护学科的基础上,升级建设“植物医学”学科,与人医学、兽医学一起构建人类健康和食物安全的三大支柱和生态命运共同体是新时期赋予医学人员的使命.“植物医学”名称自明,理念新颖;基础植物医学探讨植物与害源的关系;实用植物医学倡导以植物健康为核心的“治未病”.本文通过分析我国高校植物保护学科与专业发展中存在的问题,呼吁在原“植物保护”学科与专业的基础上,建立“植物医学”一级学科与相关专业,逐步完善科学的高素质植物医学人才培养体系,建设新农科和深入贯彻落实习近平总书记给全国涉农高校书记校长和专家代表重要回信精神,以新农科建设为统领,推进高等农林教育创新发展,培养出更多学农、知农、爱农的新型人才.

关键词：植物医学植物保护学科发展新农科

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天琴计划简介

中山大学学报（自然科学版） 2021年第1期60卷 1-19页

作者：罗俊艾凌皓艾艳丽安子聪白伟钢白彦峥包佳慧曹斌常文博陈琛陈厚源崔凯单莹丁延卫段会宗范会敏范磊范纹彤范霄冯文凡付新菊付瑜亮高晨光郜青高添泉高鑫高永新龚云贵谷德峰辜凌云郭兴韩西达何芸胡一鸣胡越新胡展黄顺佳黄祥青黄潇博纪沐婕蒋贇焦磊靳鸿鸣康小明匡双阳雷卫华李程远李洪银李珏李康康李萌李明黎明李涛李霄栋李语强李祝李竹溪黎樽彪练军想梁正程林伟凌晨刘辉刘佳恒刘建平刘力刘祺刘尚飞刘胜前刘帅刘旭辉刘雁冲刘源龙江龙军陆璐罗成健骆颖欣马波梅健伟孟云鹤明珉牛翔潘加键庞爱平彭慧生屈少波区子维任亮亮申荣锋沈岩石常富宋佳凝宋培义索晓晨谭柏轩谭定银檀庄斌涂良成王成王铖锐王凤彬王海天王继河王凌风王尚胜王泰卜汪旭东王炎汪洋汪一萍王智钊魏东东文明轩吴庆文吴勤勤吴书朝吴先霖夏冰夏旭肖青肖小圆谢宁徐家豪颜浩闫勇杨铖杨诚鋆杨涓杨列杨山清叶伯兵叶贤基叶小容尹航于达仁袁慧敏曾明张才士张德轩张建东张静怡张锦绣张居正张开张蜡宝张立华张涛张鑫张鑫2 张雪峰赵宏超赵玥赵泽伟周鸿博周金灵周立祥周泽兵朱凡朱炬波訾铁光邹远川 “天琴计划”教育部重点实验室中山大学天琴中心天琴前沿科学中心国家航天局引力波研究中心广东珠海519082 中山大学物理与天文学院广东珠海519082 华中科技大学物理学院湖北武汉430074 航天东方红卫星有限公司北京100094 中国科学院云南天文台云南昆明650011 哈尔滨工业大学能源科学与工程学院黑龙江哈尔滨150001 北京控制工程研究所北京100094 东北大学理学院辽宁沈阳110004 贵州大学电气工程学院贵州贵阳550025 南京大学电子科学与工程学院江苏南京210093 上海交通大学机械与动力工程学院上海200240 深圳技术大学工程物理学院广东深圳518118 武汉大学电子信息学院湖北武汉430072 西北工业大学航空航天学院陕西西安710072 西南大学物理科学与技术学院重庆400715 中国科学院紫金山天文台江苏南京210023 中山大学航空航天学院广东广州510006 冲绳科学技术大学院大学日本冲绳951-8073

天琴计划预期于2035年左右发射并部署边长约17万公里的等边三角形卫星星座,构成一个引力波天文台—天琴。天琴将对10^(-4)~1 Hz频段的引力波进行探测,为人类描绘一幅更全面的宇宙图景。在本文中,我们对天琴计划的背景和提出过程、天琴... 详细信息

天琴计划预期于2035年左右发射并部署边长约17万公里的等边三角形卫星星座,构成一个引力波天文台—天琴。天琴将对10^(-4)~1 Hz频段的引力波进行探测,为人类描绘一幅更全面的宇宙图景。在本文中,我们对天琴计划的背景和提出过程、天琴的主要探测对象和主要科学目标、天琴需要攻克的核心关键技术问题、天琴计划技术路线图及进展等进行介绍,以方便更多人加入这一项富有挑战而又激动人心的工作。

关键词：天琴计划空间引力波探测引力波