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Land use and land cover change and its driving forces in Maqu County, China in the past 25 years

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Research in Cold and Arid Regions 2016年第5期8卷 432-440页

作者： junfeng lu zhibao dong guangyin hu WenJin Li WanYin luo MingLiang Tan Key Laboratory of Desert and Desertification Northwest Institute of Eco-Environment and Resources Chinese Academy of Sciences State Key Laboratory of Grassland Agroecosystems School of Life Sciences Lanzhou University

Maqu County is located in the northeast Qinghai-Tibetan Plateau, and it is the main watershed for the Yellow River. The ecosystem there is extremely vulnerable and sensitive to climate change and human activities, which have caused significant deterioration of the eco-environment in this region. In order to restore the ecological environment, a government project to restore the grazing areas to grassland was implemented in Maqu County in early 2004. This study evaluates the effects of that restoration project on land use and land cover change （luCC）, and explores the driving forces of luCC in Maqu County. In the study we used Landsat images obtained in 1989, 2004, 2009, and 2014 to establish databases of land use and land cover. Then we derived luCC information by overlaying these layers using GIS software. Finally, we analyzed the main forces responsible for luCC. The results showed that forests, high-coverage grasslands, and marshes experienced the most significant decreases during 1989–2004, by 882.8 ha, 35,250.4 ha, and 2,753.4 ha, respectively. However, moderate- and low-coverage grasslands and sand lands showed the opposite trend, increasing by 12,529.7 ha, 25,491.0 ha, and 577.5 ha, respectively. luCC in 2004–2009 showed that ecological degradation slowed compared with 1989？2004. During 2009–2014, high- and moderate-coverage grasslands increased obviously, but low-coverage grasslands, marshes, unused lands, sand lands, and water areas showed the opposite trend. These results suggested that the degradation of the eco-environment was obvious before 2009, showing a decrease in the forests, grasslands, and water areas, and an increase in unused lands. The ecological degradation was reversed after 2009, as was mainly evidenced by increases in high- and mod-erate-coverage grasslands, and the shrinkage rate of marshes decreased obviously. These results showed that the project of restoring grazing lands to grassland had a positive effect on the luCC. Other major fac

关键词： luCC driving forces Maqu County source region of the Yellow River

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黄河源区沙漠化及其景观格局的变化

生态学报 2011年第14期31卷 3872-3881页

作者：胡光印董治宝逯军峰颜长珍中国科学院寒区旱区环境与工程研究所沙漠与沙漠化重点实验室甘肃兰州730000

以1975年的MSS数据、1990年和2005年的TM数据、以及2000年的ETM数据为数据源,通过遥感(RS)与地理信息系统(GIS)技术,获得了黄河源区在1975—2005年间的沙漠化发展特征,并采用景观指数运算软件(FRAGSTATS3.3)对黄河源区沙漠化土地的景观... 详细信息

以1975年的MSS数据、1990年和2005年的TM数据、以及2000年的ETM数据为数据源,通过遥感(RS)与地理信息系统(GIS)技术,获得了黄河源区在1975—2005年间的沙漠化发展特征,并采用景观指数运算软件(FRAGSTATS3.3)对黄河源区沙漠化土地的景观格局变化进行了分析。研究发现:在1975—1990年间,黄河源区的沙漠化土地面积大幅增加;在1990—2000年间,沙漠化土地面积保持稳定;在2000—2005年间,沙漠化土地面积出现了小幅度的减小趋势。黄河源区沙漠化土地的景观格局变化显著,在1975—1990年间,沙漠化土地发生了严重的破碎化;在1990—2000年间,沙漠化土地出现了连片的现象,从而使得沙漠化土地的破碎度有所下降,景观多样性降低;在2000—2005年间,沙漠化土地破碎度增加,斑块形状趋于复杂。

关键词：黄河源沙漠化景观格局青藏高原

黄河源区土地利用/覆盖变化(luCC)研究

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冰川冻土 2014年第3期36卷 573-581页

作者：胡光印金会军董治宝颜长珍逯军峰中国科学院寒区旱区环境与工程研究所沙漠与沙漠化重点实验室甘肃兰州730000 中国科学院寒区旱区环境与工程研究所冻土工程国家重点实验室甘肃兰州730000

利用遥感(RS)监测手段和地理信息系统(GIS)技术,获取了黄河源区在1975、1990、和2005年3个时期的土地利用/覆盖数据,并通过叠加分析,获得了该地区土地利用/覆盖的时空转移特征.此外,通过县级行政区对源区各县域内的土地利用/覆盖变化特... 详细信息

利用遥感(RS)监测手段和地理信息系统(GIS)技术,获取了黄河源区在1975、1990、和2005年3个时期的土地利用/覆盖数据,并通过叠加分析,获得了该地区土地利用/覆盖的时空转移特征.此外,通过县级行政区对源区各县域内的土地利用/覆盖变化特征进行了统计分析,以期为该地区的环境管理提供科学依据.结果表明:在1975-2005年间,黄河源区的环境退化非常明显,土地利用/覆盖变化主要表现为耕地、沙地、滩地和水库、坑塘面积增加;沼泽地面积减小;高覆盖度草地面积减小,中、低覆盖度草地面积增加.从县级行政区划上来看,耕地的增加主要分布于贵南、同德和泽库三个县;林地面积在玛沁和甘德两县有大面积的减小趋势;新增的沙地主要分布在玛多、共和、曲麻莱和若尔盖县;新增水库、坑塘则主要分布于共和、和贵南两县;沼泽地面积的减少绝大部分发生在若尔盖县;高覆盖度草地在甘德和玛沁两县增加非常明显,但在玛曲、玛多、达日、兴海、阿坝、若尔盖、红原等县均有大面积的减小趋势.因此,在黄河源区开展环境保护或环境治理工作,应根据不同区域的具体环境问题采取相应的治理措施.

关键词：黄河源区土地利用覆盖变化青藏高原

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黄河流域沙漠化空间格局与成因

中国沙漠 2021年第4期41卷 213-224页

作者：胡光印董治宝逯军峰杨林海南维鸽肖锋军陕西师范大学地理科学与旅游学院陕西西安710119 中国科学院西北生态环境资源研究院中国科学院沙漠与沙漠化重点实验室甘肃兰州730000

黄河流域地势西高东低,自西向东有青藏高原、内蒙古高原、黄土高原和黄淮海平原4个地貌单元,总面积为79.6万km^(2)。黄河流域是中国重要的生态屏障和重要经济带,黄河流域生态保护和高质量发展已上升为国家战略。沙漠化是中国北方干旱、... 详细信息

黄河流域地势西高东低,自西向东有青藏高原、内蒙古高原、黄土高原和黄淮海平原4个地貌单元,总面积为79.6万km^(2)。黄河流域是中国重要的生态屏障和重要经济带,黄河流域生态保护和高质量发展已上升为国家战略。沙漠化是中国北方干旱、半干旱以及部分半湿润地区主要的土地退化形式,沙漠化对黄河流域,尤其是流域中、上游地区的影响较大。为了全面掌握黄河流域的沙漠化土地空间分布特征,本研究以Landsat遥感影像为数据源,通过地理信息系统(GIS)技术,获得了黄河流域2010年的沙漠化土地分布数据。结果表明:黄河流域内沙漠化土地面积为128667 km^(2),占流域总面积的16.2%;黄河上游的沙漠化土地面积最大,然后依次是黄河中游、黄河源区、黄河下游,沙漠化土地面积分别为89341、21426、17894、7 km^(2),分别占全流域沙漠化土地总面积的69.4%、16.7%、13.9%、0.01%。黄河流域的沙漠化土地绝大部分分布于内蒙古,其沙漠化土地面积为91398 km^(2),占全流域沙漠化土地面积的71.0%;其次是青海,沙漠化土地面积为17432 km^(2),占全流域沙漠化土地面积的13.5%;陕西和宁夏的沙漠化土地面积分别占全流域沙漠化土地面积的8.3%和6.5%。黄河流域的沙漠化空间格局主要是降水量与沙源空间耦合的结果,流域92.6%(119114 km^(2))的沙漠化土地分布于干旱、半干旱地区。从20世纪70年代以来,黄河流域的沙漠化总体上经历了快速发展—发展放缓—明显逆转的过程,沙漠化大幅度的变化主要受人类活动影响所致,在过去几十年间风速持续减小对沙漠化逆转的积极作用也应引起重视。

关键词：沙漠化分布格局黄河黄河流域

Einstein Probe discovery of EP240408a:A peculiar X-ray transient with an intermediate timescale

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Science China(Physics,Mechanics & Astronomy) 2024年

作者： Wenda Zhang Weimin Yuan Zhixing Ling Yong Chen Nanda Rea Arne Rau Zhiming Cai huaqing Cheng Francesco Coti Zelati Lixin Dai Jingwei hu Shumei Jia Chichuan Jin dongyue Li Paul O’Brien Rongfeng Shen Xinwen Shu Shengli Sun Xiaojin Sun Xiaofeng Wang Lei yang Bing Zhang Chen Zhang Shuang-Nan Zhang Yonghe Zhang Jie An David Buckley Alexis Coleiro Bertrand Cordier Liming Dou Rob Eyles-Ferris Zhou Fan hua Feng Shaoyu Fu Johan P. U. Fynbo Lluis Galbany Saurabh W. Jha Shuaiqing Jiang Albert Kong Erik Kuulkers Weihua Lei Wenxiong Li Bifang Liu Mingjun Liu Xing Liu Yuan Liu Zhu Liu Chandreyee Maitra Alessio Marino Itumeleng Monageng Kirpal Nandra Jeremy Sanders Roberto Soria Lian Tao junfeng Wang Song Wang Tinggui Wang Zhongxiang Wang Qingwen Wu Xuefeng Wu dong Xu yanjun Xu Suijian Xue Yongquan Xue Zijian Zhang Zipei Zhu hu Zou Congying Bao Fansheng Chen Houlei Chen Tianxiang Chen Wei Chen Yehai Chen Yifan Chen Chenzhou Cui Weiwei Cui yanfeng Dai dongwei Fan Ju Guan Dawei Han dongjie Hou Haibo hu Maohai huang Jia huo Zhenqing Jia Bowen Jiang Ge Jin Chengkui Li Junfei Li Longhui Li Maoshun Li Wei Li Zhengda Li Tianying Lian Congzhan Liu Heyang Liu huaqiu Liu Fangjun lu Laidan luo Jia Ma Xuan Mao Haiwu Pan Xin Pan Liming Song hui Sun Yunyin Tan Qingjun Tang Yihan Tao Hao Wang Juan Wang Lei Wang Wenxin Wang Yilong Wang Yusa Wang Qinyu Wu Haitao Xu Jingjing Xu Xinpeng Xu Yunfei Xu Zhao Xu Changbin Xue Yulong Xue Ailiang yan Haonan yang Xiongtao yang yanji yang Juan Zhang Mo Zhang Wenjie Zhang Zhen Zhang Zhen Zhang Ziliang Zhang donghua Zhao Haisheng Zhao Xiaofan Zhao Zijian Zhao Hongyan Zhou Yilin Zhou Yuxuan Zhu Zhencai Zhu Institut d’Estudis Espacials de Catalunya (IEEC) Max Planck Institute for Extraterrestrial Physics Innovation Academy for Microsatellites Chinese Academy of Sciences Department of Physics University of Hong Kong School of Physics and Astronomy University of Leicester School of Physics and Astronomy Sun Yat-sen University National Astronomical Observatories Department of Physics Anhui Normal University Shanghai Institute of Technical Physics Chinese Academy of Sciences Physics Department Tsinghua University Nevada Center for Astrophysics University of Nevada Las Vegas Department of Physics and Astronomy University of Nevada Las Vegas Chinese Academy of Sciences South African Astronomical Observatory Department of Astronomy University of Cape Town Department of Physics University of the Free State Universite' Paris Cite' CNRS Astroparticule et Cosmologie Universite' Paris Cite' CEA Paris-Saclay School of Astronomy and Space Sciences IRFU/DAp-AIM Department of Astronomy Guangzhou University Cosmic Dawn Center (DAWN) Niels Bohr Institute University of Copenhagen Department of Physics and Astronomy Rutgers the State University of New Jersey Institute for Cosmic Ray Research University of Chinese Academy of Sciences The University of Tokyo ESA/ESTEC Noordwijk 2201 AZ The Netherlands Department of Astronomy School of Physics huazhong University of Science and Technology INAF-Osservatorio Astrofisico di Torino Sydney Institute for Astronomy School of Physics Key Laboratory of Particle Astrophysics The University of Sydney Department of Astronomy Xiamen University Institute for Frontiers in Astronomy and Astrophysics Beijing Normal University Department of Astronomy University of Science and Technology Hefei School of Astronomy and Space Sciences University of Science and Technology of China Institute of High Energy Physics Institute of Deep Space Sciences Deep Space Exploration Laboratory Department of Astronomy School of Physics and Astronomy Yunnan University Shanghai Astronomical Observatory Chinese Academy of Science

We report the discovery of a peculiar X-ray transient,EP240408a,by Einstein Probe （EP） and follow-up studies made with EP,Swift,NICER,GROND,ATCA and other ground-based multiwavelength *** new transient was first detected with Wide-field X-ray Telescope （WXT） on board EP on April 8th,2024,manifested in an intense yet brief X-ray flare lasting for *** flare reached a peak flux of 3.9×10-9erg cm-2s-1in 0.5-4 keV,300 times brighter than the underlying X-ray emission detected throughout the *** and more precise follow-up observations by EP/FXT,Swift and NICER confirmed the finding of this new *** X-ray spectrum is non-thermal in 0.5-10 keV,with a power-law photon index varying *** X-ray light curve shows a plateau lasting for4d,followed by a steep decay till becoming undetectable10 d after the initial *** on its temporal property and constraints from previous EP observations,an unusual timescale in the range of 7-23 d is found for EP240408a,which is intermediate between the commonly found fast and long-term *** counterparts have been found in optical and near-infrared,with the earliest observation at 17 h after the initial X-ray detection,suggestive of intrinsically weak emission in these *** demonstrate that the remarkable properties of EP240408a are inconsistent with any of the transient types known so far,by comparison with,in particular,jetted tidal disruption events,gamma-ray bursts,X-ray binaries and fast blue optical *** nature of EP240408a thus remains an *** suggest that EP240408a may represent a new type of transients with intermediate timescales of the order of10 *** detection and follow-ups of more of such objects are essential for revealing their origin.

关键词：

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

基于3S的豫北内黄县近30年来植被覆被变化研究

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地域研究与开发 2010年第4期29卷 127-130,144页

作者：李根明董治宝孙虎钱广强罗万银王洪涛逯军峰中国科学院寒区旱区环境与工程研究所沙漠与沙漠化重点实验室兰州730000 陕西师范大学旅游与环境学院西安710006

运用3S技术,分析和探讨了河南省内黄县1979—2007年的植被覆盖度变化特征。结果显示,该区30年间的植被覆盖度变化显著。具体为：高覆盖度和中高覆盖度逐年上升,而中覆盖度、低覆盖度和极低覆盖度出现不同程度的降低,中覆盖度降低的幅度... 详细信息

运用3S技术,分析和探讨了河南省内黄县1979—2007年的植被覆盖度变化特征。结果显示,该区30年间的植被覆盖度变化显著。具体为：高覆盖度和中高覆盖度逐年上升,而中覆盖度、低覆盖度和极低覆盖度出现不同程度的降低,中覆盖度降低的幅度较小,而低级覆盖度下降幅度较大。结论表明研究区的生态环境质量呈现不断上升的态势。一方面反映了人口增长和经济建设需求对植被覆被变化的积极影响,另一方面反映相关部门重视生态环境的建设,研究区人口素质提高环保意识增强。

关键词：植被覆盖度 3S 生态环境质量内黄县

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激光聚变内爆流体不稳定性基础问题研究进展

强激光与粒子束 2021年第1期33卷 1-60页

作者：王立锋叶文华陈竹李永升丁永坤赵凯歌张靖李志远杨云鹏吴俊峰范征锋薛创李纪伟王帅杭旭登缪文勇袁永腾涂绍勇尹传盛曹柱荣邓博杨家敏江少恩董佳钦方智恒贾果谢志勇黄秀光傅思祖郭宏宇李英骏程涛高振方丽丽王保山王英华曾维新卢艳旷圆圆赵振朝陈伟戴振生谷建法葛峰峻康洞国张桦森乔秀梅李蒙刘长礼申昊许琰高耀明刘元元胡晓燕徐小文郑无敌邹士阳王敏朱少平张维岩贺贤土北京应用物理与计算数学研究所北京100094 北京大学应用物理与技术研究中心高能量密度物理数值模拟教育部重点实验室工学院北京100871 中国工程物理研究院激光聚变研究中心四川绵阳621900 中国工程物理研究院上海激光等离子体研究所上海201800 中国矿业大学(北京) 北京100083 中国海洋大学数学科学学院山东青岛266100 安徽大学物理与材料科学学院合肥230039

激光聚变有望一劳永逸地解决人类的能源问题,因而受到国际社会的普遍重视,一直是国际研究的前沿热点。目前实现激光惯性约束聚变所面临的最大科学障碍(属于内禀困难)是对内爆过程中高能量密度流体力学不稳定性引起的非线性流动的有效控... 详细信息

激光聚变有望一劳永逸地解决人类的能源问题,因而受到国际社会的普遍重视,一直是国际研究的前沿热点。目前实现激光惯性约束聚变所面临的最大科学障碍(属于内禀困难)是对内爆过程中高能量密度流体力学不稳定性引起的非线性流动的有效控制,对其研究涵盖高能量密度物理、等离子体物理、流体力学、计算科学、强冲击物理和高压原子物理等多个学科,同时还要具备大规模多物理多尺度多介质流动的数值模拟能力和高功率大型激光装置等研究条件。作为新兴研究课题,高能量密度非线性流动问题充满了各种新奇的现象亟待探索。此外,流体力学不稳定性及其引起的湍流混合,还是天体物理现象(如星系碰撞与合并、恒星演化、原始恒星的形成以及超新星爆炸)中的重要过程,涉及天体物理的一些核心研究内容。本文首先综述了高能量密度非线性流动研究的现状和进展,梳理了其中的挑战和机遇。然后介绍了传统中心点火激光聚变内爆过程发生的主要流体力学不稳定性,在大量分解和综合物理研究基础上,凝练出了目前制约美国国家点火装置(NIF)内爆性能的主要流体不稳定性问题。接下来,总结了国外激光聚变流体不稳定性实验物理的研究概况。最后,展示了内爆物理团队近些年在激光聚变内爆流体不稳定性基础性问题方面的主要研究进展。该团队一直从事激光聚变内爆非线性流动研究与控制,以及聚变靶物理研究与设计,注重理论探索和实验研究相结合,近年来在内爆重要流体力学不稳定性问题的解析理论、数值模拟和激光装置实验设计与数据分析等方面取得了一系列重要成果,有力地推动了该研究方向在国内的发展。

关键词：激光聚变惯性约束聚变流体力学不稳定性高能量密度物理非线性流动辐射流体力学内爆物理