国家重点基础研究发展计划(2013CBA01503)

作品数:24被引量:39H指数:4
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相关作者:林隽赵刚王菲鹿吴宁仲佳勇更多>>
相关机构:中国科学院大学中国科学院云南天文台中国科学院云南师范大学更多>>
相关期刊:《High Power Laser Science and Engineering》《北京师范大学学报(自然科学版)》《Earth and Planetary Physics》《Chinese Physics B》更多>>
相关主题:喷流太阳日冕物质抛射磁重联磁场更多>>
相关领域:天文地球电子电信理学政治法律更多>>
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磁中子星巨耀发的观测和理论研究
《天文学进展》2019年第3期240-264,共25页蒙盈 林隽 
国家自然科学基金(11333007);国家基金委员会-中国科学院联合基金(U1631130);中国科学院项目(XDA17040507,XDA15010900,QYZDJ-SSWSLH012);973项目(2013CBA01503);云南省创新团队基金(2018HC023);云南省“万人计划-云岭学者”专项
软γ重复暴(soft gamma-ray repeater, SGR)被认为产生于磁中子星。发生在SGR上的巨耀发在短时标内释放出大于10^39J的巨大能量,被认为是宇宙中已知最强的能量释放过程之一,其剧烈程度仅次于超新星爆发和γ暴。详细介绍了几种磁球层理...
关键词:磁流体动力学 磁重联 中子星 吸积盘 黑洞 
太阳爆发的抵近探测被引量:12
《中国科学:物理学、力学、天文学》2019年第5期70-89,共20页林隽 汪敏 田晖 宋红强 符慧山 黄旻 吕群波 张伟杰 张贤国 张坤毅 李明涛 张艺腾 金振宇 陈东 尹增山 邓雷 毛羽丰 李燕 梅志星 叶景 
中国科学院战略先导性专项课题(编号:XDA17040507;XDA15010900);中国科学院前沿科学重点研究项目(编号:QYZDJ-SSWSLH012);国家重点基础研究发展计划(编号:2013CBA01503);国家基金重点项目(编号:11333007);国家基金委员会-中国科学院联合基金项目(编号:U1631130);云南省创新团队项目资助
本工作将介绍一项具有重大科学和实际意义的深空探测任务,这项任务的顺利实施将允许我们在一个前所未有的近距离上以遥感和实地探测手段相结合的方式观测和研究一颗恒星的磁活动以及磁重联区域.首先,我们将首次直接进入太阳风暴的核心...
关键词:磁重联 日冕 日冕物质抛射 
Electron acceleration in interaction of magnetic islands in large temporal-spatial turbulent magnetic reconnection被引量:1
《Earth and Planetary Physics》2019年第1期17-25,共9页BoJing Zhu Hui Yan David A Yuen YaoLin Shi 
supported by the strategic priority research program of CAS (XDA17040507, XDA15010900);the national basic research program of China (2013CBA01503);the key program of NSFC (11333007);joint funds of NSFC(U1631130);frontier science key programs of CAS (QYZDJ-SSWSLH012);the program for innovation team of Yunnan Province;the program for Guangdong introducing Innovative and entrepreneurial teams (2016ZT06D211);the special program for applied research on super computation of the NSFC-Guangdong joint fund (second phase) under No.U1501501
A new combined Fermi, betatron, and turbulent electron acceleration mechanism is proposed in interaction of magnetic islands during turbulent magnetic reconnection evolution in explosive astrophysical phenomena at lar...
关键词:hybrid PARTICLE ACCELERATION mechanism LARGE temporal-spatial TURBULENT magnetic RECONNECTION Hydro-Dynamic-Kinetic model 
Manifestations of bright points observed in G-band and CaⅡH by Hinode/SOT
《Research in Astronomy and Astrophysics》2018年第10期85-96,共12页Yan-Xiao Liu Ning Wu Jun Lin 
supported by the CAS grants(XDA17010507,XDA15010900 and QYZDJ-SSWSLH012);the NationalBasic Research Program of China(973 Program,2013CBA01503);the National Natural Science Foundation of China(Grant Nos.U1631130,11333007 and 11763004);supported by a grant associated with the Project of the Group for Innovation of Yunnan Province
An algorithm was developed for identifying and tracking a magnetic bright point, or bright point (BP) for short, observed in both the photosphere (G-band) and chromosphere (Ca II H), as well as for pairing a pho...
关键词:SUN photosphere - Sun chromosphere - methods observational - techniques image processing 
Magnetic reconnection driven by intense lasers被引量:1
《High Power Laser Science and Engineering》2018年第3期85-101,共17页Jiayong Zhong Xiaoxia Yuan Bo Han Wei Sun Yongli Ping 
supported by the Science Challenge Project(No.TZ2016005);the National Basic Research Program of China(No.2013CBA01503);the National Natural Science Foundation of China(Nos.10905004,11220101002,and11622323);the Fundamental Research Funds for the Central Universities
Laser-driven magnetic reconnection(LDMR) occurring with self-generated B fields has been experimentally and theoretically studied extensively, where strong B fields of more than megagauss are spontaneously generated i...
关键词:high energy density physics laser plasmas interaction plasmas astrophysics 
Measurement and analysis of K-shell lines of silicon ions in laser plasmas被引量:1
《High Power Laser Science and Engineering》2018年第2期133-140,共8页Bo Han Feilu Wang Jiayong Zhong Guiyun Liang Huigang Wei Dawei Yuan Baojun Zhu Fang Li Chang Liu Yanfei Li Jiarui Zhao Zhe Zhang Chen Wang Jun Xiong Guo Jia Neng Hua Jianqiang Zhu Yutong Li Gang Zhao Jie Zhang 
supported by the Science Challenge Project(No.TZ2016005);the National Basic Research Program of China(No.2013CBA01503);the National Natural Science Foundation of China(Nos.10905004,11220101002,and11622323);the Fundamental Research Funds for the Central Universities
We present laboratory measurement and theoretical analysis of silicon K-shell lines in plasmas produced by Shenguang II laser facility, and discuss the application of line ratios to diagnose the electron density and t...
关键词:high energy density physics laser plasmas interaction plasmas astrophysics 
Numerical studies of the Kelvin-Hemholtz instability in a coronal jet
《Research in Astronomy and Astrophysics》2018年第4期91-104,共14页Tian-Le Zhao Lei Ni Jun Lin Udo Ziegler 
supported by the National Natural Science Foundation of China (Grant Nos. 11573064, 11203069, 11333007, 11303101 and 11403100);the National Basic Research Program of China (973 program, 2013CBA01503);the NSFCCAS Joint Fund (U1631130); the CAS grant QYZDJSSW-SLH012;the Western Light of Chinese Academy of Sciences 2014;the Youth Innovation Promotion Association, CAS 2017;the Key Laboratory of Solar Activity (Grant KLSA201404);the NSFC-Guangdong Joint Fund (U1501501, nsfc2015460 and nsfc2015-463)
Kelvin-Hemholtz(K-H)instability in a coronal EUV jet is studied via 2.5D MHD numerical simulations.The jet results from magnetic reconnection due to the interaction of the newly emerging magnetic field and the pre-e...
关键词:Sun corona jet  Kelvin-Hemholtz instability  guide-field  method numerical simulations 
A small electron beam ion trap/source facility for electron/neutral-ion collisional spectroscopy in astrophysical plasmas
《Research in Astronomy and Astrophysics》2018年第1期1-10,共10页Gui-Yun Liang Hui-Gang Wei Da-Wei Yuan Fei-Lu Wang Ji-Min Peng Jia-Yong Zhong Xiao-Long Zhu Mike Schmidt Günter Zschornack Xin-Wen Ma Gang Zhao 
supported by the National Key R&D Program of China(No.2017YFA0402401);the National Natural Science Foundation of China(Grant No.11522326);the National Basic Research Program of China(973 Program,Grant 2013CBA01503);support by the Science Challenge Project(No.TZ2016005)
Spectra are fundamental observation data used for astronomical research,but understanding them strongly depends on theoretical models with many fundamental parameters from theoretical calculations.Different models giv...
关键词:X-ray:general atomic processes line:formation method:laboratory:atomic 
基于太阳爆发灾变模型的数值实验被引量:3
《天文学报》2017年第6期37-56,共20页谢小妍 ZIEGLER Udo 梅志星 吴宁 林隽 
国家自然科学基金项目(11333007,U1631130);973项目(2013CBA01503);中国科学院前沿重点研究项目(QYZDJ-SSW-SLH012);NSFC-广东联合基金(第二期)超级计算科学应用研究专项(U1501501)资助
在Isenberg等人发展的灾变模型基础上根据接近真实的日冕环境,通过数值实验,对磁通量绳的平衡高度对光球磁场变化的响应开展了研究.利用NIRVANA程序进行了计算.日冕的等离子密度分布采用了一个半经验的模型,模拟中包含了物理耗散.考察了...
关键词:太阳 日冕物质抛射 太阳 磁场 磁流体动力学 方法 数值 
Measurement of iron characteristics under ramp compression
《Chinese Physics B》2017年第11期360-364,共5页魏会冈 E Brambrink N Amadou A Benuzzi-Mounaix A Ravasio G Morard F Guyot T de Rességuier N Ozaki K Miyanishi 赵刚 M Koenig 
Project supported by the National Basic Research Program of China(Grant No.2013CBA01503);the National Natural Science Foundation of China(Grant No.11103040)
Laser-driven ramp compression was used to investigate iron characteristics along the isentropic path. The iterative Lagrangian analysis method was employed to analyze the free surface velocity profiles in iron stepped...
关键词:isentropic compression iron phase transformation 
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