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| 1 | Advanced Space-based Solar Observatory(ASO-S):an overview显示文摘The Advanced Space-based Solar Observatory(ASO-S)is a mission proposed for the 25 th solar maximum by the Chinese solar community.The scientific objectives are to study the relationships between the solar magnetic field,solar flares and coronal mass ejections(CMEs).Three payloads are deployed:the Full-disk vector Magneto Graph(FMG),the Lyman-αSolar Telescope(LST)and the Hard X-ray Imager(HXI).ASO-S will perform the first simultaneous observations of the photospheric vector magnetic field,non-thermal imaging of solar flares,and the initiation and early propagation of CMEs on a single platform.ASO-S is scheduled to be launched into a 720 km Sun-synchronous orbit in 2022.This paper presents an overview of the mission till the end of Phase-B and the beginning of Phase-C. | Wei-Qun Gan Cheng Zhu Yuan-Yong Deng Hui Li Yang Su Hai-Ying Zhang Bo Chen Zhe Zhang Jian Wu Lei Deng Yu Huang Jian-Feng Yang Ji-Jun Cui Jin Chang Chi Wang Ji Wu Zeng-Shan Yin Wen Chen Cheng Fang Yi-Hua Yan Jun Lin Wei-Ming Xiong Bin Chen Hai-Chao Bao Cai-Xia Cao Yan-Ping Bai Tao Wang Bing-Long Chen Xin-Yu Li Ye Zhang Li Feng Jiang-Tao Su Ying Li Wei Chen You-Ping Li Ying-Na Su Hai-Yan Wu Mei Gu Lei Huang Xue-Jun Tang | 2019 | Research in Astronomy and Astrophysics2019，19，11： | 17 |
| 2 | Hard X-ray Imager (HXI) onboard the ASO-S mission显示文摘Hard X-ray Imager(HXI)is one of the three scientific instruments onboard the Advanced Spacebased Solar Observatory(ASO-S)mission,which is proposed for the 25th solar maximum by the Chinese solar community.HXI is designed to investigate the non-thermal high-energy electrons accelerated in solar flares by providing images of solar flaring regions in the energy range from 30 keV to 200 keV.The imaging principle of HXI is based on spatially modulated Fourier synthesis and utilizes about 91 sets of bi-grid sub-collimators and corresponding LaBr3 detectors to obtain Fourier components with a spatial resolution of about 3 arcsec and a time resolution better than 0.5 s.An engineering prototype has been developed and tested to verify the feasibility of design.In this paper,we present background,instrument design and the development and test status of the prototype. | Zhe Zhang Deng-Yi Chen Jian Wu Jin Chang Yi-Ming Hu Yang Su Yan Zhang Jian-Ping Wang Yao-Ming Liang Tao Ma Jian-Hua Guo Ming-Sheng Cai Yong-Qiang Zhang Yong-Yi Huang Xiao-Yan Peng Zong-Bin Tang Xuan Zhao Hong-He Zhou Lian-Guo Wang Jing-Xing Song Miao Ma Guang-Zhou Xu Jian-Feng Yang Di Lu Ying-Hong He Jin-You Tao Xiao-Long Ma Bao-Gang Lv Yan-Ping Bai Cai-Xia Cao Yu Huang Wei-Qun Gan | 2019 | Research in Astronomy and Astrophysics2019，19，11： | 9 |
| 3 | Impact of potentially lethal ventricular arrhythmias on long-term outcome in patients with chronic heart failure显示文摘背景潜在地致命的室的心律不齐( PLVA )在尖锐心肌的梗塞以后在幸存者经常发生并且逐渐地在调查的结构的心 diseases.This 学习的另外的形式被认出流行和在有长期的心失败( CHF )的病人的 PLVA 的预示的意义有关人口分布的 .Methods 数据,心失败的病原学, NYHA 功能的班,生物化学的变量, electrocardiographic 和 echocardiographic 调查结果,和医疗是 c 23.4 在病人 45 岁, 27.8 在那些在 45-65 岁之间,并且 33.5 没有 PLVAs.Age ,在病人,有 PLVA 的 65 岁( P=0.033 ) .Patients 比那些在5年的后续期间有更大的 LV 尺寸和更低的喷射部分(两 P 0.01 )和更高的所有原因死亡( P=0.014 )(或 1.041,95 Cl 1.004-1.079 , P=0.03 )并且 LV 结束心脏舒张的尺寸(或 1.068,95 Cl 1.013-1.126 , P=0.015 )独立地预言 PLVAs.And PLVA 的出现是为所有原因死亡的一个独立因素( RR 1.702。 | Liu Ye-hong Su Jing-ying Wang Lin-jie Li Jin-ping Zhou Qing-fen Gan Qian Chai Xi-chen Dai Li-ying Zhang Feng-ru Shen Wei-feng | 2012 | Chinese Medical Journal2012，，4： | 8 |
| 4 | Simulations and software development for the Hard X-ray Imager onboard ASO-S显示文摘China’s first solar mission,the Advanced Space-based Solar Observatory(ASO-S),is now changing from Phase B to Phase C.Its main scientific objectives are summarized as’1M2B’,namely magnetic field and two types of bursts(solar flares and coronal mass ejections).Among the three scientific payloads,Hard X-ray Imager(HXI)observes images and spectra of X-ray bursts in solar flares.In this paper,we briefly report on the progresses made by the HXI science team(data and software team)during the design phase(till May 2019).These include simulations of HXI imaging,optimization of HXI grids,development of imaging algorithms,estimation of orbital background,as well as in-orbit calibration plan.These efforts provided guidance for the engineering,improved HXI’s imaging capability and reduced the cost of the instrument. | Yang Su Wei Liu You-Ping Li Zhe Zhang Gordon JHurford Wei Chen Yu Huang Zhen-Tong Li Xian-Kai Jiang Hao-Xiang Wang Fan-Xiao-Yu Xia Chang-Xue Chen Wen-Hui Yu Fu Yu Jian Wu Wei-Qun Gan | 2019 | Research in Astronomy and Astrophysics2019，19，11： | 7 |
| 5 | Preface:Advanced Space-based Solar Observatory(ASO-S)显示文摘The Advanced Space-based Solar Observatory(ASO-S)is the first approved solar space mission in China.This special issue includes a total of 13 papers,which were selected from presentations at the First ASO-S International Workshop,held in Nanjing from 2019 January 15 to 18.Taken together,these 13 papers provide a complete description of ASO-S until the end of Phase-B and the beginning of Phase-C. | Wei-Qun Gan Ming-De Ding Yu Huang Ying-Na Su | 2019 | Research in Astronomy and Astrophysics2019，19，11： | 7 |
| 6 | A Comparison Study of Working Memory Deficits between Patients with Methamphetamine-Associated Psychosis and Patients with Schizophrenia显示文摘 | Hong GAN Zhenhua SONG Peiwei XU Hang SU Yingying PAN Min ZHAO Dengtang LIU | 2018 | 上海精神医学2018，30，3： | 6 |
| 7 | Data reduction and calibration of the FMG onboard ASO-S显示文摘The Full-disk vector Magneto Graph(FMG)instrument will carry out polarization observations at one wavelength position of the Fe I 5324.179?spectral line.This paper describes how to choose this single wavelength position,the relevant data-processing and the magnetic field calibrations based on the measured polarization signals at one single wavelength position.It is found that solar radial Doppler velocity,which can cause the spectral line to shift,is a disadvantageous factor for the linear calibration at one wavelength position.Observations at two symmetric wavelength positions may significantly reduce the wavelength shift effect(~75%),but simulations show that such polarization signals located at the solar limbs(e.g.,beyond the longitude range of±30°)are not free from the effect completely.In future work,we plan to apply machine learning techniques to calibrate vector magnetic fields,or employ full Stokes parameter profile inversion techniques to obtain accurate vector magnetic fields,in order to complement the linear calibration at the single wavelength position. | Jiang-Tao Su Xian-Yong Bai Jie Chen Jing-Jing Guo Suo Liu Xiao-Fan Wang Hai-Qing Xu Xiao Yang Yong-Liang Song Yuan-Yong Deng Kai-Fan Ji Lei Deng Yu Huang Hui Li Wei-Qun Gan | 2019 | Research in Astronomy and Astrophysics2019，19，11： | 6 |
| 8 | Measurement of γ detector backgrounds in the energy range of 3-8 MeV at Jinping underground laboratory for nuclear astrophysics显示文摘The astrophysical reaction rate of the charged-particleinduced reaction is dominated by the cross section within the Gamow window.The total cross section σ(E)of a chargedparticle-induced reaction is known to drops steeply with decreasing energy owing to the Coulomb barrier in the entrance channel: | YangPing Shen Jun Su WeiPing Liu Gang Lian Lin Gan LvHua Qiao ShengQuan Yan Yong Zhou Qian Yue Zhi Zeng QingDong Hu YuHao Mi Wei Zhao | 2017 | Science China(Physics,Mechanics & Astronomy)2017，60，10： | 5 |
| 9 | The FAST Galactic Plane Pulsar Snapshot survey:I.Project design and pulsar discoveries显示文摘Discovery of pulsars is one of the main goals for large radio telescopes.The Five-hundredmeter Aperture Spherical radio Telescope(FAST),that incorporates an L-band 19-beam receiver with a system temperature of about 20 K,is the most sensitive radio telescope utilized for discovering pulsars.We designed the snapshot observation mode for a FAST key science project,the Galactic Plane Pulsar Snapshot(GPPS)survey,in which every four nearby pointings can observe a cover of a sky patch of 0.1575 square degrees through beam-switching of the L-band 19-beam receiver.The integration time for each pointing is 300 seconds so that the GPPS observations for a cover can be made in 21 minutes.The goal of the GPPS survey is to discover pulsars within the Galactic latitude of±10∘from the Galactic plane,and the highest priority is given to the inner Galaxy within±5∘.Up to now,the GPPS survey has discovered 201 pulsars,including currently the faintest pulsars which cannot be detected by other telescopes,pulsars with extremely high dispersion measures(DMs)which challenge the currently widely used models for the Galactic electron density distribution,pulsars coincident with supernova remnants,40 millisecond pulsars,16 binary pulsars,some nulling and mode-changing pulsars and rotating radio transients(RRATs).The follow-up observations for confirmation of new pulsars have polarization-signals recorded for polarization profiles of the pulsars.Re-detection of previously known pulsars in the survey data also leads to significant improvements in parameters for 64 pulsars.The GPPS survey discoveries are published and will be updated at http://zmtt.bao.ac.cn/GPPS/. | J.L.Han Chen Wang P.F.Wang Tao Wang D.J.Zhou Jing-Hai Sun Yi Yan Wei-Qi Su Wei-Cong Jing Xue Chen X.Y.Gao Li-Gang Hou Jun Xu K.J.Lee Na Wang Peng Jiang Ren-Xin Xu Jun Yan Heng-Qian Gan Xin Guan Wen-Jun Huang Jin-Chen Jiang Hui Li Yun-Peng Men Chun Sun Bo-Jun Wang H.G.Wang Shuang-Qiang Wang Jin-Tao Xie Heng Xu Rui Yao Xiao-Peng You D.J.Yu Jian-Ping Yuan Rai Yuen Chun-Feng Zhang Yan Zhu | 2021 | Research in Astronomy and Astrophysics2021，21，5： | 4 |
| 10 | Transboundary eco-security and its regulation system in the Longitudinal Range-Gorge Region显示文摘这份报纸讨论了 transboundary eco 安全问题,他们的分发模式,特征和驱动力,和在纵的范围峡区域(LRGR ) 的规定系统。除了沙灰尘暴风雨,主要 transboundary eco 安全问题能在 LRGR 沿着中国的陆上的边阶区域被发现。直接驱动力包括了串联水力发出的电力水坝,高速公路和国际航行开发的构造,斜坡陆地耕作和矿物质探索。Transboundary eco 安全问题沿着国际水路在陆上的区域,和下游的国家影响附近的区域。在邻国的生态的变化在 LRGR 在国内方面上有效果,例如种类侵略。综合措施应该被考虑,包括边阶 eco 保护工程和 transboundary 自然保护区的构造,生态的阀值安装,种类侵略控制,监视平台的 eco 安全的建立,组成生态的赔偿机制和法律(规则) 并且机构,和能力大楼。在 LRGR 处理 transboundary 问题的最重要的任务是国际性地形成参与合作机制,为 transboundary eco 安全建立资金,实现生态的赔偿策略,并且开发信息交换站台和警告系统。 | HE DaMing LIU Jiang HU JinMing FEN Yan GAN Su | 2007 | Chinese Science Bulletin2007，52，A02： | 4 |
| 11 | Progress of Jinping Underground laboratory for Nuclear Astrophysics(JUNA)显示文摘Jinping Underground laboratory for Nuclear Astrophysics(JUNA) will take the advantage of the ultra-low background of CJPL lab and high current accelerator based on an ECR source and a highly sensitive detector to directly study for the first time a number of crucial reactions occurring at their relevant stellar energies during the evolution of hydrostatic stars. In its first phase, JUNA aims at the direct measurements of^(25)Mg(p,γ)^(26)Al,^(19)F(p,α)^(16)O,^(13)C(α,n)^(16)O and ^(12)C(α,γ)^(16)O reactions. The experimental setup,which includes an accelerator system with high stability and high intensity, a detector system, and a shielding material with low background, will be established during the above research. The current progress of JUNA will be given. | WeiPing Liu ZhiHong Li JiangJun He XiaoDong Tang Gang Lian Zhu An JianJun Chang Han Chen QingHao Chen XiongJun Chen ZhiJun Chen BaoQun Cui XianChao Du ChangBo Fu Lin Gan Bing Guo GuoZhu He Alexander Heger SuQing Hou HanXiong Huang Ning Huang BaoLu Jia LiYang Jiang Shigeru Kubono JianMin Li KuoAng Li Tao Li YunJu Li Maria Lugaro XiaoBing Luo HongYi Ma ShaoBo Ma DongMing Mei YongZhong Qian JiuChang Qin Jie Ren YangPing Shen Jun Su LiangTing Sun WanPeng Tan Isao Tanihata Shuo Wang Peng Wang YouBao Wang Qi Wu ShiWei Xu ShengQuan Yan LiTao Yang Yao Yang XiangQing Yu Qian Yue Sheng Zeng HuanYu Zhang Hui Zhang LiYong Zhang NingTao Zhang QiWei Zhang Tao Zhang XiaoPeng Zhang XueZhen Zhang ZiMing Zhang Wei Zhao Zuo Zhao Chao Zhou | 2016 | Science China(Physics,Mechanics & Astronomy)2016，59，4： | 3 |
| 12 | The Science Operations and Data Center (SODC) of the ASO-S mission显示文摘A ground data analysis center is very important to the success of a mission.We introduce the Science Operations and Data Center(SODC)for the ASO-S mission,which consists of a scientific operation subcenter,a data management subcenter,a data analysis subcenter and a user service subcenter.The mission planning process,instrument observation modes and the data volume are presented.We describe the data flow and processing procedures from spacecraft telemetry to high-level science data,and the long-term archival as well.The data policy and distributions are also briefly introduced. | Yu Huang Hui Li Wei-Qun Gan You-Ping Li Jiang-Tao Su Yuan-Yong Deng Li Feng Yang Su Wei Chen Shi-Jun Lei Ying Li Yun-Yi Ge Ying-Na Su Si-Ming Liu Jing-Jing Zang Zun-Lei Xu Xian-Yong Bai Jing-Wei Li | 2019 | Research in Astronomy and Astrophysics2019，19，11： | 3 |
| 13 | Joint hard X-ray observations with ASO-S/HXI and SO/STIX显示文摘This paper discusses the potential of future joint hard X-ray solar flare observations between the Hard X-ray Imager(HXI)onboard the Advanced Space-based Solar Observatory(ASO-S)mission and the Spectrometer/Telescope for Imaging X-rays(STIX)on Solar Orbiter.The different viewing perspectives of the two telescopes relative to the Sun will allow us for the first time to systematically study non-thermal hard X-ray emissions stereoscopically.During the 4-years of the nominal mission of ASO-S,we expect to jointly observe about 160 flares above GOES M1 class to systematically study hard X-ray directivity.For about 16 partially limb-occulted STIX flares,we will have observations of the entire flare by HXI.Such observations will enable us to simultaneously study the all-important coronal hard X-ray sources,which are generally lost in the instrument’s individual imaging dynamic range,in combination with the chromospheric footpoint emissions.The two different detector systems used in the two telescopes make the relative calibration between the two instruments a key task that needs to be addressed before creditable science results can be published.If an accurate inter-calibration can be achieved using jointly observed flares on the disk,observations with HXI and STIX will provide new and essential key diagnostics for solar flare physics. | Sam Krucker Gordon JHurford Yang Su Wei-Qun Gan | 2019 | Research in Astronomy and Astrophysics2019，19，11： | 3 |
| 14 | Carbon combustion synthesis of lithium cobalt oxide as cathode material for lithium ion battery显示文摘Lithium cobalt oxide(LiCoO2) was synthesized by carbon combustion synthesis(CCS) using carbon as fuel.X-ray diffraction(XRD) and scanning electron microscope(SEM) measurements showed that carbon combustion led to the formation of layered structure of LiCoO2 and the particle size could be controlled by carbon content.For the LiCoO2 sample prepared at 800℃ for 2 h,at molar ratio of C/Co=0.5,the particle-size distribution fell in the narrow range of 3-5 m.Electrochemical tests indicated this LiCoO2 sample delivered an initial discharge capacity of 148 mAh/g with capacity retention rate higher than 97% after 10 cycles. | Yongle Gan Li Zhang Yanxuan Wen Fan Wang Haifeng Su | 2008 | Particuology2008，6，2： | 3 |
| 15 | Parametrization of woods-saxon potential for heavy-ion systems显示文摘Several elastic scattering angular distributions of ^(12)C from target nuclei of A ≥39 are analyzed to extract the Woods-Saxon potential parameters with the fixed imaginary potential and Coulomb radius parameters.Using the best fitted diffuseness parameters,the correlations of the real part parameters with A_1^(1/3)+ A_2^(1/3) and incident energy are revealed, and the systematic Woods-Saxon potential parameters are presented for nucleus-nucleus interaction.The proposed potential parameters can reproduce not only the elastic scattering angular distributions induced by ^(12)C,but also many elastic scattering angular distributions induced by the projectiles other than ^(12)C,thus providing important inputs for the study of nuclear reactions of heavy-ion systems. | Lin Gan ZhiHong Li HuiBin Sun DanYang Pang Bing Guo YunJu Li Jun Su ShengQuan Yan ErTao Li YouBao Wang Gang Lian ZhiYu Han XinYue Li DongHui Li TianLi Ma ChangJin Pei YangPing Shen Yi Su Sheng Zeng Yong Zhou WeiPing Liu | 2017 | Science China(Physics,Mechanics & Astronomy)2017，60，8： | 2 |
| 16 | Double hard X-ray peaks in RHESSI flares as evidence of chromospheric evaporation and implications for modifying the Neupert effect显示文摘Among the RHESSI flare samples,we concentrated on a kind of flare that presents two successive peaks(that is,it presents both an impulsive phase and a gradual phase)in 12-25 keV light curves.Taking the C1.4 flare on 2002 August 12 as an example,we studied the light curves,spectra,and images in detail.Making full use of the capabilities of RHESSI,we showed some evidence to support the expected causal relationship between these two peaks:the first peak is mainly nonthermal,while the second peak is mainly thermal;the energy carried by nonthermal electrons during the first peak seems to be comparable to the thermal energy of the second peak.The morphologies of X-ray images and their evolutions provide additional evidence for this causality.We conclude that two such peaks in the 12-25 keV light curve are good evidence for the chromospheric evaporation.However,the maximum time of the second peak is later than the end time of the first peak,suggesting that for some events,a modification of the traditional Neupert effect could be necessary by inclusion of a time delay,which might be partly related to the filling of the loop by evaporated material. | You-Ping Li Wei-Qun Gan Yang Su | 2009 | Research in Astronomy and Astrophysics2009，9，10： | 2 |
| 17 | EjBZR1 represses fruit enlargement by binding to the EjCYP90 promoter in loquat显示文摘Loquat(Eriobotrya japonica)is a subtropical tree that bears fruit that ripens during late spring.Fruit size is one of the dominant factors inhibiting the large-scale production of this fruit crop.To date,little is known about fruit size regulation.In this study,we first discovered that cell size is more important to fruit size than cell number in loquat and that the expression of the EjBZR1 gene is negatively correlated with cell and fruit size.Virus-induced gene silencing(VIGS)of EjBZR1 led to larger cells and fruits in loquat,while its overexpression reduced cell and plant size in Arabidopsis.Moreover,both the suppression and overexpression of EjBZR1 inhibited the expression of brassinosteroid(BR)biosynthesis genes,especially that of EjCYP90A.Further experiments indicated that EjCYP90A,a cytochrome P450 gene,is a fruit growth activator,while EjBZR1 binds to the BRRE(CGTGTG)motif of the EjCYP90A promoter to repress its expression and fruit cell enlargement.Overall,our results demonstrate a possible pathway by which EjBZR1 directly targets EjCYP90A and thereby affects BR biosynthesis,which influences cell expansion and,consequently,fruit size.These findings help to elucidate the molecular functions of BZR1 in fruit growth and thus highlight a useful genetic improvement that can lead to increased crop yields by repressing gene expression. | Wenbing Su Zikun Shao Man Wang Xiaoqing Gan Xianghui Yang Shunquan Lin | 2021 | Horticulture Research2021，8，1： | 2 |
| 18 | Volatile Oil of Platycladus Orientalis(L.)Franco Leaves Exerts Strong Anti-inflammatory Effects via Inhibiting the IκB/NF-κB Pathway显示文摘This study was designed to investigate the anti-inflammatory effects of volatile oil of Platycladus orientalis(L.)Franco leaves(VOPF)and the underlying molecular mechanisms by using the non-infectious inflammation rat models and infectious inflammation mouse models.Ear swelling and intraperitoneal capillary permeability in mice,and carrageenan-induced toe swelling and cotton ball-induced granuloma in rats were used to reveal anti-inflammatory effects of VOPF.Moreover,the lipopolysaccharide(LPS)-induced mouse model of acute lung injury was used to explore the anti-inflammatory mechanism of VOPF.The results showed that VOPF could significantly inhibit auricular swelling,intraperitoneal capillary permeability in mice,and reduce granuloma swelling and paw swelling in rats.Furthermore,it significantly alleviated the pathological damage of the lung tissue.In addition,VOPF could reduce the contents of IL-1β and TNF-αand increase the content of IL-10 in the serum.It had little effect on the expression of p65 but reduced the phosphorylation level of p65 and IκB in NF-κB pathway.In conclusion,VOPF has anti-inflammatory effects and the mechanisms involve the down-regulation of the phosphorylation levels of p65 and IκB and blockage of the NF-κB signaling pathway. | Da-li GAN Yan YAO Han-wen SU Yu-ying HUANG Jun-feng SHI Xiong-biao LIU Mei-xian XIANG | 2021 | Current Medical Science2021，41，1： | 2 |
| 19 | Expression of a variant of CD28 on a subpopulation of human NK cells : implications for B7 - mediated stimulation of NK cells 显示文摘 | Galea - Lauri J Darling D Gan SU | 1999 | J Immunol1999，163，1： | 1 |
| 20 | Keloid fibroblasts are more sensitive to Wnt3a treatment in terms of elevated cellular growth and fibronectin expression显示文摘 | Chua AW Gan SU Ting Y | 2011 | J Dermatol Sei2011，64，3： | 1 |
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