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| 1 | Magnetohydrodynamics (MHD) numerical simulations on the interaction of the solar wind with the magnetosphere: A review显示文摘The magnetosphere is the outermost layer of the geospace, and the interaction of the solar wind with the magnetosphere is the key element of the space weather cause-and-effect chain process from the Sun to Earth, which is one of the most challenging scientific problems in the geospace weather study. The nonlinearity, multiple component, and time-dependent nature of the geospace make it very difficult to describe the physical process in geospace using traditional analytic analysis approach. Numerical simulations, a new research tool developed in recent decades, have a deep impact on the theory and application of the geospace. MHD simulations started at the end of the 1970s, and the initial study was limited to two-dimensional (2D) cases. Due to the intrinsic three-dimensional (3D) characteristics of the geospace, 3D MHD simulations emerged in the 1980s, in an attempt to model the large-scale structures and fundamental physical processes in the magnetosphere. They started to combine with the space exploration missions in the 1990s and make comparisons with observations. Physics-based space weather forecast models started to be developed in the 21st century. Currently only a few space-power countries such as USA and Japan have developed 3D magnetospheric MHD models. With the rapid advance of space science in China, we have developed a new global MHD model, namely PPMLR-MHD, which has high order spatial accuracy and low numerical dissipation. In this review, we will briefly introduce the global 3D MHD modeling, especially the PPMLR-MHD code, and summarize our recent work based on the PPMLR-MHD model, with an emphasis on the interaction of interplanetary shocks with the magnetosphere, large-scale current systems, reconnection voltage and transpolar potential drop, and Kelvin-Helmholtz (K-H) instability at the magnetopause. | WANG Chi GUO XiaoCheng PENG Zhong TANG BinBin SUN TianRan LI WenYa HU YouQiu | 2013 | Science China Earth Sciences2013，56，7： | 10 |
| 2 | Tianwen-1 MINPA observations in the solar wind显示文摘The Mars Ion and Neutral Particle Analyzer(MINPA)is one of the three scientific instruments onboard the Tianwen-1 orbiter to investigate the Martian space environment.During Tianwen-1’s transfer orbit to Mars,the MINPA was switched on to measure the solar wind ions.Here,we present the first results of the MINPA observations in the solar wind.During cruise,nearly half of the MINPA ion field-of-view(FOV)was blocked by the lander capsule;thus only the solar-wind ions with azimuthal speeds pointing towards the unblocked FOV sectors could be detected.We perform a detailed comparison of the MINPA’s solar wind observations with data from Earth-based missions when MINPA reached its count-rate peak,finding a general consistency of the ion moments between them.The blocking effect due to the lander is evaluated quantitatively under varying solar-wind velocity conditions.Despite the blocking effect,the MINPA’s solar wind measurements during the transfer orbit suggest a good performance. | AiBing Zhang LingGao Kong WenYa Li Lei Li BinBin Tang ZhaoJin Rong Yong Wei JiJie Ma YiTeng Zhang LiangHai Xie YuXian Wang JianSen He Bin Liu WenJing Wang Bin Su JiaWei Li Xu Tan Fang Wang TaiFeng Jin FuHao Qiao Peter Wurz Yan Zhu YunFei Bai YiRen Li XinBo Zhu YueQiang Sun YongLiao Zou Chi Wang | 2022 | Earth and Planetary Physics2022，6，1： | 5 |
| 3 | Ameliorating effects of Inonotus obliquus on high fat diet-induced obese rats显示文摘根据从的数据,将在在一年 2030 的世界上有 21.6 亿过重和 11.2 亿个肥胖的个人[1 ] ,它提起多重疾病的风险例如高血压,癌症的糖尿病,心血管的疾病,和几种类型[2,3 ] 。肥胖被看作新陈代谢的混乱,它被高精力吸入主要导致。在哺乳动物,过量精力首先在脂肪质的织物作为 triglyceride (TG ) 被存储。在过去的十年,调整 adipogenesis 的过程的众多的分子很好被记录了。Peroxisome 激活 proliferator 的受体(PPAR-) 为脂肪质的织物的累积被要求并且贡献肥胖[4 ] 。甾醇规章的元素绑定蛋白质(SREBP ) 作为激活胆固醇和丰满的酸合成的全部节目的抄写因素的一个家庭被识别了[5 ] 。Glyceraldehydes 3 磷酸盐 acyltransferase (GPAT ) 和 diacylglycerol acyltransferase (DGAT ) 广泛地在哺乳动物的纸巾被表示并且催化第一并且在 TG 合成的最后的步,分别地[6 ] 。因此,这些分子可以是为肥胖和类脂化合物新陈代谢的评估的大目标。最近,阳光等。[7 ] 证明了在糖尿病的老鼠的类脂化合物的浆液层次显著地与 Inonotus obliquus 的文化肉汤的干燥的事在 3 星期的治疗以后被减少。李和 Hyun [8 ] 证明水摘录从我。obliquus 减少了高脂肪的饮食的胖重量喂的肥胖的老鼠。因此,我们对什么进一步感兴趣,是怎么能我。obliquus 摘录影响类脂化合物新陈代谢并且什么是位于这反肥胖效果下面的可能的机制。在现在的学习,我们造了一个高脂肪的导致食谱的老鼠模型。 | Tao Wu Qingyu Shu Kai Yang Xiaoxian Xie Xia Wang Yangling Wang Anqi Guo Nate Y-uan Binggong Zhao Binbin Chi QiaobeiWu Zhengwei Fu | 2015 | Acta Biochimica et Biophysica Sinica2015，47，9： | 4 |
| 4 | Spatial Interaction Between the Industrial Undertaking Capacity and Global Value Chain Position of East Asian Countries显示文摘A comprehensive understanding of the spatial interaction between the industrial undertaking capability and the position of the global value chain of the 12 East Asian countries is conducive to strengthening regional cooperation, gaining a say in foreign trade and becoming the dominant player in the global division of labor system. The article reveals the operating rules of the interaction between the industrial undertaking capacity and the global value chain position of East Asian countries by calculating the Global Moran Index(Moran’s I), coupling coordination degree and other indicators. The results show that: in time, the values of industrial undertaking capacity and the positions of global value chain in East Asian countries showed a sustained and stable growth trend, and have a consistent trend of change. Spatially, both of the two indexes had significant positive spatial correlation, with Moran’s I showing an ‘inverted U’pattern, and the spatial aggregation distribution of global value chain position lagged behind the spatial aggregation distribution of industrial undertaking capacity by one year. In terms of spatial coupling coordination, the coupling coordination values of the two indicators show a steady upward trend. Combined with the comparative advantage of each country, this paper provides suggestions for promoting the positions of Chinese and other East Asian industries in the global value chain from the perspectives of enhancing independent innovation capability and upgrading industrial structure. | ZHU Binbin CHI Fangyuan DU Lei | 2021 | Chinese Geographical Science2021，31，1： | 3 |
| 5 | Improved method to derive equivalent current systems from global MHD simulations显示文摘Derivation of equivalent current systems(ECS)from a global magnetospheric magnetohydrodynamics(MHD)model is very useful in studying magnetosphere-ionosphere coupling,ground induction effects,and space weather forecast.In this study we introduce an improved method to derive the ECS from a global MHD model,which takes account of the obliqueness of the magnetic field lines.By comparing the ECS derived from this improved method and the previous method,we find that the main characteristics of the ECS derived from the two methods are generally consistent with each other,but the eastward-westward component of the geomagnetic perturbation calculated from the ECS derived from the improved method is much stronger than that from the previous method.We then compare the geomagnetic perturbation as a function of the interplanetary magnetic field(IMF)clock angle calculated from the ECS derived from both methods with the observations.The comparison indicates that the improved method can improve the performance of the simulation.Furthermore,it is found that the incomplete counterbalance of the geomagnetic effect produced by the ionospheric poloidal current and field-aligned current(FAC)contributes to most of the eastward-westward component of geomagnetic perturbation. | ZHANG JiaoJiao WANG Chi TANG BinBin | 2014 | Science China Earth Sciences2014，57，1： | 3 |
| 6 | The solar wind plasma upstream of Mars observed by Tianwen-1:Comparison with Mars Express and MAVEN显示文摘On the great journey to Mars,China’s first planetary exploration mission,the Tianwen-1 came within 26 million kilometers of Mars from 31 October 2020 to 25 January 2021 and was getting closer to its destination,the red planet,in search of answers to the cataclysmic climate change that occurred in Martian history.Both the escape of the Martian atmosphere and the loss of surface water were firmly influenced by solar activities.Tianwen-1 provided a unique chance to depict the solar wind streams between Earth and Mars during the minimum of Solar Cycle 25.During the three-month cruise phase of Tianwen-1,the solar wind flows were successively observed at Earth,Tianwen-1,and Mars.After the field of view correction and noise reduction,the solar wind velocity and density measured by Tianwen-1 show good agreement with those at Earth and Mars.The results indicate that the performance of the ion analyzer onboard the Tianwen-1 orbiter is reliable and stable.It is worth looking forward to the joint observations of ion escape with other Mars probes in the following Martian years. | Kai FAN Limei YAN Yong WEI Aibing ZHANG Linggao KONG Markus FRÄNZ Fei HE Lihui CHAI Chongjing YUAN Yuqi WANG Jun ZHONG Zhaojin RONG Zhonghua YAO Yongxin PAN Jun CUI Jiansen HE Wenya LI Binbin TANG Chi WANG | 2022 | Science China Earth Sciences2022，65，4： | 2 |
| 7 | Large scale current systems developed from substorm onset:Global MHD results显示文摘We investigate the large-scale substorm current systems developed from its onset in an idealized substorm event simulated by global magnetohydrodynamic(MHD) models. Mainly three current systems(loops) are revealed:(1) the classical substorm current wedge, which is composed by the disputed cross-tail current in the magnetotail, the nightside westward electrojet in the high-latitude ionosphere and a pair of region 1 field-aligned currents(FAC);(2) the partial-ring current system, which is braced by two region 2 FACs; and(3) the meridional current system, which is formed by an equatorial radial current(outward/inward in the morning/evening sector), and region 1 and region 2 FACs at its two ends. The region 2 FAC connects with region 1 FAC by a latitudinal horizontal current at each morning/evening ionosphere to complete Loops 2 and 3. A quantitative study shows the significant enhancement of these current systems during the substorm expansion phase, while Loop 1 dominates, which can reach a magnitude of ~1 MA. Empirical relations among the ionospheric currents and the related magnetotail currents are established based on the simulation results, implying that the substonn current systems are not evolved locally or separately, but must be viewed from a global perspective. This knowledge of large-scale substorm current system would deepen our understanding of the substorm development and could be validated by observations in the future. | TANG BinBin WANG Chi | 2018 | Science China(Technological Sciences)2018，61，3： | 2 |
| 8 | An altered CD8^(+) T cell epitope of insulin prevents type 1 diabetes in humanized NOD mice显示文摘Autoreactive CD8^(+)T cells,which play an indispensable role inβcell destruction,represent an emerging target for the prevention of type 1 diabetes(T1D).Altered peptide ligands(APLs)can efficiently induce antigen-specific T cells anergy,apoptosis or shifts in the immune response.Here,we found that HLA-A*0201-restricted CD8^(+)T cell responses against a primaryβ-cell autoantigen insulin epitope InsB15–14 were present in both NOD.β2m null.HHD NOD mice and T1D patients.We generated several APL candidates for InsB15–14 by residue substitution at the p6 position.Only H6F exhibited an inhibitory effect on mInsB1_(5–14)-specific CD8^(+)T cell responses in vitro.H6F treatment significantly reduced the T1D incidence,which was accompanied by diminished autoreactive CD8^(+)T cell responses to mInsB15-14,inhibited infiltration of CD8^(+)and CD4^(+)T cells in the pancreas and reduced pro-inflammatory cytokine production in pancreatic and splenic T cells in NOD.β2m^(null).HHD mice.Mechanistically,H6F treatment significantly augmented a tiny portion of CD8^(+)CD25^(+)Foxp3^(+)T cells in the spleen and especially in the pancreas.This subset exhibited typical Treg phenotypes and required peptide-specific restimulation to exert immunosuppressive activity.Therefore,this APL H6F may be a promising candidate with potential clinical application value for antigen-specific prevention of T1D. | Mengjun Zhang Shufeng Wang Binbin Guo Gang Meng Chi Shu Wenli Mai Qian Zheng Xiaoling Chen Yuzhang Wu Li Wang | 2019 | Cellular & Molecular Immunology2019，16，6： | 1 |
| 9 | Experimental study of the loop heat pipe with a flat disk-shaped evaporator 显示文摘 | Wang Dongdong Liu Zhichun Shen Jun Jiang Chi Chen Binbin Yang Jinguo Tu Zhengkai Liu Wei | 2014 | Experimental Thermal and Fluid Science2014，57，： | 1 |
| 10 | Deformations at Earth’s dayside magnetopause during quasi-radial IMF conditions:Global kinetic simulations and Soft X-ray Imaging显示文摘The Solar wind Magnetosphere Ionosphere Link Explorer(SMILE)is a joint mission of the European Space Agency(ESA)and the Chinese Academy of Sciences(CAS).Primary goals are investigating the dynamic response of the Earth's magnetosphere to the solar wind(SW)impact via simultaneous in situ magnetosheath plasma and magnetic field measurements,X-Ray images of the magnetosheath and magnetic cusps,and UV images of global auroral distributions.Magnetopause deformations associated with magnetosheath high speed jets(HSJs)under a quasi-parallel interplanetary magnetic field condition are studied using a threedimensional(3-D)global hybrid simulation.Soft X-ray intensity calculated based on both physical quantities of solar wind proton and oxygen ions is compared.We obtain key findings concerning deformations at the magnetopause:(1)Magnetopause deformations are highly coherent with the magnetosheath HSJs generated at the quasi-parallel region of the bow shock,(2)X-ray intensities estimated using solar wind h+and self-consistentO7+ions are consistent with each other,(3)Visual spacecraft are employed to check the discrimination ability for capturing magnetopause deformations on Lunar and polar orbits,respectively.The SMILE spacecraft on the polar orbit could be expected to provide opportunities for capturing the global geometry of the magnetopause in the equatorial plane.A striking point is that SMILE has the potential to capture small-scale magnetopause deformations and magnetosheath transients,such as HSJs,at medium altitudes on its orbit.Simulation results also demonstrate that a lunar based imager(e.g.,Lunar Environment heliospheric X-ray Imager,LEXI)is expected to observe a localized brightening of the magnetosheath during HSJ events in the meridian plane.These preliminary results might contribute to the pre-studies for the SMILE and LEXI missions by providing qualitative and quantitative soft X-ray estimates of dayside kinetic processes. | ZhongWei Yang RiKu Jarvinen XiaoCheng Guo TianRan Sun Dimitra Koutroumpa George K.Parks Can Huang BinBin Tang QuanMing Lu Chi Wang | 2024 | Earth and Planetary Physics2024，8，1： | 1 |
| 11 | Modeling the Jovian magnetosphere under an antiparallel interplanetary magnetic field from a global MHD simulation显示文摘We present preliminary results of a new global Magnetohydrodynamics(MHD) simulation model of the Jovian magnetosphere.The model incorporates mass loading from Jupiter's satellite Io, the planet's fast corotation, and electrostatic coupling between its magnetosphere and ionosphere(M-I coupling). The basic configuration of the Jovian magnetosphere including the equatorial plasma flow pattern, the corotation enforcement current system, and the field aligned currents(FACs) in the ionosphere are presented under an antiparallel interplanetary magnetic field(IMF) condition. The simulation model results for equatorial density and pressure profiles are consistent with results from data-based empirical models. It is also found that there are similarities between the FACs distribution in the ionosphere and the observed aurora features, showing the potential application of the simple ionospheric model to the complicated M-I coupling. This model will help deepen our understanding of the global dynamics of the Jovian magnetosphere. | YuXian Wang XiaoCheng Guo BinBin Tang WenYa Li Chi Wang | 2018 | Earth and Planetary Physics2018，2，4： | 1 |
| 12 | Invariant Modulation of IMF Clock Angle on the Solar Wind Energy Input into the Magnetosphere显示文摘By use of the global PPMLR Magnetohydrodynamics(MHD) model,a serial of quasisteady-state numerical simulations were conducted to examine the modulation property of the interplanetary magnetic field clock angle θ on the solar wind energy input into the magnetosphere.All the simulations can be divided into seven groups according to different criteria of solar wind conditions.For each group,37 numerical examples are analyzed,with the clock angle varying from 0° to 360° with an interval of 10°,keeping the other solar wind parameters(such as the solar wind number density,velocity,and the magnetic field magnitude) unchanged.As expected,the solar wind energy input into the magnetosphere is modulated by the IMF clock angle.The axisymmetrical bell-shaped curve peaks at the clock angle of 180°.However,the modulation effect remains invariant with varying other solar wind conditions.The function form of such an invariant modulation is found to be sin(0/2)^(2.70) + 0.25. | HAN Jinpeng LI Hui TANG Binbin WANG Chi | 2015 | 空间科学学报2015，35，6： | 0 |
| 13 | Unraveling the Effects of Austenitizing Temperature and Austenite Grain Size on the Crystallographic Characteristics and Mechanical Properties of Martensitic Transformation Products in a Low‑Alloy Steel显示文摘The influence of austenitizing temperature and austenite grain size on the crystallographic characteristics and mechanical properties of transformation products was investigated in a low-alloy steel.Annealing at a lower temperature after austenitization at 1050℃ can reduce the vacancy concentration and enhance the stability of austenite,thereby determining the martensite-start(Ms)temperature and density of twin-related V1/V2 variant pairs.V1/V2 variant pairs are predominately generated by autocatalytic nucleation,which can promote transformation by self-accommodation.Annealing at 800℃ after austenitization at 1050℃ generated the highest content of V1/V2 variant pairs,which contributed to high values of strength,Charpy impact energy,and elongation.In addition to refining the austenite grain size,niobium(Nb)microalloying increases the packet boundaries of the transformation products,mainly because the refined austenite grains provide more nucleation sites for the martensitic transformation.However,the density of block boundaries decreases after austenite refinement by Nb microalloying,owing to insufficient autocatalytic nucleation. | Binbin Wu Fangzhong Hu Zhiquan Wang Shaopeng Yang Rui Zhong Chengjia Shang Zhigang Yang Chi Zhang | 2023 | Acta Metallurgica Sinica(English Letters)2023，36，4： | 0 |
| 14 | Determination of the Kelvin-Helmholtz Wave Parameters on the Magnetopause in Single-spacecraft Observations显示文摘Kelvin-Helmholtz(K-H) waves are formed from the triggering of the K-H instability on the magnetopause,which is a candidate mechanism for solar wind entry into the magnetosphere,especially under northward interplanetary magnetic field conditions.In this study,a K-H wave event was identified from the observation of probe B of the Time History of Events and Macroscale Interactions during Substorms(THEMIS) mission on 15 May 2008.A new method to determine the wave parameters of the K-H waves in single-spacecraft observations is proposed.The dominant wave period is determined by three kinds of spectrograms for three key parameters,namely the ion density,the ion temperature,and the z component of magnetic field.The phase velocity is estimated by calculating the center-of-mass velocity of the detected K-H vortex region.This approximation is validated by comparison with other alternative methods.The method to determine the wave parameters is a first step to further study K-H wave properties and their relationship with interplanetary conditions. | LIN Dong WANG Chi LI Wenya TANG Binbin | 2015 | 空间科学学报2015，35，4： | 0 |
| 15 | Endoscopic resection of a huge Brunner’s gland adenoma显示文摘Brunner’s gland adenoma is a rare tumour of the duodenum,which is usually benign.A 71-year-old woman presenting with epigastric pain,upper gastro-intestinal haemorrhage and melaena was reported in this paper.Upper gastro-intestinal(GI)endoscopy revealed a large pedunculated tumour on the superior part of the duodenal bulb.Endoscopic polypectomy was successfully performed by clipping and nylon thread without any com-plications.Histological examination revealed a Brunner’s gland adenoma. | Binbin ZHANG Xu REN Xiufen TANG Yuxin CHI Xuesong SHI | 2008 | Frontiers of Medicine2008，2，4： | 0 |
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