Ti-6Al-4Zr-2Sn-6Mo alloy is one of the most recent titanium alloys processed using powder bed fusion-laser beam(PBF-LB)technology.This alloy has the potential to replace Ti-6Al-4V in automotive and aerospace applicati...Ti-6Al-4Zr-2Sn-6Mo alloy is one of the most recent titanium alloys processed using powder bed fusion-laser beam(PBF-LB)technology.This alloy has the potential to replace Ti-6Al-4V in automotive and aerospace applications,given its superior mechanical properties,which are approximately 10%higher in terms of ultimate tensile strength(UTS)and yield strength after appropriate heat treatment.In as-built conditions,the alloy is characterized by the presence of soft orthorhombicα″martensite,necessitating a postprocessing heat treatment to decompose this phase and enhance the mechanical properties of the alloy.Usually,PBFed Ti6246 components undergo an annealing process that transforms theα″martensite into anα-βlamellar microstructure.The primary objective of this research was to develop a solution treatment and aging(STA)heat treatment tailored to the unique microstructure produced by the additive manufacturing process to achieve an ultrafine bilamellar microstructure reinforced by precipitation hardening.This study investigated the effects of various solution temperatures in theα-βfield(ranging from 800 to 875℃),cooling media(air and water),and aging time to determine the optimal heat treatment parameters for achieving the desired bilamellar microstructure.For each heat treatment condition,differentα-βmicrostructures were found,varying in terms of theα/βratio and the size of the primaryα-phase lamellae.Particular attention was given to how these factors were influenced by increases in solution temperature and how microhardness correlated with the percentage of the metastableβphase present after quenching.Tensile tests were performed on samples subjected to the most promising heat treatment parameters.A comparison with literature data revealed that the optimized STA treatment enhanced hardness and UTS by13%and 23%,respectively,compared with those of the annealed alloy.Fracture surface analyses were conducted to investigate fracture mechanisms.展开更多
本文基于近岸海洋数值模式ADCIRC(a parallel advanced circulation model for oceanic,coastal and estuarine waters)和近海波浪数值模式SWAN(simulating waves nearshore),建立了适用于文昌市的高分辨率风暴潮-海浪耦合漫滩模型,并以...本文基于近岸海洋数值模式ADCIRC(a parallel advanced circulation model for oceanic,coastal and estuarine waters)和近海波浪数值模式SWAN(simulating waves nearshore),建立了适用于文昌市的高分辨率风暴潮-海浪耦合漫滩模型,并以1415“海鸥”路径为基础,构建了覆盖文昌市岸段的台风路径集,对登陆位置进行敏感性分析,结果表明,在相同台风参数下,登陆位置对文昌市沿岸的增水幅度有明显影响。通过构建不同台风强度路径集,对比分析了不同台风强度下文昌市的风暴潮淹没情况,开展危险性分析。结果显示台风强度越强,引起的风暴潮淹没范围越大,淹没水深越深,高危险性面积越大。随着台风强度的降低,淹没范围逐渐减小,但由于八门湾、铺前湾地势较低,河道、滩涂较多,在990 hPa的强度下仍出现超过1.2 m的淹没水深,为易受灾区域,需要多加关注和防范。展开更多
In the quest for the development of safer lithium-metal batteries(LMBs),the integration of inorganic fillers and ionic liquids into polymer matrices has emerged as a promising strategy to enhance safety,ionic conducti...In the quest for the development of safer lithium-metal batteries(LMBs),the integration of inorganic fillers and ionic liquids into polymer matrices has emerged as a promising strategy to enhance safety,ionic conductivity and battery performance.This study introduces a novel composite ionogel(IG)synthesized through a facile one-pot method,incorporating butyl methacrylate(BMA)and poly(ethylene glycol)diacrylate(PEGDA)with the ionic liquid 1-butyl-1-methylpyrrolidinium bis(fluorosulfonyl)imide(PYR_(14)FSI)and garnet Li_(6.4)La_(3)Zr_(1.4)Ta_(0.6)O_(12)(LLZTO)nanoparticles.A distinctive feature of the approach is the use of an organosilane functionalization of the LLZTO nanoparticles,which ensures their full integration into the polymer matrix during free-radical polymerization.Moreover,this method effectively eliminates the Li_(2)CO_(3)passivation layer that typically forms on the surface of the LLZTO nanoparticles,thus,further contributing to an enhanced performance.As a result,a LMB with the functionalized LLZTO IG electrolyte delivered more than 160 mA h g^(−1)with a very good capacity retention of 97.7%after 400 cycles in Li|IG|LFP cells.展开更多
ENN He Long-2(EHL-2)is the next-generation large mega-Ampere(MA)spherical torus(ST)proposed and funded by the ENN company.The design parameters are:Ti0>30 keV,n_(e0)~1×10^(20)m^(-3),Ip~3 MA,Bt~3 T.One of the b...ENN He Long-2(EHL-2)is the next-generation large mega-Ampere(MA)spherical torus(ST)proposed and funded by the ENN company.The design parameters are:Ti0>30 keV,n_(e0)~1×10^(20)m^(-3),Ip~3 MA,Bt~3 T.One of the biggest challenges of EHL-2 is how to achieve several MA current flat-tops with limited voltage-seconds(Vs)of the center solenoid(CS)coils.In order to minimize the consumption of Vs,a fully non-inductive start-up by electron cyclotron resonance heating(ECRH)will be applied in EHL-2.The ramp-up phase will be accomplished with the synergetic mode between the CS and non-inductive methods.The strategy of non-inductive start-up and ramp-up with synergetic mode has been verified on EXL-50U’s experiments.Based on this strategy,numerical simulations indicate the feasibility of EHL-2 achieving 3 MA plasma current.A high-performance steady-state scenario with Ip~1.5 MA is also designed.In this scenario,the bootstrap current fraction fBS>70%,the safety factor q at the magnetic axis q0>2,the minimum safety factor qmin>1,the poloidal betaβp>3 and normalized betaβN>2.3.Each design iteration integrates the validation of physical models with the constraints of engineering implementation,gradually optimizing the performance of the heating and current drive(H&CD)systems.Numerical simulation results for general auxiliary H&CD systems such as neutral beam injection(NBI),electron cyclotron(EC)wave,ion cyclotron wave(ICW),and lower hybrid wave(LHW)are presented.These simulation results ensure that the 31 MW H&CD systems comprehensively cover all scenarios while maintaining engineering feasibility.展开更多
Early multiwavelength observations offer crucial insights into the nature of the relativistic jets responsible for gamma-ray bursts and their interaction with the surrounding medium.We present data of GRB 240825A from...Early multiwavelength observations offer crucial insights into the nature of the relativistic jets responsible for gamma-ray bursts and their interaction with the surrounding medium.We present data of GRB 240825A from 17 space-and ground-based telescopes/instruments,covering wavelengths from NIR/optical to X-ray and GeV,and spanning from the prompt emission to the afterglow phase triggered by Swift and Fermi.The early afterglow observations were carried out by SVOM/C-GFT,and spectroscopic observations of the afterglow by GTC,VLT,and TNG determined the redshift of the burst(z=0.659)later.A comprehensive analysis of the prompt emission spectrum observed by Swift-BAT and Fermi-GBM/LAT reveals a rare and significant high-energy cutoff at 76 MeV.Assuming this cutoff is due toγγabsorption allows us to place an upper limit on the initial Lorentz factor,Γ_(0)<245.The optical/NIR and GeV afterglow light curves can be described by the standard external shock model,with early-time emission dominated by a reverse shock(RS)and a subsequent transition to forward shock(FS)emission.Our afterglow modeling yields a consistent estimate of the initial Lorentz factor(Γ_(0)∼234).Furthermore,the RS-to-FS magnetic field ratio(R 302B)indicates that the RS region is significantly more magnetized than the FS region.An isotropic-equivalent kinetic energy of E_(k,iso)=5.25×10^(54) erg is derived,and the correspondingγ-ray radiation efficiency is estimated to beη_(γ)=3.1%.On the other hand,the standard afterglow model cannot reproduce the X-ray light curve of GRB 240825A,calling for improved models to characterize all multiwavelength data.展开更多
局地微地形产生的微气象环境是造成气象预报误差的重要因素之一,也是导致覆冰预报准确性不高的主要原因。该研究利用高精度MODIS系统15 s(约500 m)地形数据驱动中尺度天气研究和预报(weather research and forecasting,WRF)模式,并使用...局地微地形产生的微气象环境是造成气象预报误差的重要因素之一,也是导致覆冰预报准确性不高的主要原因。该研究利用高精度MODIS系统15 s(约500 m)地形数据驱动中尺度天气研究和预报(weather research and forecasting,WRF)模式,并使用基于决策树的梯度提升框架(light gradient boosting machine,LightGBM)对WRF预报进行订正,通过局地个例评估订正后的覆冰预测效果。结果表明:在假设条件下,过冷液滴覆冰速率随温度降低先快速增加,后增长速率保持不变,且液滴粒径越大,完全冻结所需温度越低;WRF-LightGBM订正算法在山区微地形下有效提升了温度预报准确度,典型冬季寒潮条件下预测温度与实际温度的误差在2℃以内,预报准确率为76%;以典型区域杆塔覆冰为例,输入订正后的温度和相对湿度数据后,覆冰融化时段被消除,覆冰厚度曲线与实际基本一致,增长速率接近一致。展开更多
基金financed by the European Union-Next Generation EU(National Sustainable Mobility Center CN00000023,Italian Ministry of University and Research Decree n.1033-17/06/2022,Spoke 11-Innovative Materials&Lightweighting)。
文摘Ti-6Al-4Zr-2Sn-6Mo alloy is one of the most recent titanium alloys processed using powder bed fusion-laser beam(PBF-LB)technology.This alloy has the potential to replace Ti-6Al-4V in automotive and aerospace applications,given its superior mechanical properties,which are approximately 10%higher in terms of ultimate tensile strength(UTS)and yield strength after appropriate heat treatment.In as-built conditions,the alloy is characterized by the presence of soft orthorhombicα″martensite,necessitating a postprocessing heat treatment to decompose this phase and enhance the mechanical properties of the alloy.Usually,PBFed Ti6246 components undergo an annealing process that transforms theα″martensite into anα-βlamellar microstructure.The primary objective of this research was to develop a solution treatment and aging(STA)heat treatment tailored to the unique microstructure produced by the additive manufacturing process to achieve an ultrafine bilamellar microstructure reinforced by precipitation hardening.This study investigated the effects of various solution temperatures in theα-βfield(ranging from 800 to 875℃),cooling media(air and water),and aging time to determine the optimal heat treatment parameters for achieving the desired bilamellar microstructure.For each heat treatment condition,differentα-βmicrostructures were found,varying in terms of theα/βratio and the size of the primaryα-phase lamellae.Particular attention was given to how these factors were influenced by increases in solution temperature and how microhardness correlated with the percentage of the metastableβphase present after quenching.Tensile tests were performed on samples subjected to the most promising heat treatment parameters.A comparison with literature data revealed that the optimized STA treatment enhanced hardness and UTS by13%and 23%,respectively,compared with those of the annealed alloy.Fracture surface analyses were conducted to investigate fracture mechanisms.
文摘本文基于近岸海洋数值模式ADCIRC(a parallel advanced circulation model for oceanic,coastal and estuarine waters)和近海波浪数值模式SWAN(simulating waves nearshore),建立了适用于文昌市的高分辨率风暴潮-海浪耦合漫滩模型,并以1415“海鸥”路径为基础,构建了覆盖文昌市岸段的台风路径集,对登陆位置进行敏感性分析,结果表明,在相同台风参数下,登陆位置对文昌市沿岸的增水幅度有明显影响。通过构建不同台风强度路径集,对比分析了不同台风强度下文昌市的风暴潮淹没情况,开展危险性分析。结果显示台风强度越强,引起的风暴潮淹没范围越大,淹没水深越深,高危险性面积越大。随着台风强度的降低,淹没范围逐渐减小,但由于八门湾、铺前湾地势较低,河道、滩涂较多,在990 hPa的强度下仍出现超过1.2 m的淹没水深,为易受灾区域,需要多加关注和防范。
基金the German Federal Ministry for Education and Research(BMBF)for financial support within the FB2-Hybrid project(03XP0428B)Moreover,D.Bresser and T.Diemant would like to acknowledge financial support from the Helmholtz Association.
文摘In the quest for the development of safer lithium-metal batteries(LMBs),the integration of inorganic fillers and ionic liquids into polymer matrices has emerged as a promising strategy to enhance safety,ionic conductivity and battery performance.This study introduces a novel composite ionogel(IG)synthesized through a facile one-pot method,incorporating butyl methacrylate(BMA)and poly(ethylene glycol)diacrylate(PEGDA)with the ionic liquid 1-butyl-1-methylpyrrolidinium bis(fluorosulfonyl)imide(PYR_(14)FSI)and garnet Li_(6.4)La_(3)Zr_(1.4)Ta_(0.6)O_(12)(LLZTO)nanoparticles.A distinctive feature of the approach is the use of an organosilane functionalization of the LLZTO nanoparticles,which ensures their full integration into the polymer matrix during free-radical polymerization.Moreover,this method effectively eliminates the Li_(2)CO_(3)passivation layer that typically forms on the surface of the LLZTO nanoparticles,thus,further contributing to an enhanced performance.As a result,a LMB with the functionalized LLZTO IG electrolyte delivered more than 160 mA h g^(−1)with a very good capacity retention of 97.7%after 400 cycles in Li|IG|LFP cells.
基金supported by ENN Group and ENN Energy Research Institute.The authors would like to express their gratitude for the contributions of the ENN fusion team and collaborators,such as Tiantian Sun,Haojie Ma,and Yong Guo,in supporting these endeavours.The authors also acknowledge the support of the National SuperComputer Center in Tianjin and Beijing PARATERA Tech Corp.,Ltd.,for providing HPC resources that have contributed to the research results reported in this paper.This work was partly supported by National Natural Science Fundation of China(Nos.12375215 and 12475210).
文摘ENN He Long-2(EHL-2)is the next-generation large mega-Ampere(MA)spherical torus(ST)proposed and funded by the ENN company.The design parameters are:Ti0>30 keV,n_(e0)~1×10^(20)m^(-3),Ip~3 MA,Bt~3 T.One of the biggest challenges of EHL-2 is how to achieve several MA current flat-tops with limited voltage-seconds(Vs)of the center solenoid(CS)coils.In order to minimize the consumption of Vs,a fully non-inductive start-up by electron cyclotron resonance heating(ECRH)will be applied in EHL-2.The ramp-up phase will be accomplished with the synergetic mode between the CS and non-inductive methods.The strategy of non-inductive start-up and ramp-up with synergetic mode has been verified on EXL-50U’s experiments.Based on this strategy,numerical simulations indicate the feasibility of EHL-2 achieving 3 MA plasma current.A high-performance steady-state scenario with Ip~1.5 MA is also designed.In this scenario,the bootstrap current fraction fBS>70%,the safety factor q at the magnetic axis q0>2,the minimum safety factor qmin>1,the poloidal betaβp>3 and normalized betaβN>2.3.Each design iteration integrates the validation of physical models with the constraints of engineering implementation,gradually optimizing the performance of the heating and current drive(H&CD)systems.Numerical simulation results for general auxiliary H&CD systems such as neutral beam injection(NBI),electron cyclotron(EC)wave,ion cyclotron wave(ICW),and lower hybrid wave(LHW)are presented.These simulation results ensure that the 31 MW H&CD systems comprehensively cover all scenarios while maintaining engineering feasibility.
基金supported by the National Key R&D Program of China(grant No.2024YFA1611600)the SVOM project(a mission under the Strategic Priority Program on Space Science of the Chinese Academy of Sciences)+23 种基金the Strategic Priority Research Program of the Chinese Academy of Sciences(grant No.XDB0550401)the National Natural Science Foundation of China(NSFC,grant No.12494573)partly supported by Natural Science Foundation of Xinjiang Uygur Autonomous Region(grant No.2024D01D32)Tianshan Talent Training Program(grant No.2023TSYCLJ0053)Tianshan Innovation Team Program(grant No.2024D14015)supported by the Jiangsu Funding Program for Excellent Postdoctoral Talent(grant No.2024ZB110)the Postdoctoral Fellowship Program(grant No.GZC20241916)the General Fund(grant No.2024M763531)of the China Postdoctoral Science Foundationsupported by a Royal Society Dorothy Hodgkin Fellowship(grant Nos.DHF-R1-221175 and DHF-ERE-221005)support by a postdoctoral fellowship from the CNESsupported by the National Key R&D Program of China(grant No.2024YFA1611702)the Strategic Priority Research Program of the Chinese Academy of Sciences(grant No.XDB0550101)the support of the French Agence Nationale de la Recherche(ANR),under grant ANR-23-CE31-0011(project PEGaSUS)financial support from the GRAWITA Large Program Grant(PI P.D’Avanzo)financial support from the Italian Space Agency,contract ASI/INAF No.I/004/11/6support from the INAF project Premiale Supporto Arizona&Italiasupported by the National Natural Science Foundation of China(NSFC,grant No.12133003)supported by the National Natural Science Foundation of China(NSFC,grant No.12373042)the Bagui Scholars Program(No.GXR-6BG2424001)funded by the European Union(ERC,HEAVYMETAL,101071865,Views and opinions expressed are,however,those of the authors only and do not necessarily reflect those of the European Union or the European Research Council Neither the European Union nor the granting authority can be held responsible for them)the Cosmic Dawn Center(DAWN)is funded by the Danish National Research Foundation under grant No.DNRF140supported by the National Natural Science Foundation of China(NSFC,grant Nos.12225305 and 12321003)supported by the National Natural Science Foundation of China(NSFC,grant No.12473049)supported by the General Fund(grant No.2024M763530)of the China Postdoctoral Science Foundation。
文摘Early multiwavelength observations offer crucial insights into the nature of the relativistic jets responsible for gamma-ray bursts and their interaction with the surrounding medium.We present data of GRB 240825A from 17 space-and ground-based telescopes/instruments,covering wavelengths from NIR/optical to X-ray and GeV,and spanning from the prompt emission to the afterglow phase triggered by Swift and Fermi.The early afterglow observations were carried out by SVOM/C-GFT,and spectroscopic observations of the afterglow by GTC,VLT,and TNG determined the redshift of the burst(z=0.659)later.A comprehensive analysis of the prompt emission spectrum observed by Swift-BAT and Fermi-GBM/LAT reveals a rare and significant high-energy cutoff at 76 MeV.Assuming this cutoff is due toγγabsorption allows us to place an upper limit on the initial Lorentz factor,Γ_(0)<245.The optical/NIR and GeV afterglow light curves can be described by the standard external shock model,with early-time emission dominated by a reverse shock(RS)and a subsequent transition to forward shock(FS)emission.Our afterglow modeling yields a consistent estimate of the initial Lorentz factor(Γ_(0)∼234).Furthermore,the RS-to-FS magnetic field ratio(R 302B)indicates that the RS region is significantly more magnetized than the FS region.An isotropic-equivalent kinetic energy of E_(k,iso)=5.25×10^(54) erg is derived,and the correspondingγ-ray radiation efficiency is estimated to beη_(γ)=3.1%.On the other hand,the standard afterglow model cannot reproduce the X-ray light curve of GRB 240825A,calling for improved models to characterize all multiwavelength data.
文摘局地微地形产生的微气象环境是造成气象预报误差的重要因素之一,也是导致覆冰预报准确性不高的主要原因。该研究利用高精度MODIS系统15 s(约500 m)地形数据驱动中尺度天气研究和预报(weather research and forecasting,WRF)模式,并使用基于决策树的梯度提升框架(light gradient boosting machine,LightGBM)对WRF预报进行订正,通过局地个例评估订正后的覆冰预测效果。结果表明:在假设条件下,过冷液滴覆冰速率随温度降低先快速增加,后增长速率保持不变,且液滴粒径越大,完全冻结所需温度越低;WRF-LightGBM订正算法在山区微地形下有效提升了温度预报准确度,典型冬季寒潮条件下预测温度与实际温度的误差在2℃以内,预报准确率为76%;以典型区域杆塔覆冰为例,输入订正后的温度和相对湿度数据后,覆冰融化时段被消除,覆冰厚度曲线与实际基本一致,增长速率接近一致。
