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| 1 | Origin, Evolution, and Genotyping of Emergent Porcine Epidemic Diarrhea Virus Strains in the United States显示文摘 | Yao-Wei Huang Allan W. Dickerman Pablo Pi?eyro Long Li Li Fang Ross Kiehne Tanja Opriessnig Xiang-Jin Meng | 2013 | mBio2013，，5： | 2 |
| 2 | Effect of narrow-band UVB phototherapy on soluble cell adhesion molecules in patients with psoriasis vulgaris显示文摘 | Long J Tao J Pi X | 2010 | J Int Med Res2010，38，1： | 1 |
| 3 | A microstructure-based analysis of cyclic plasticity of pearlitic steels with Hill's self-consistent scheme incorporating general anisotropic Eshelby tensor显示文摘pearlitic 钢与随机的取向由众多的 pearlitic 殖民地组成,并且每个殖民地由铁酸盐和渗碳体的许多平行薄片组成。这种材料的组成的行为可以包含两固有的 anisotropy,塑料变丑导致 anisotropy。对为这种双阶段的材料的周期的粘性的描述被一个基于微观结构的组成的模型的使用为一个 pearlitic 殖民地,和山为椭圆体的包括合并各向异性的 Eshelby 张肌的前後一致的计划建议。相应数字算法被开发。pearlitic 钢 BS11 和单相的冷抽的铜的回答使遭到了到一相称性地周期的装载被分析。分析结果与试验性的同意很好。与用各向同性的 Eshelby 张肌的结果相比,各向同性的近似能以一个简单得多的方法提供可接受的全面回答,这被显示出。 | Xuesong Long Xianghe Peng Wenli Pi | 2008 | Acta Mechanica Sinica2008，24，1： | 1 |
| 4 | Cost Optimization of Internal Grinding显示文摘 | Vu Ngoc Pi Le Xuan Hung Luu Anh Tung Banh Tien Long | 2016 | 材料科学与工程(中英文B版)2016，6，6： | 1 |
| 5 | Profit Optimization of External Cylindrical Grinding显示文摘 | Vu Ngoc Pi Banh Tien Long Vu Hong Khiem Nguyen Hong Quan | 2014 | Journal of Environmental Science and Engineering(B)2014，3，5： | 0 |
| 6 | Virulence of Salmonella enterica Serovar Enteritidis Isolate LN-248-0 and Immune Responses in BALB/c Mice显示文摘Salmonella enterica serovar Enteritidis(S.Enteritidis)is a major etiological agent of acute gastroenteritis in humans;the mode of infection being consumption of undercooked or improperly handled poultry meat or contaminated eggs or milk[1,2].Among more than 2,600 serotypes of Salmonella,S.Enteritidis frequently causes Salmonella infections in humans[3]. | LIU Yang LI You Zhi FENG Tao GONG Pi Qian JIN Ying Cai ZHU Hong Wei JIANG Lin Lin ZHANG Jian Long CHEN Guo Zhong YU Xin ZHANG Xing Xiao | 2020 | Biomedical and Environmental Sciences2020，33，8： | 0 |
| 7 | Cost Optimization of Surface Grinding Process显示文摘 | Vu Ngoc Pi Luu Anh Tung Le Xuan Hung Banh Tien Long | 2016 | Journal of Environmental Science and Engineering(A)2016，5，12： | 0 |
| 8 | Properties of Flare Events on M Stars from LAMOST Spectral Survey Based on Kepler and TESS Light Curves显示文摘A catalog of M stars has been published from the Large Sky Area Multi-Object Fiber Spectroscopic Telescope data release 7(LAMOST DR7).We cross-matched the LAMOST M catalog with Kepler,Kepler 2(K2)and Transiting Exoplanet Survey Satellite(TESS)surveys.We obtained the light curves from the Kepler and TESS surveys.We detected 20,047 flare events from 4053 M stars and calculated their durations,amplitudes,and energies.We analyzed the distribution of the flare durations and energies.The distributions of flare duration for Kepler,K2 and TESS peak are at 3–3.5 hr,4–6 hr and 1–1.5 hr,respectively.This may be the result of the different cadences for the three data sets.The highest regions of the flare energies of Kepler,K2 and TESS are 32–32.5,32–32.5 and31–31.5 erg in Log format,respectively.A linear relationship between flare duration and energy emerges from our analysis.The ratio of flare duration to total observational time is approximately 0.2%–0.3%for the Kepler,K2 and TESS surveys.The occurrence rate of a star with a flare event increases from the M0 to M4 subtypes.We also determined the spatial distribution of the flare rate of M stars in the Milky Way.It seems that the flare rate decreases as the vertical height increases.The power index of the flare energies is in the region of 1.53–2.32,which is similar to previous result for solar type star(2.0).Further,we examined the relationship between the flare amplitude and chromospheric intensity.The flare activity increases rapidly with the increase in the HαEW at the lower values(less approximately 2?)and it increases slowly at the higher values. | Gang Meng Li-Yun Zhang Tianhao Su Zilu Yang Xianming LHan Prabhakar Misra Liu Long Qingfeng Pi Zhongzhong Zhu Linyan Jiang | 2023 | Research in Astronomy and Astrophysics2023，23，5： | 0 |
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