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The Interpretation of "Ju Men","Wen Qu" from Kun Ren yi of Qing nang Ao Yu-Also Discuss on the Cognition of the Study of Traditional Feng Shui

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Journal of Literature and Art Studies 2019年第6期9卷 654-659页

作者： Liu yi Zhang Yan Shanghai Institute of Visual Art Shanghai Academy of Social Sciences

There are three different opinions of the first sentence from Qin nang Ao Yu (青囊奥语), which was written by Yang Jun-song (杨筠松). They are “Kun Ren yi (坤壬乙) should start from the star Ju Men (巨门)”;“Kun Ren yi should start from the star Wen Qu (文曲)” and “Kun Ren yi should start from both the star Lian Zhen and the star Ju Men (Lian Ju (廉巨))”. Because of the sectarianism,though the people were at odds with the opinions, we cannot find out any comprehensive and objective study on these. According to the analysis of some relevant literatures, it can be seen that there are two viewpoints nowadays. One of the viewpoints deemed that the first sentence was falsified by Jiang Da-hong (蒋大鸿), and another one deemed that was falsified by Zhang Shou-qi (张受祺). But neither of the view was credible. More precisely is that “Wen Qu” and “Ju Men” were both found in the publications simultaneously, and there were more “Wen Qu”, during the period of the end of the Ming Dynasty and the era of the emperors Kangxi and Qianlong of the Qing Dynasty. The influence of “Ju Meg” was gradually spread when Jiang Da-hong used it in his book and also Si Ku Quan Shu (四库全书) cited it, then let to more pithy formulas of “Ju Men” to be used now. And the “Lian Ju” was rare to be used except Duan Mu Guo-hu (端木国瑚) who used to use it. The way of interpretation is so multiple and complex on the “Wen Qu” and “Ju Men” from the Qin nang Ao Yu, according to the perspective of Feng Shui, which is reflecting the pluralism and uncertainty of the interpretation of the traditional Feng Shui. And it is still need to be required a further more careful consideration on how to treat the studies of the traditional Feng Shui for the nowadays scholars.

关键词： Qin nang Ao Yu Ju Men Wen Qu

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加强合作共赢未来——第24届中国机床工具行业发展论坛暨2012年运营形势研讨会现场报道

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制造技术与机床 2012年第1期 13-14页

作者：汪艺《制造技术与机床》编辑部

2011年12月6—9日，中国机械工业集团有限公司中国机床总公司主办，北京国机展览中心、广州数控设备有限公司等协办的第24届中国机床工具行业发展论坛（MTDF）暨2012年运营形式研讨会在广州召开。

关键词：机床工具行业中国运营论坛合作机械工业展览中心数控设备

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Localization Method for the Pointing Observation with the Collimated Telescopes of Insight-HXMT

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Research in Astronomy and Astrophysics 2023年第5期23卷 38-43页

作者： Qi Luo Jin-Yuan Liao yi nang Cheng-Kui Li Chen Wang Na Sai Ju Guan Yu-Peng Chen Cheng-Cheng Guo Yuan Liu Shu Zhang Shuang-Nan Zhang Key Laboratory of Particle Astrophysics Institute of High Energy PhysicsChinese Academy of SciencesBeijing 100049China University of Chinese Academy of Sciences Beijing 100049China Key Laboratory of Space Astronomy and Technology National Astronomical ObservatoriesChinese Academy of SciencesBeijing 100101China School of Physics and Technology Wuhan UniversityWuhan 430072China WHU-NAOC Joint Center for Astronomy Wuhan UniversityWuhan 430072China

An accurate target source position is sometimes useful for the pointing observation with the collimated telescopes of the Hard X-ray Modulation Telescope(Insight-HXMT),which is determined by the reliability of the instrumental ***-HXMT has the unique design that all three main payloads(LE,ME and HE)consist of detector groups with three fields of views(FOVs)whose orientations differ by 60°.As the point-spread functions are different at different positions in the FOV coordinates,the count rate ratios between the detector groups depend on the position of an X-ray source in the *** on the multi-FOV design,we develop a localization method for an X-ray source in the pointing observation of *** accuracy of the method is investigated with the pointing observations of the Crab with different *** find that the statistical error decreases with the exposure,and the systematic error is dominant for the exposure>128 *** the exposure of1024 s,the total error is 0°.015 for the *** method can effectively distinguish the Rapid Burster H 1730–333and Slow Burster GX 354–0,which are only 0°.5 apart and can both contribute to bursts in the light curve obtained by *** also apply the pointing observation localization method to locate the X-ray counterpart of FRB 200428 with high *** located position is consistent with SGR J1935+2154 within 1σuncertainty of 10′,which provides important evidence that fast radio bursts can originate from magnetars.

关键词： instrumentation detectors-space vehicles instruments-telescopes

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基于Blast-GO的蛋白质亚线粒体定位预测

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生物化学与生物物理进展 2015年第12期42卷 1136-1143页

作者：曩毅梅含雪赵燕侯宝妍赵志远樊国梁内蒙古大学物理科学与技术学院呼和浩特010021

本文建立了一个最新的蛋白质亚线粒体定位数据集,包含4个亚线粒体定位的1 293条序列,结合基因本体(GO)信息和同源信息对线粒体蛋白质进行特征提取,利用支持向量机算法建立分类器,经Jackknife检验,对于4个亚线粒体位置的总体预测准确率为... 详细信息

本文建立了一个最新的蛋白质亚线粒体定位数据集,包含4个亚线粒体定位的1 293条序列,结合基因本体(GO)信息和同源信息对线粒体蛋白质进行特征提取,利用支持向量机算法建立分类器,经Jackknife检验,对于4个亚线粒体位置的总体预测准确率为93.27%,其中3个亚线粒体位置的总体预测准确率为94.73%.

关键词：亚线粒体定位基因本体同源信息支持向量机

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土坝回填粘土渗透变形特性试验研究

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金华职业技术学院学报 2007年第4期7卷 14-18,89页

作者：杜宁陈兰云李宪辉易南概金华职业技术学院浙江金华321007 沈阳建筑大学土木工程学院辽宁沈阳110168

土石坝的除险加固方案中常采用冲抓套井回填夯实粘土作为防渗体,即粘土心墙防渗体,该方法已在许多水库和相当长度的堤防工程建设中得到广泛的应用;然而其渗透稳定一直是工程设计和施工中的关键问题之一。本文结合某水库土石坝除险加固... 详细信息

土石坝的除险加固方案中常采用冲抓套井回填夯实粘土作为防渗体,即粘土心墙防渗体,该方法已在许多水库和相当长度的堤防工程建设中得到广泛的应用;然而其渗透稳定一直是工程设计和施工中的关键问题之一。本文结合某水库土石坝除险加固工程坝体渗透稳定问题,开展了坝体心墙粘土的物理特性、渗透特性、临界坡降的研究,为工程设计和施工提供了必要的分析成果和参考依据。

关键词：土石坝粘土渗透破坏临界水力梯度

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Timing analysis of the black hole candidate EXO 1846–031 with Insight-HXMT monitoring

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Research in Astronomy and Astrophysics 2021年第3期21卷 193-204页

作者： He-Xin Liu Yue Huang Guang-Cheng Xiao Qing-Cui Bu Jin-Lu Qu Shu Zhang Shuang-Nan Zhang Shu-Mei Jia Fang-Jun Lu Xiang Ma Lian Tao Wei Zhang Li Chen Li-Ming Song Ti-Pei Li Yu-Peng Xu Xue-Lei Cao Yong Chen Cong-Zhan Liu Ce Cai Zhi Chang Gang Chen Tian-Xiang Chen yi-Bao Chen Yu-Peng Chen Wei Cui Wei-Wei Cui Jing-Kang Deng Yong-Wei Dong Yuan-Yuan Du Min-Xue Fu Guan-Hua Gao He Gao Min Gao Ming-Yu Ge Yu-Dong Gu Ju Guan Cheng-Cheng Guo Da-Wei Han Jia Huo Lu-Hua Jiang Wei-Chun Jiang Jing Jin Yong-Jie Jin Ling-Da Kong Bing Li Cheng-Kui Li Gang Li Mao-Shun Li Wei Li Xian Li Xiao-Bo Li Xu-Fang Li Yang-Guo Li Zheng-Wei Li Xiao-Hua Liang Jing-Yuan Liao Bai-Sheng Liu Guo-Qing Liu Hong-Wei Liu Xiao-Jing Liu yi-Nong Liu Bo Lu Xue-Feng Lu Qi Luo Tao Luo Bin Meng yi nang Jian-yin Nie Ge Ou Na Sai Ren-Cheng Shang Xin-ying Song Liang Sun ying Tan You-Li Tuo Chen Wang Guo-Feng Wang Juan Wang Ling-Jun Wang Weng-Shuai Wang Yu-Sa Wang Xiang-Yang Wen Bai-Yang Wu Bo-Bing Wu Mei Wu Shuo Xiao Shao-Lin Xiong He Xu Jia-Wei Yang Sheng Yang Yan-Ji Yang yi-Jung Yang Qi-Bin yi Qian-Qing yin Yuan You Ai-Mei Zhang Cheng-Mo Zhang Fan Zhang Hong-Mei Zhang Juan Zhang Tong Zhang Wan-Chang Zhang Wen-Zhao Zhang yi Zhang yi-Fei Zhang Yong-Jie Zhang Yuan-Hang Zhang Yue Zhang Zhao Zhang Zhi Zhang Zi-Liang Zhang Hai-Sheng Zhao Xiao-Fan Zhao Shi-Jie Zheng Yao-Guang Zheng Deng-Ke Zhou Jian-Feng Zhou Yu-Xuan Zhu Ren-Lin Zhuang Yue Zhu Key Laboratory of Particle Astrophysics Institute of High Energy PhysicsChinese Academy of SciencesBeijing 100049China University of Chinese Academy of Sciences Chinese Academy of SciencesBeijing 100049China Institut fur Astronomie und Astrophysik Kepler Center for Astro and Particle PhysicsEberhard Karls Universität72076 TubingenGermany Department of Astronomy Beijing Normal UniversityBeijing 100088China Department of Astronomy Tsinghua UniversityBeijing 100084China Department of Physics Tsinghua UniversityBeijing 100084China Department of Engineering Physics Tsinghua UniversityBeijing 100084China Key Laboratory of Space Astronomy and Technology National Astronomical ObservatoriesChinese Academy of SciencesBeijing 100101China College of Physics Sciences&Technology Hebei UniversityBaoding 071002Hebei ProvinceChina

We present the observational results from a detailed timing analysis of the black hole candidate EXO 1846-031 during its outburst in 2019 with the observations of Insight-HXMT,NICER and *** outburst can be classified roughly into four different ***-C quasi-periodic oscillations(QPOs)observed by NICER(about 0.1-6 Hz)and Insight-HXMT(about 0.7-8 Hz)are also reported in this ***,we study various physical quantities related to QPO *** QPO rms-frequency relationship in the energy band 1-10 keV indicates that there is a turning pointing in frequency around2 Hz,which is similar to that of GRS 1915+105.A possible hypothesis for the relationship above may be related to the inclination of the source,which may require a high inclination to explain *** relationships between QPO frequency and QPO rms,hardness,total fractional rms and count rate have also been found in other transient sources,which can indicate that the origin of type-C QPOs is non-thermal.

关键词： X-ray binaries black hole candidate QPO EXO 1846–031

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Overview to the Hard X-ray Modulation Telescope (Insight-HXMT) Satellite

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Science China(Physics,Mechanics & Astronomy) 2020年第4期63卷 2-19页

作者： Shuang-Nan Zhang TiPei Li FangJun Lu LiMing Song YuPeng X u CongZhan Liu Yong Chen XueLei Cao QingCui Bu Zhi Chang Gang Chen Li Chen TianXiang Chen yiBao Chen YuPeng Chen Wei Cui WeiWei Cui JingKang Deng YongWei Dong Yuan Yuan Du MinXue Fu GuanHua Gao He Gao Min Gao MingYu Ge YuDong Gu Ju Guan Can Gungor ChengCheng Guo DaWei Han Wei Hu Yue Huang Jia Huo ShuMei Jia LuHua Jiang WeiChun Jiang Jing Jin YongJie Jin Bing Li ChengKui Li Gang Li MaoShun Li Wei Li Xian Li XiaoBo Li XuFang Li YanGuo Li ZiJian Li ZhengWei Li XiaoHua Liang JinYuan Liao GuoQing Liu HongWei Liu ShaoZhen Liu XiaoJing Liu Yuan Liu yiNong Liu Bo Lu XueFeng Lu Tao Luo Xiang Ma Bin Meng yi nang Jianyin Nie Ge Ou JinLu Qu Na Sai RenCheng Shang GuoHong Shen Liang Sun ying Tan Lian Tao YouLi Tuo Chen Wang ChunQin Wang GuoFeng Wang HuanYu Wang Juan Wang WenShuai Wang YuSa Wang XiangYang Wen BaiYang Wu BoBing Wu Mei Wu GuangCheng Xiao ShaoLin Xiong LinLi Yan JiaWei Yang Sheng Yang YanJi Yang QiBin yi Bin Yuan AiMei Zhang ChunLei Zhang ChengMo Zhang Fan Zhang HongMei Zhang Juan Zhang Qiang Zhang Shenyi Zhangs Shu Zhang Tong Zhang WanChang Zhang Wei Zhang WenZhao Zhang yi Zhang yiFei Zhang YongJie Zhang Yue Zhang Zhao Zhang Zhi Zhang ZiLiang Zhang HaiSheng Zhao XiaoFan Zhao ShiJie Zheng JianFeng Zhou YuXuan Zhu Yue Zhu RenLin Zhuang Key Laboratory of Particle Astrophysics Institute of High Energy PhysicsChinese Academy of SciencesBeijing 100049China University of Chinese Academy of Sciences Beijing 100049China Department of Astronomy Tsinghua UniversityBeijing 100084China Department of Physics Tsinghua UniversityBeijing 100084China Department of Astronomy Beijing Normal UniversityBeijing 100088China Department of Engineering Physics Tsinghua UniversityBeijing 100084China National Astronomical Observatories Chinese Academy of SciencesBeijing 100101China National Space Science Center Chinese Academy of SciencesBeijing 100190China

As China’s first X-ray astronomical satellite, the Hard X-ray Modulation Telescope (HXMT), which was dubbed as Insight-HXMT after the launch on June 15, 2017, is a wide-band(1-250 ke V) slat-collimator-based X-ray astronomy satellite with the capability of all-sky monitoring in 0.2-3 Me V. It was designed to perform pointing, scanning and gamma-ray burst(GRB)observations and, based on the Direct Demodulation Method (DDM), the image of the scanned sky region can be *** we give an overview of the mission and its progresses, including payload, core sciences, ground calibration/facility, ground segment, data archive, software, in-orbit performance, calibration, background model, observations and some preliminary results.

关键词： X-and γ-ray telescopes and instrumentation neutron stars black holes X-ray binaries γ-ray bursts

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Insight-HXMT observations of the first binary neutron star merger GW170817

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Science China(Physics,Mechanics & Astronomy) 2018年第3期61卷 26-33页

作者： TiPei Li ShaoLin Xiong ShuangNan Zhang FangJun Lu LiMing Song XueLei Cao Zhi Chang Gang Chen Li Chen TianXiang Chen Yong Chen yiBao Chen YuPeng Chen Wei Cui WeiWei Cui JingKang Deng YongWei Dong YuanYuan Du MinXue Fu GuanHua Gao He Gao Min Gao MingYu Ge YuDong Gu Ju Guan ChengCheng Guo DaWei Han Wei Hu Yue Huang Jia Huo ShuMei Jia LuHua Jiang WeiChun Jiang Jing Jin YongJie Jin Bing Li ChengKui Li Gang Li MaoShun Li Wei Li Xian Li XiaoBo Li XuFang Li YanGuo Li ZiJian Li ZhengWei Li XiaoHua Liang JinYuan Liao CongZhan Liu GuoQing Liu HongWei Liu ShaoZhen Liu XiaoJing Liu Yuan Liu yiNong Liu Bo Lu XueFeng Lu Tao Luo Xiang Ma Bin Meng yi nang Jianyin Nie Ge OU JinLu Qu Na Sai Liang Sun yin Tan Lian Tao WenHui Tao YouLi Tuo GuoFeng Wang HuanYu Wang Juan Wang WenShuai Wang YuSa Wang XiangYang Wen BoBing WU Mei Wu GuangCheng Xiao He Xu YuPeng Xu LinLi Yan JiaWei Yang Sheng Yang YanJi Yang AiMei Zhang ChunLei Zhang ChengMo Zhang Fan Zhang HongMei Zhang Juan Zhang Qiang Zhang Shu Zhang Tong Zhang Wei Zhang WanChang Zhang WenZhao Zhang yi Zhang Yue Zhang yiFei Zhang YongJie Zhang Zhao Zhang ZiLiang Zhang HaiSheng Zhao JianLing Zhao XiaoFan Zhao ShiJie Zheng Yue Zhu YuXuan Zhu ChangLin Zou Key Laboratory of Particle Astrophysics Institute of High Energy Physics Chinese Academy of Sciences Beijing 100049 China Department of Physics Tsinghua University Beijing 100084 China University of Chinese Academy of Sciences Chinese Academy of Sciences Beijing 100049 China Department of Astronomy Beijing Normal University Beijing 100088 China Department of Engineering Physics Tsinghua University Beijing 100084 China

Finding the electromagnetic （EM） counterpart of binary compact star merger, especially the binary neutron star （BNS） merger, is critically important for gravitational wave （GW） astronomy, cosmology and fundamental physics. On Aug. 17, 2017, Advanced LIGO and Fermi/GBM independently triggered the first BNS merger, GW170817, and its high energy EM counterpart, GRB 170817A, respectively, resulting in a global observation campaign covering gamma-ray, X-ray, UV, optical, IR, radio as well as neutrinos. The High Energy X-ray telescope （HE） onboard Insight-HXMT （Hard X-ray Modulation Telescope） is the unique high-energy gamma-ray telescope that monitored the entire GW localization area and especially the optical counterpart （SSS17a/AT2017gfo） with very large collection area （M000 cm2） and microsecond time resolution in 0.2-5 MeV. In addition, Insight-HXMT quickly implemented a Target of Opportunity （TOO） observation to scan the GW localization area for potential X-ray emission from the GW source. Although Insight-HXMT did not detect any significant high energy （0.2-5 MeV） radiation from GW170817, its observation helped to confirm the unexpected weak and soft nature of GRB 170817A. Meanwhile, Insight-HXMT/HE provides one of the most stringent constraints （-10-7 to 104 erg/cm2/s） for both GRB170817A and any other possible precursor or extended emissions in 0.2-5 MeV, which help us to better understand the properties of EM radiation from this BNS merger. Therefore the observation of Insight-HXMT constitutes an important chapter in the full context of multi-wavelength and multi-messenger observation of this historical GW event.

关键词： GW170817 BNS merger gravitational wave electromagnetic counterpart

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Effect of the Vacuolation of Helicobacter Pylori

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Journal of Huazhong University of Science and Technology(Medical Sciences) 2001年第2期21卷 97-99页

作者：施理候晓华易粹琼张锦坤 Digestive Disease Institute of PLA Nang Fang Hospital Guangzhou 510515

Cytotoxic test in vitro combined with cytochemical stain, fluorescent stain, transmission electronmicrograph was used to study the vacuolated effect by helicobacter pylori (***) (Toxin+) and its pathological mechanism. 78..26 % patients with peptic ulcer associated with *** was infected with *** (Toxin+), while 42.86 % patients with gastritis was infected with *** (Toxin+). It was positive in vacuole with acridine orange and acid phosphatase stain. Transmission electronmicrograph of vacuole revealed the presence of abounding membrane. There was a closed relationship between infection with *** (Toxin+) and peptic ulcer disease. The vacuole induced by *** (Toxin+) was autophagosome, which was pathological phenomenon induced by toxin.

关键词： helicobacter pylori vacuolation autophagosome

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Modeling of automobile air conditioning systems

Modeling of automobile air conditioning systems

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2009中国控制与决策会议

作者： Chung-Lun Li Shung-Luen Chung Jing-nang Lee Department of Electrical Engineering National Taiwan University of Science and TechnologyTaiwan Department of Refrigeration Air Conditioning and Energy EngineeringNational Chin-Yi University of TechnologyTaiwan

＜正＞This paper studies the dynamics of temperature and humidity of air in a car compartment by the concept of enthalpy in analyzing the heat exchange *** heat change decomposed into sensible heat and latent heat,we are able to derive dynamics of temperature and humidity of the car compartment after taking into account of the difference of ASHF（apparatus sensible heat factor） and RSHF（room sensible heat factor）.These two formulas are used in conjunction with two control strategies on flow rates of supply air to simulate the intended controlled car compartment at constant enthalpy and of constant *** contribution of this work is to provide a framework for automobile air-conditioning analysis and simulation.

关键词： automobile air-conditioning enthalpy HVAC

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