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中国员工工作价值观的代际变迁

心理学报 2024年第7期56卷 876-894,I0001-I0003页

作者：唐宁玉甄丹蕾关健上海交通大学安泰经济与管理学院上海200030

随着时代发展,我国工作场所中的员工队伍构成呈现出多样化趋势。多代际并存,使得理解不同代际员工的工作价值观变得迫切而重要。本文基于Inglehart的现代化演进理论,通过采用不同研究设计、不同测量工具、不同分析方法和不同研究视角的... 详细信息

随着时代发展,我国工作场所中的员工队伍构成呈现出多样化趋势。多代际并存,使得理解不同代际员工的工作价值观变得迫切而重要。本文基于Inglehart的现代化演进理论,通过采用不同研究设计、不同测量工具、不同分析方法和不同研究视角的三个研究,对不同代际(改革前一代、改革一代和后改革一代)员工工作价值观的变迁展开了系统而深入的分析。研究结果显示,我国不同代际员工的工作价值观既存在差异,又存在相似之处,后改革一代的工作价值观较之其他两代差异最为明显。具体而言,相比于改革前一代与改革一代,后改革一代的物质主义工作价值观最低,后物质主义工作价值观最高;后改革一代相比于前两个代际对开放工作价值观的重视程度最高,但三代员工在自我超越工作价值观上没有显著差异。研究还发现,不同代际员工对物质主义工作价值观的重视程度仍然高于后物质主义。本研究丰富了工作价值观代际差异以及新生代员工研究的知识体系,研究结果也可以为处在大变局中的企业管理实践提供借鉴和参考。

关键词：工作价值观代际差异物质主义后物质主义开放-保守自我增强-自我超越 APC分析方法

HiFAST:An HIdata calibration and imaging pipeline for FAST

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Science China(Physics,Mechanics & Astronomy) 2024年第5期67卷 182-199页

作者： Yingjie Jing Jie Wang Chen Xu Ziming Liu Qingze Chen Tiantian Liang Jinlong Xu Yixian Cao Jing Wang Huijie Hu Chuan-Peng Zhang Qi Guo Liang Gao Mei Ai Hengqian Gan Xuyang Gao Jinlin Han Ligang Hou Zhipeng Hou Peng Jiang Xu Kong Fujia Li Zerui Liu Li Shao Hengxing Pan Jun Pan Lei Qian Jinghai Sun ningyu tang Qingliang Yang Bo Zhang Zhiyu Zhang Ming Zhu National Astronomical Observatories Chinese Academy of SciencesBeijing 100012China Institute for Frontiers in Astronomy and Astrophysics Beijing Normal UniversityBeijing 02206China School of Astronomy and Space Science University of Chinese Academy of SciencesBeijing 100049China Guizhou Radio Astronomical Observatory Guizhou UniversityGuiyang 55000China Max Planck Institute for Extraterrestrial Physics Garching 85748Germany Kavli Institute for Astronomy and Astrophysics Peking UniversityBeijing 100871China Institute of Computational Cosmology Department of PhysicsUniversity of DurhamDurham DHI 3LEUK CAS Key Laboratory of FAST National Astronomical ObservatoriesChinese Academy of SciencesBeijing 100101China Deep Space Exploration Laboratory/Department of Astronomy University of Science and Technology of ChinaHefei 230026China School of Astronomy and Space Science University of Science and Technology of ChinaHefei 230026China Astrophysics Department of PhysicsUniversity of OxfordOxford OX/3RHUK College of Earth Sciences Guilin University of TechnologyGuilin 541004China Department of Physics Anhui Normal UniversityWuhu 241002China School of Astronomy and Space Science Nanjing UniversityNanjing 210023China Key Laboratory of Modern Astronomy and Astrophysics Nanjing UniversityNanjing 20023China

The Five-hundred-meter Aperture Spherical radio Telescope(FAST)has the largest aperture and a 19-beam L-band receiver,making it powerful for investigating the neutral hydrogen atomic gas(HI)in the *** present HiFAST(https://***),a dedicated,modular,and self-contained calibration and imaging pipeline for processing the H?data of *** pipeline consists of frequency-dependent noise diode calibration,baseline fitting,standing wave removal using an FFT-based method,flux density calibration,stray radiation correction,and gridding to produce data *** modules can be combined as needed to process the data from most FAST observation modes:tracking,drift scanning,On-The-Fly mapping,and most of their *** HiFAST,the root-mean-square(RMS)noises of the calibrated spectra from all 19 beams were only slightly(~5%)higher than the theoretical *** results for the extended source M33 and the point sources are consistent with the results from *** moment maps(0,1 and 2)of M33 agree well with the results from the Arecibo Galaxy Environment Survey(AGES)with a fractional difference of less than 10%.For a common sample of 221 sources with signal-to-noise ratio S/N>10 from the Arecibo Legacy Fast ALFA(ALFALFA)survey,the mean value of fractional difference in the integrated flux density,Sint,between the two datasets is approximately 0.005%,with a dispersion of 15.4%.Further checks on the integrated flux density of 23 sources with seven observations indicate that the variance in the flux density of the source with luminous objects(Sint>2.5 Jy km s-1)is less than 5%.Our tests suggest that the FAST telescope,with the efficient,precise,and user-friendly pipeline HiFAST,will yield numerous significant scientific findings in the investigation of the H?in the universe.

关键词： fractional luminous correction

HiFAST:An H?data calibration and imaging pipeline for FAST

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Science China(Physics,Mechanics & Astronomy) 2024年第5期Mechanics & Astronomy) .卷 186-203页

作者： Yingjie Jing Jie Wang Chen Xu Ziming Liu Qingze Chen Tiantian Liang Jinlong Xu Yixian Cao Jing Wang Huijie Hu Chuan-Peng Zhang Qi Guo Liang Gao Mei Ai Hengqian Gan Xuyang Gao Jinlin Han Ligang Hou Zhipeng Hou Peng Jiang Xu Kong Fujia Li Zerui Liu Li Shao Hengxing Pan Jun Pan Lei Qian Jinghai Sun ningyu tang Qingliang Yang Bo Zhang Zhiyu Zhang Ming Zhu National Astronomical Observatories Chinese Academy of Sciences Institute for Frontiers in Astronomy and Astrophysics Beijing Normal University School of Astronomy and Space Science University of Chinese Academy of Sciences Guizhou Radio Astronomical Observatory Guizhou University Max Planck Institute for Extraterrestrial Physics Kavli Institute for Astronomy and Astrophysics Peking University Institute of Computational Cosmology Department of PhysicsUniversity of Durham CAS Key Laboratory of FAST National Astronomical ObservatoriesChinese Academy of Sciences Deep Space Exploration Laboratory/Department of Astronomy University of Science and Technology of China School of Astronomy and Space Science University of Science and Technology of China Astrophysics Department of PhysicsUniversity of Oxford College of Earth Sciences Guilin University of Technology Department of Physics Anhui Normal University School of Astronomy and Space Science Nanjing University Key Laboratory of Modern Astronomy and Astrophysics Nanjing University

The Five-hundred-meter Aperture Spherical radio Telescope（FAST） has the largest aperture and a 19-beam L-band receiver,making it powerful for investigating the neutral hydrogen atomic gas（H?） in the *** present HiFAST（https://***）,a dedicated,modular,and self-contained calibration and imaging pipeline for processing the H?data of *** pipeline consists of frequency-dependent noise diode calibration,baseline fitting,standing wave removal using an FFT-based method,flux density calibration,stray radiation correction,and gridding to produce data *** modules can be combined as needed to process the data from most FAST observation modes:tracking,drift scanning,On-The-Fly mapping,and most of their *** HiFAST,the root-mean-square（RMS） noises of the calibrated spectra from all 19 beams were only slightly（～5%） higher than the theoretical *** results for the extended source M33 and the point sources are consistent with the results from *** moment maps（0,1 and 2） of M33 agree well with the results from the Arecibo Galaxy Environment Survey（AGES） with a fractional difference of less than 10%.For a common sample of 221 sources with signal-to-noise ratio S/N>10 from the Arecibo Legacy Fast ALFA（ALFALFA） survey,the mean value of fractional difference in the integrated flux density,Sint,between the two datasets is approximately 0.005%,with a dispersion of 15.4%.Further checks on the integrated flux density of 23 sources with seven observations indicate that the variance in the flux density of the source with luminous objects(Sint>2.5 Jy km s-1) is less than 5%.Our tests suggest that the FAST telescope,with the efficient,precise,and user-friendly pipeline HiFAST,will yield numerous significant scientific findings in the investigation of the H? in the universe.

关键词：

The Distribution of UV Radiation Field in the Molecular Clouds of Gould Belt

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Research in Astronomy and Astrophysics 2022年第8期22卷 206-217页

作者： Jifeng Xia ningyu tang Qijun Zhi Sihan Jiao Jinjin Xie Gary A.Fuller Paul F.Goldsmith Di Li School of Physics and Electronic Science Guizhou Normal UniversityGuiyang 550025China National Astronomical Observatories Chinese Academy of SciencesBeijing 100101China University of Chinese Academy of Sciences Beijing 100049China Department of Physics Anhui Normal UniversityWuhu 241002China Guizhou Provincial Key Laboratory of Radio Astronomy and Data Processing Guizhou Normal UniversityGuiyang 550001China Shanghai Astronomical Observatory CASShanghai 200030China Jodrell Bank Centre for Astrophysics Department of Physics&AstronomyThe University of ManchesterManchester M139PLUnited Kingdom I.Physikalisches Institut University of CologneZülpicher Str.77D-50937 KölnGermany Jet Propulsion Laboratory California Institute of Technology4800 Oak Grove DrivePasadenaCA 91109United States of America

The distribution of ultraviolet(UV)radiation field provides critical constraints on the physical environments of molecular *** 1 kpc of our solar system and fostering protostars of different masses,the giant molecular clouds in the Gould Belt present an excellent opportunity to resolve the UV field structure in star-forming *** performed spectral energy distribution(SED)fitting of the archival data from the Herschel Gould Belt Survey(HGBS).Dust radiative transfer analysis with the DUSTY code was applied to 23 regions in 14 molecular complexes of the Gould Belt,resulting in the spatial distribution of the radiation field in these *** 10 of 15 regions with independent measurements of star formation rate,their star formation rate and UV radiation intensity largely conform to a linear correlation found in previous studies.

关键词： ISM:clouds (ISM:)dust extinction radiative transfer

Commissioning progress of the FAST

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Science China(Physics,Mechanics & Astronomy) 2019年第5期62卷 3-24页

作者： Peng Jiang YouLing Yue HengQian Gan Rui Yao Hui Li GaoFeng Pan JingHai Sun DongJun Yu HongFei Liu ningyu tang Lei Qian JiGuang Lu Jun Yan Bo Peng ShuXin Zhang QiMing Wang Qi Li Di Li CAS Key Laboratory of FAST National Astronomical Observatories Chinese Academy of Sciences School of Astronomy and Space Science University of Chinese Academy of Sciences

The Five-hundred-meter Aperture Spherical radio Telescope(FAST) was completed with its main structure installed on September 25, 2016, after which it entered the commissioning phase. This paper aims to introduce the commissioning progress of the FAST over the past two years. To improve its operational reliability and ensure effective observation time, FAST has been equipped with a real-time information system for the active reflector system and hierarchical commissioning scheme for the feed support system, which ultimately achieves safe operation of the two systems. For meeting the high-performance indices, a highprecision measurement system was set up based on the effective control methods that were implemented for the active reflector system and feed support system. Since the commissioning of the FAST, a low-frequency ultra-wideband receiver and 19-beam1.05-1.45 GHz receiver have been mainly used. Telescope efficiency, pointing accuracy, and system noise temperature were completely tested and ultimately achieved the acceptance indices of the telescope. The FAST has been in the process of national acceptance preparations and has begun to search for pulsars. In the future, it will still strive to improve its capabilities and expand its application prospects.

关键词： radio telescopes and instrumentation astronomical observations radio wave receivers algorithms and implementation control systems

Status and perspectives of the CRAFTS extra-galactic HI survey

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Science China(Physics,Mechanics & Astronomy) 2019年第5期62卷 52-60页

作者： Kai Zhang JingWen Wu Di Li Marko Krco Lister Staveley-Smith ningyu tang Lei Qian MengTing Liu ChengJin Jin YouLing Yue Yan Zhu HongFei Liu DongJun Yu JingHai Sun GaoFeng Pan Hui Li HengQian Gan Rui Yao FAST Collaboration National Astronomical Observatories Chinese Academy of SicencesBeijing 100101China University of Chinese Academy of Sciences Beijing 100049China CAS Key Laboratory of FAST National Astronomical Obserx'atoriesChinese Academy of SciencesBeijing 100101China International Centre for Radio Astronomy Research (ICRAR) The University1 of Western AustraliaPerth 6907Australia ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D) The University of Western AustraliaPerth 6907Australia 不详

The Five-hundred-meter Aperture Spherical radio Telescope(FAST) is expected to complete its commissioning in 2019. FAST will soon begin the Commensal Radio Astronomy FasT Survey(CRAFTS), a novel and unprecedented commensal drift scan survey of the entire sky visible from FAST. The goal of CRAFTS is to cover more than 20000 deg2 and reach redshift up to about 0.35. We provide empirical measurements of the beam size and sensitivity of FAST across the 1.05 to 1.45 GHz frequency range of the FAST L-band array of 19-beams(FLAN). Using a simulated HI-galaxy catalogue based on the HI Mass Function(HIMF), we estimate the number of galaxies that CRAFTS may detect. At redshifts below 0.35, over 6 × 105 HI galaxies may be detected. Below the redshift of 0.07, the CRAFTS HIMF will be complete above a mass threshold of 109.5 M⊙. FAST will be able to investigate the environmental and redshift dependence of the HIMF to an unprecedented depth, shedding light onto the missing baryon and missing satellite problems.

关键词： HI regions and 21-cm lines radio telescopes and instrumentation statistical and correlative studies of properties

“极端天气”还是“气候改变”:对中国商学院本科教育的反思

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管理学报 2021年第11期18卷 1608-1611页

作者：唐宁玉上海交通大学安泰经济与管理学院海南大学管理学院

1缘起:两篇论文2020年第1期的AMLE期刊上发表了一篇BUNCH撰写的题为“Stateofundergraduatebusinesseducation:aperfectstorm orclimatechange”的论文(以下简称BUNCH论文),对商科本科教育的现状和存在问题进行了分析,认为许多大学生在评判性思考、复杂推理和书面沟通上并没有太大的提升,而这种不足在商学院学生中尤其明显,商学院毕业生存在着或准备不足或就业不足的情况。

关键词：极端天气就业不足商学院书面沟通教育的反思评判性商科本科 BUN

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虚拟团队学习效能研究:社会认知因素的影响

心理科学 2007年第1期30卷 227-231,215页

作者：唐宁玉王重鸣上海交通大学安泰经济与管理学院上海200052 浙江大学管理学院杭州310028

本研究采用现场研究的方法,对21个虚拟团队学习的效能进行了实证研究。研究对社会认知因素中的效能感和目标取向对虚拟团队学习效能(技能改变、工作任务和团队健康水平)的影响进行了研究,并探讨了对虚拟团队的态度在中间所起的作用。研... 详细信息

本研究采用现场研究的方法,对21个虚拟团队学习的效能进行了实证研究。研究对社会认知因素中的效能感和目标取向对虚拟团队学习效能(技能改变、工作任务和团队健康水平)的影响进行了研究,并探讨了对虚拟团队的态度在中间所起的作用。研究发现,虚拟团队效能感和学习取向对虚拟团队的学习效能产生作用,而对虚拟团队学习的态度、团队信任对虚拟团队学习的效能起着中介或直接的作用。

关键词：虚拟团队学习团队效旺盛目标取向对虚拟团队举习的态度团队信任

责任型领导研究:基于知识图谱的国内外研究对比分析

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管理科学 2022年第4期35卷 82-98页

作者：李叶叶唐宁玉海南大学管理学院海口570228 上海交通大学安泰经济与管理学院上海200030

企业丑闻和商业不道德行为的频发,使领导者的责任和道德行为受到广泛关注。责任型领导考虑不同利益相关者群体的利益,打破了传统的领导-员工二元关系,在应对全球社会、经济和环境等重大问题中发挥重要作用,引起了学界和商界的广泛关注... 详细信息

企业丑闻和商业不道德行为的频发,使领导者的责任和道德行为受到广泛关注。责任型领导考虑不同利益相关者群体的利益,打破了传统的领导-员工二元关系,在应对全球社会、经济和环境等重大问题中发挥重要作用,引起了学界和商界的广泛关注。特别是在新冠肺炎疫情期间和后疫情时代,责任型领导被世界各级组织和学界广泛呼吁,是对传统领导理论的新发展和新超越。通过文献计量的方法对国内外责任型领导研究的发展脉络、研究热点及发展趋势进行分析,采用CiteSpace 5.8.R3c和VOSviewer1.6.18对Web of Science和中国知网数据库中196篇相关文献数据构建知识图谱,通过引文分析、关键词共现分析和内容分析,对责任型领导的相关研究进行梳理和分析,并对未来研究前景进行展望。研究结果表明,影响责任型领导的前因有个体、情景、组织、社会和超国家因素,但前因研究基本停留在理论层面,实证研究较少。随着责任型领导概念的不断发展,近期的研究更关注责任型领导的后果。在组织内部,主要关注责任型领导对个体层面和组织层面的作用结果。在个体层面,责任型领导可以促进员工的创新行为、绿色行为和组织公民行为等积极行为,降低缺勤和不道德行为等消极行为;在组织层面,责任型领导与企业可持续发展、组织绩效、道德氛围等呈正相关。在组织外部,责任型领导能够提升组织的社会绩效和社会资本。在作用机制方面,责任型领导通过心理和知识两种路径产生影响,心理路径包括较高水平的信任、对组织的心理所有权和对组织的承诺,知识路径包括选择、创新和知识共享。目前对不同情景下责任型领导的异同、责任型领导的多重作用结果和前因的实证研究较少,通过定性分析与定量分析相结合的方式,对责任型领导的研究进行梳理,厘清了责任型领导的发展现状、前因、后果和作用机制,未来研究可以进一步关注情景因素、内在机制、多层互动、动态变化和交叉融合。

关键词：责任型领导利益相关者文献计量引文分析知识图谱