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Field experiment using transient energy method to locate a single-phase to ground fault 被引量:1
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作者 Wei Xie Xuewen Wang +4 位作者 Chen Fang Hengxu Zhang Fang Shi Xiaodong Xing Baicong Sun 《Global Energy Interconnection》 CAS 2020年第6期585-594,共10页
Distribution networks in China and several other countries are predominantly neutral inefficiently grounding systems(NIGSs),and more than 80%of the faults in distribution networks are single-phase-to-ground(SPG)faults... Distribution networks in China and several other countries are predominantly neutral inefficiently grounding systems(NIGSs),and more than 80%of the faults in distribution networks are single-phase-to-ground(SPG)faults.Because of the weak fault current and imperfect monitoring equipment configurations,methods used to determine the faulty line secti ons with SPG faults in NIGSs are in effective.The developme nt and application of distributi on-level phasor measurement units(PMUs)provide further comprehensive fault information for fault diagnosis in a distribution network.When an SPG fault occurs,the transient energy of the faulted line section tends to be higher than the sum of the transient energies of other line sections.In this regard,transient energy-based fault location algorithms appear to be a promising resolution.In this study,a field test plan was designed and implemented for a 10 kV distribution network.The test results dem on strate the effective ness of the transient en ergy-based SPG locati on method in practical distributi on networks. 展开更多
关键词 Sin gle-phase-to-gro und fault Fault location Neutral in efficiently groundi ng systems Distributi on n etwork Distribution-level PMU transient energy.
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Progress of GECAM Observation Research
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作者 WANG Chenwei ZHANG Yanqiu +8 位作者 XIONG Shaolin LIU Jiacong TAN Wenjun XIAO Shuo XIE Shenglun XUE Wangchen ZHAO Haisheng ZHAO Yi ZHENG Chao 《空间科学学报》 CAS CSCD 北大核心 2024年第4期668-673,共6页
Gravitational wave high-energy Electromagnetic Counterpart All-sky Monitor(GECAM)is a constellation with four instruments(launch date):GECAM-A/B(10 December 2020),GECAM-C(27 July 2022)and GECAM-D(13 March 2024),which ... Gravitational wave high-energy Electromagnetic Counterpart All-sky Monitor(GECAM)is a constellation with four instruments(launch date):GECAM-A/B(10 December 2020),GECAM-C(27 July 2022)and GECAM-D(13 March 2024),which are dedicated to monitoring gamma-ray transients in all-sky.The primary science objectives of GECAM include Gamma-Ray Bursts(GRBs),Soft Gamma-ray Repeaters(SGRs),high energy counterparts of Gravitation Wave(GW)and Fast Radio Burst(FRB),Solar Flares(SFLs),as well as Terrestrial Gamma-ray Flashes(TGFs)and Terrestrial Electron Beams(TEBs).A series of observations and research have been made since the launch of GECAM-A/B.GECAM observations provide new insights into these highenergy transients,demonstrating the unique role of GECAM in the“multi-wavelength,multi-messenger”era. 展开更多
关键词 GECAM Gravitational wave electromagnetic counterpart High energy transients
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