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The Effects of Magnetic Fields on Swing Amplifier 被引量:1
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作者 Chih Kang Chou, Kuo Ming Wang Institute of Astronomy and Department of Physics, National Central University Chung Li, Taiwan, 32054, China, chou @ joule. phy. ncu. edu. tw 《天文研究与技术》 CSCD 1999年第S1期274-278,共5页
The excitation and evolution of magnetohydrodynamic density waves are considered in a differentially rotating thin gaseous disk embedded with both an azimuthal magnetic field and a vertical magnetic field perpendicula... The excitation and evolution of magnetohydrodynamic density waves are considered in a differentially rotating thin gaseous disk embedded with both an azimuthal magnetic field and a vertical magnetic field perpendicular to the disk. Our results shows that the effect of isopedic vertical magnetic fields tend to stabilize the fast MHD density waves while slow MHD density waves are not affected by such vertical magnetic fields for either rigid or differential rotation. 展开更多
关键词 The Effects of magnetic Fields on Swing Amplifier
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APPLICATION OF MAGNETIZATION VISCOUS CHARACTER OF MAGNETIC FLUID IN ELECTRO-HYDRAULIC SERVO AMPLIFIER
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作者 Zhang Jiancheng Chen Jianwen Wang AilingLiu Chunrong Cao Xinming Zhou ShichangNortheastern University 《Chinese Journal of Mechanical Engineering》 SCIE EI CAS CSCD 1995年第2期172-175,共4页
The magnetic fluid is used as working medium in pilot stage of electro-hydraulic servoamplifier. Utilizing the magnetization viscous character of the fluid, a new type of electro-hydraulicservo amplifier without any m... The magnetic fluid is used as working medium in pilot stage of electro-hydraulic servoamplifier. Utilizing the magnetization viscous character of the fluid, a new type of electro-hydraulicservo amplifier without any moving parts in its pilot stage has been developed. This research provides a way for improving the frequency property and reliability of electro-hydraulic servoelements. 展开更多
关键词 magnetic fluid Magnetization viscous character Pilot stage Electro-Hy-draulic servo amplifier
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A novel current-sharing scheme based on magamp
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作者 Wen-xi YAO Xiao-yuan HONG Zheng-yu LU 《Journal of Zhejiang University-Science A(Applied Physics & Engineering)》 SCIE EI CAS CSCD 2008年第8期1150-1156,共7页
The magamp (magnetic amplifier) is widely used in power supplies due to its low cost, simplicity and other advan-tages. This paper discusses a novel application of the magamp in switching power supplies, where the mag... The magamp (magnetic amplifier) is widely used in power supplies due to its low cost, simplicity and other advan-tages. This paper discusses a novel application of the magamp in switching power supplies, where the magamp is used to regulate pulse width modulation (PWM) instead of power signal in the main circuit. This method extends the application of the magamp in power supplies, and makes it possible to further regulate control signal when PWMs have been generated. Based on this applica-tion, a new current-sharing (CS) scheme using the magamp is proposed, which uses a modified inner loop CS structure. In this scheme PWMs are generated by one main controller, and CS is achieved by regulating PWMs using a magamp in each module. Compared with traditional application of the magamp, the new CS scheme can be used in most topologies and only requires magamps of low power capacity. Then a test circuit of parallel power supply is developed, in which CS is achieved by a PWM regulator with the magamp. The proposed scheme is also used to upgrade an electroplate power to make it capable of paralleling supplies. Experimental results show that the proposed scheme has good CS performance. 展开更多
关键词 Current-sharing (CS) magnetic amplifier (magamp) PARALLEL
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A possible explanation of the knee of cosmic light component spectrum from 100 TeV to 3 PeV
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作者 林文慧 鲍必文 +1 位作者 姜泽军 张力 《Chinese Physics C》 SCIE CAS CSCD 2017年第10期110-114,共5页
A mixed hydrogen and helium(H + He) spectrum with a clear steepening at ~700 TeV has been detected by the ARGO-YBJ experiments. In this paper, we demonstrate that the observed H + He spectrum can be reproduced wel... A mixed hydrogen and helium(H + He) spectrum with a clear steepening at ~700 TeV has been detected by the ARGO-YBJ experiments. In this paper, we demonstrate that the observed H + He spectrum can be reproduced well with a model of cosmic rays escaping from the supernova remnants(SNRs) in our Galaxy. In this model, particles are accelerated in a SNR through a non-linear diffusive shock acceleration mechanism. Three components of high energy light nuclei escaped from the SNR are considered. It should be noted that the proton spectrum observed by KASCADE can be also explained by this model given a higher acceleration efficiency. 展开更多
关键词 cosmic Rays particle acceleration supernova remnants amplified magnetic field
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