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Featured researches published by Hua Huang.


Physics of Plasmas | 2013

High power operation of an X-band coaxial multi-beam relativistic klystron amplifier

Zhenbang Liu; Hua Huang; Xiao Jin; Yucong Zhao; Hu He; Lurong Lei; Zhaofu Chen

An X-band coaxial multi-beam relativistic klystron amplifier is designed in order to increase output microwave power and operating frequency of the amplifier tube. The experiment is performed on a Tesla-type accelerator. The amplifier is driven by an electron beam of 2.8 kA at 720 kV, and a microwave power of 30 kW and frequency of 9.384 GHz is injected into an input cavity by means of an external source, then a microwave power of over 800 MW is extracted, the amplifier gain is about 44 dB, and conversion efficiency is 40%. The experiment proves that output power of nearly GWs can be generated with the X-band coaxial multi-beam relativistic klystron amplifier driven by a kW-level input power.


Physics of Plasmas | 2015

Investigation of an X-band gigawatt long pulse multi-beam relativistic klystron amplifier

Zhenbang Liu; Hua Huang; Lurong Lei; Xiao Jin; Lei Zhu; Ganping Wang; Hu He; Yao Wu; Yi Ge; Huan Yuan; Zhaofu Chen

To achieve a gigawatt-level long pulse radiation power in X-band, a multi-beam relativistic klystron amplifier is proposed and studied experimentally. By introducing 18 electron drift tubes and extended interaction cavities, the power capacity of the device is increased. A radiation power of 1.23 GW with efficiency of 41% and amplifier gain of 46 dB is obtained in the particle-in-cell simulation. Under conditions of a 10 Hz repeat frequency and an input RF power of 30 kW, a radiation power of 0.9 GW, frequency of 9.405 GHz, pulse duration of 105 ns, and efficiency of 30% is generated in the experiment, and the amplifier gain is about 45 dB. Both the simulation and the experiment prove that the multi-beam relativistic klystron amplifier can generate a long pulse GW-level radiation power in X-band.


IEEE Transactions on Plasma Science | 2015

Analysis and Simulation of a Multigap Sheet Beam Extended Interaction Relativistic Klystron Amplifier

Yucong Zhao; Shifeng Li; Hua Huang; Zhenbang Liu; Zhanliang Wang; Zhaoyun Duan; Xinyi Li; Yanyu Wei; Yubin Gong

To improve the output power and electron efficiency and broaden the operating bandwidth, the three-gap extended output cavity was used in the relativistic klystron to replace the single-gap output cavity. The high-frequency characteristics of the three-gap extended cavity were studied. The electron load conductance was derived and corrected based on the theory of relativity, by which a more accurate relation of electron load conductance versus transmit angle can be obtained. The characteristic impedance is three times bigger than that of the single-gap cavity under the case of the 2π mode, which can improve the M2(R/Q) and the beam-wave interaction efficiency. The model of sheet beam klystron (SBK) is comprised of three-gap input cavity, two-gap first idler, three-gap second idler cavity, and three-gap output cavity. The 3-D particle-in-cell simulation results show that for a 500 kV, 1 kA, 40.134 GHz, and 20 W input power, the SBK is capable of generating an output power higher than 142 MW with the gain of 68.5 dB, maximum interaction efficiency of 28.4%, and 3-dB bandwidth of 240 MHz.


IEEE Transactions on Plasma Science | 2014

Design of an \(X\) -Band Gigawatt Multibeam Relativistic Klystron Amplifier

Zhenbang Liu; Hua Huang; Xiao Jin; Lurong Lei

To achieve gigawatt-level amplification output radiation in X-band, an X-band coaxial multibeam relativistic klystron amplifier is designed. When the diode voltage and diode current are increased to obtain higher output power, higher modes can seriously degrade Klystron performance and cause pulse shortening. Special measures are introduced in the device to suppress the higher mode excitation and avoid pulse shortening. Finally, pulse shortening is avoided in the coaxial multibeam relativistic Klystron amplifier. Output power of 2.1 GW with an efficiency of 40% is obtained in the particle-in-cell simulation when driven microwave power is only several kilowatts.


IEEE Transactions on Electron Devices | 2017

Investigation of a Ka-Band High-Power Sheet Beam Relativistic Extended Interaction Oscillator

Zhenbang Liu; Hua Huang; Lurong Lei; Xiao Jin; Shifeng Li; Lele Li

The sheet beam relativistic extended interaction oscillator (REIO) is a very important high-power millimeter-wave source for many actual and potential applications. A Ka-band sheet beam REIO is designed by means of particle-in-cell (PIC) simulation. In the design, we adopt a sheet electron beam with dimensions of 45 mm


Physics of Plasmas | 2018

Extended interaction oversized coaxial relativistic klystron amplifier with gigawatt-level output at Ka band

Shifeng Li; Zhaoyun Duan; Hua Huang; Zhenbang Liu; Hu He; Fei Wang; Zhanliang Wang; Yubin Gong

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Journal of Infrared, Millimeter, and Terahertz Waves | 2016

Study on Ka-Band Sheet Beam Traveling Wave Tube Focused by Closed PCM

Zhanliang Wang; Xianbao Shi; Yubin Gong; Yanyu Wei; Zhaoyun Duan; Xiaogang Su; Huarong Gong; Jinjun Feng; Hua Huang

mm to reduce the space charge effect and the extended interaction cavities to increase the power capacity. The results of the PIC simulation demonstrate the device can generate an output power of 404 MW at 30 GHz with an efficiency of 20%. In addition, we develop the experiment on a short-pulse accelerator. In the experiment, the oscillator generates a millimeter-wave power of 125 MW with a beam current of 4 kA, a beam voltage of 500 kV, and guiding magnetic field of 1 T. The frequency of the output millimeter wave is 30.6 GHz and the pulsewidth is 16 ns. The experiment proves that millimeter wave of over 100 MW can be generated with the sheet beam REIO.


Archive | 2012

Microwave power synthesis method

Cangli Liu; Anbi Chang; Xiao Jin; Jie Tan; Hua Huang; Min Luo; Qiang Kang; Fei Xiang; Mingjia Li; Ganping Wang; Hu He; Hui Jin; Shenggang Gong; Guangyao Luo

In this paper, an extended interaction oversized coaxial relativistic klystron amplifier (EIOC-RKA) with Gigawatt-level output at Ka band is proposed. We introduce the oversized coaxial and multi-gap resonant cavities to increase the power capacity and investigate a non-uniform extended interaction output cavity to improve the electronic efficiency of the EIOC-RKA. We develop a high order mode gap in the input and output cavities to easily design and fabricate the input and output couplers. Meanwhile, we design the EIOC-RKA by using the particle-in-cell simulation. In the simulations, we use an electron beam with a current of 6 kA and a voltage of 525 kV, which is focused by a low focusing magnetic flux intensity of 0.5 T. The simulation results demonstrate that the saturated output power is 1.17 GW, the electronic efficiency is 37.1%, and the saturated gain is 57 dB at 30 GHz. The self-oscillation is suppressed by adopting the absorbing materials. The proposed EIOC-RKA has plenty of advantages such as large power capacity, high electronic efficiency, low focusing magnetic, high gain, and simple structure.In this paper, an extended interaction oversized coaxial relativistic klystron amplifier (EIOC-RKA) with Gigawatt-level output at Ka band is proposed. We introduce the oversized coaxial and multi-gap resonant cavities to increase the power capacity and investigate a non-uniform extended interaction output cavity to improve the electronic efficiency of the EIOC-RKA. We develop a high order mode gap in the input and output cavities to easily design and fabricate the input and output couplers. Meanwhile, we design the EIOC-RKA by using the particle-in-cell simulation. In the simulations, we use an electron beam with a current of 6 kA and a voltage of 525 kV, which is focused by a low focusing magnetic flux intensity of 0.5 T. The simulation results demonstrate that the saturated output power is 1.17 GW, the electronic efficiency is 37.1%, and the saturated gain is 57 dB at 30 GHz. The self-oscillation is suppressed by adopting the absorbing materials. The proposed EIOC-RKA has plenty of advantages such as la...


international vacuum electronics conference | 2018

Analysis of high-order mode self-oscillation in an oversized coaxial relativistic Klystron amplifier at Ka band

Shifeng Li; Zhaoyun Duan; Hua Huang; Zhenbang Liu; Fei Wang; Xin Wang; Zhaniiang Wang; Yubin Gong


The Journal of Engineering | 2018

Oversized coaxial output cavity for Ka band relativistic klystron

Shifeng Li; Zhaoyun Duan; Hua Huang; Fei Wang; Xin Wang; Zhenbang Liu; Hu He; Zhanliang Wang; Yubin Gong

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Zhenbang Liu

China Academy of Engineering Physics

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Hu He

China Academy of Engineering Physics

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Shifeng Li

University of Electronic Science and Technology of China

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Xiao Jin

China Academy of Engineering Physics

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Yubin Gong

University of Electronic Science and Technology of China

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Zhaoyun Duan

University of Electronic Science and Technology of China

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Lurong Lei

China Academy of Engineering Physics

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Zhanliang Wang

University of Electronic Science and Technology of China

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Fei Wang

University of Electronic Science and Technology of China

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Ganping Wang

China Academy of Engineering Physics

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