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Plasma Application Modeling, POSTECH

Date post: 04-Jan-2016
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Plasma Application Modeling, POSTECH. XOOPIC and MAGIC Codes for Electromagnetic Field. S.J. Kim and J.K. Lee. Contents. Overview of XOOPIC code Overview of MAGIC code Klystron simulation using XOOPIC code. Plasma Application Modeling, POSTECH. Overview of XOOPIC Code. - PowerPoint PPT Presentation
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Plasma Application Modeling, POSTECH Overview of XOOPIC code Overview of MAGIC code Klystron simulation using XOOPIC code Contents XOOPIC and MAGIC Codes for Electromagnetic Field S.J. Kim and J.K. Lee
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  • Overview of XOOPIC code Overview of MAGIC code Klystron simulation using XOOPIC codeContentsXOOPIC and MAGIC Codes for Electromagnetic Field S.J. Kim and J.K. Lee

  • Overview of XOOPIC Code Two dimension and three velocity Cartesian (x-y) or cylindrical (r-z) coordinates Electrostatic or full electromagnetic field Discrete model (Finite-Difference Method) : uniform or non-uniform mesh Boltzmann and inertial electrons Immobile and inertial ions Monte-Carlo collision model Complex boundaries : conductor, cylindrical axis, wave ports, absorption, transmission, emission.XOOPIC Features* Values of gridded quantities can be approximated at intermediate points by interpolation.

  • Program FlowDefined region of the discrete modelElectromagnetic fields on the meshDiscretization meshGroup of similar particlesIndividual particle (position, momentum, mass, charging, numerical weight)

  • Maxwells Equations for Electromagnetic FieldMaxwells equations in integral formC-1, L-1: coupling matrices withthe dimemsionality of capacitanceand inductance.Nonuniform orthogonal Yee mesh

  • Maxwell Curl EquationsTransverse magnetic (TM) setTransverse electric (TE) setThe TM and TE field equations are advanced in time using a leap frog advance.The currents result from charged particle motion.

  • Velocity Advance Half acceleration: Rotation: Half acceleration: Relativistic Boris advance

  • Charge Conserving Current Weighting AlgorithmCharge conserving current weighting =

  • Overview of MAGIC CodeUniform gridManual gridAppended regionsPolynomial smoothly varying gridPade smoothly varying gridResistiveDielectricConductorsScattering foilPolarizer sheetHelix elementGeneral current sourceAir chemistrySemiconductorCartesian coordinatesPolar coordinatesCylindrical coordinatesSpherical coordinatesMirror symmetry boundaryPeriodic symmetry boundaryAbsorbing boundaryOutgoing wave boundaryApplied voltage boundaryExternal circuit voltage sourceParticle and field importStandard leapfrogTime-reversible leapfrogSemi-implicitStandard noise filteringHigh-Q noise filteringQuasistaticElectrostatic ADIElectrostatic SORExternally specified magnet fieldRestricted TE or TM modes GridMaterialsGeometryField algorithm Application fields : microwave amplifiers, antennas, sensors, fiber optics, lasers, accelerator components, beam propagation, pulsed power, plasma switches, microwave plasma heating, ion sources, field emitter arrays, semiconductor devices, wave scattering, and coupling analyses Particle-in-cell (PIC) approach Maxwells equations on a finite-difference grid for electromagnetic fieldElectromagnetic computational processing cycleMAGIC code

  • Method and NoiseLeapfrog time integration schemeWell-centering Particle-induced noise is introduced through the current term in Maxwells equations. Propagating, wave-like, electromagnetic nose Large curl derivatives Time-biased and high-Q algorithms Spatial fluctuations in space charge and the Gausss law constraint The slow, self-heating instability Charge allocation algorithmTransverse particle noiseLongitudinal particle noise

  • Time-Biased AlgorithmTime-biased algorithm : semi-implicit schemea1, a2, and a3 determine the degree of spatial filtering and the time-centering.i : iteration coefficient=k/kmax : normalized eigenmodekmax : maximum spatially-resolvable Fourier wave number

  • Charge Conservation SchemeBoris-DADI correctionLangdon-Marder correction

  • Simulation Domain of KlystronRF input portRF output portE-beamCylindrical Axis10.05 cm13.07 cm9.55 cm37.2 cm7.569 cm6.66 cm Simulation condition: Beam emitter: I= 12 kA, ud =2.48e8 m/s Input port : Rin=2300 , R=20 , f=7.69 GHz Output port : R=47.124

  • Example of Klystron Simulation Phase spaceDensityKinetic energyuz

  • Simulation Results at 0.5 ns

  • Simulation Results at 2.5 ns

  • Simulation Results at 10 ns

  • Simulation Results at 20 ns

  • Simulation Results at 6 us

  • KE as a Function of Beam Current

  • KE as a Function of Beam Energy

  • Klystron Phase spaceDensityKinetic energyuz2 cm3 cm

  • Simulation Results at 0.5 ns and 2.5 ns

  • Simulation Results at 10 ns and 20 ns

  • Simulation Results at 6 us


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