arc modeling at sumy,ukraine

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Arc modeling at Sumy,Ukraine Speakers: Serhiy Mordyk (Institute of Applied Physics, National Academy of Sciences of the Ukraine)

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Arc modeling at Sumy,Ukraine Speakers: Serhiy Mordyk (Institute of Applied Physics, National Academy of Sciences of the Ukraine). DC-spark breakdown. Laser—induced breakdown. RF breakdown. What kind of plasma is produced during a breakdown, how does it develop with time?. - PowerPoint PPT Presentation

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Arc modeling at Sumy,Ukraine

Speakers: Serhiy Mordyk (Institute of Applied Physics, National

Academy of Sciences of the Ukraine)

It is necessary to know plasma parameters for arc modeling

Laser—induced breakdown

RF breakdown

DC-spark breakdown

What kind of plasma is produced during a breakdown, how does it develop with time?

Optical spectra tell us:• Compositions: elements & molecules (line positions)• Ion temperatures of plasma (Doppler effect)• Vibrational and rotational temperatures of plasma (line

strengths and positions)• Pressures (line widths: pressure broadening)• Plasma density ( Stark broadening)• Magnetic fields (Zeeman splitting)Mass spectra tell us:• Compositions: elements & molecules • Time-resolved dynamics of dischargeMicrowave interferometer tells us:• Plasma density

Plasma Plasma diagnosticsdiagnostics

Setup for measurement of plasma parameters

Time-resolved laser mass spectrometer

Optical spectrometer

Optical spectrum of nitrogen

Helicon discharge (IAP NASU)

Determination of vibrational and rotational temperature is necessary for modeling of kinetic of plasma processes

Hydrogen optical line

•H Balmer beta (486,1 nm) Plasma density

Stark broadening

Doppler effect

Ion temperatures of plasma

•H Balmer alpha (656,3 nm)

DC-spark (data from Jan Koverman)

Sample Cu 9(7)

DC-spark (data from Jan Koverman)

Sample Cu 9(7)Strong optical line Н2 (462.9 nm)

Processing of optical spectra was carried out with the assistance of Dr. O.M. Buhay

Mechanisms underlying RF breakdowns in high-gradient Mechanisms underlying RF breakdowns in high-gradient accelerating structures accelerating structures

explosion (Power absorption, Joule law)explosion (Power absorption, Joule law)

evaporation (Cu, H, O, N …) + Power absorptionevaporation (Cu, H, O, N …) + Power absorption

ionization – dischargeionization – discharge

electron electron plasma formation and disassimilationplasma formation and disassimilation ionion

PIC modelPIC model

, , ,,

1i e i e i ei e

f f fv e E v H S

t r c v

4 1 1,

E Hrot H j rot E

c c t c t

4 , 0ediv E div H

,e i e i ee f f dv j e v f f dv

Vlasov–Boltzmann Equation

Maxwell’s equations

Charge density, current density

Source codes at OOPIC (Berkeley Laboratory) http://langmuir.nuc.berkeley.edu/pub/codes/xoopic/

The length of the space z = 0.00005 m

The radius of the space r = 0.00001 m

The simulation time step Δt = 0. 001 ns

The electron temperature Te = 5 eV

The ion temperature Ti = 1 eV

Initial plasma density n = 1019 m-3

Pressure in chamber p = 0.000001 Torr

DC voltage φ = - 12000 V

Initial parameters

Initial state of plasma

anodecathode

Electrons on the anode

Ions CU on the cathode

Ions CU on the cathode

Equations system of the two fluids hydrodynamics

Poisson equations

Fluid model

A

PLASMA C

Equation of motion

Integration modelIntegration modelVlasov–Boltzmann Equation:

Poisson’s equation

where na is the density:

Photoionization

ConclusionConclusion

It is necessary to know plasma parameters for arc modeling