A Kinetic Theory of Planar Plasma Sheaths Surrounding
Electron Emitting SurfacesJ. P. Sheehan1, I. Kaganovich2,
E. Barnat3, B. Weatherford3, H. Wang2,D. Sydorenko4, N. Hershkowitz1, and Y. Raitses2
1 University of Wisconsin – Madison2 Princeton Plasma Physics Laboratory3 Sandia National Laboratories4 University of Alberta
DOE Plasma Science Center Teleseminar, December 7, 2012 2
Outline
● Fluid theory of emissive sheaths● Kinetic theory of emissive sheaths
● Electrons lost to surface● Temperature of emitted electrons
● Particle in cell simulations● Afterglow of capacitively coupled plasma● Measurements of emissive sheath versus time● Conclusions
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Emitted electrons reduce sheath potential and electric field at surface
● Three species
● Plasma electrons● Plasma ions● Emitted electrons
● Plasma fills the - half-plane
● One dimensional
● Emitted electrons reduce:
● The electric field at the surface
● The floating sheath potential
x̂Collecting Sheath
Emissive Sheath
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Fluid Theory: a SCL emitting surface floats Tep below the plasma potential
● Collisionless
● Φ = 0 at the sheath edge (definition)
● Plasma electrons
● Maxwellian (temperature Tep)
● Boltzmann relation
● Emitted Electrons
● Zero energy at surface
● Plasma Ions
● One species
● Cold (Ti = 0 eV)
● Singly ionized
● Integrate Poisson's equation
● Bohm's criterion, E = 0 at sheath edge
● E = 0 at surface G. D. Hobbs and J. A. Wesson, Plasma Physics 9 (1), 85 (1967).
Space-Charge Limited Solution
Φw=−eϕwT ep
=1.02 E0=miu0
2
2T ep=0.58
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Emissive probes are used tomeasure the plasma potential
● Emissive probes are Langmuir probes that emit electrons
● Usually Joule heated to emit thermionically
● Allows good control over emission current
● Used to measure the plasma potential
● Electrons are emitted when probe bias is above plasma potential, but not when below
● Can be used in plasmas where Langmuir probe measurements fail
● Smaller uncertainty than Langmuir probeJ. P. Sheehan and N. Hershkowitz, Plasma
Sources Science and Technology 20 (6), 063001 (2011).
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The floating point method isoften used in Hall thrusters
● Heat probe until floating potential saturates
● Potential at saturation is measure of plasma potential
● Heating voltage swept at 0.1Hz
● Potential measured through a high impedance op-amp
● Potential saturates past peak heating current because probe continues to heat
● Uncertainty ~0.1Te/e
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Inflection point in the limit of zero emission attempts to reduce space-charge effects● Typically 7 I-V traces were
taken
● Emission current less than electron saturation current
● Inflection point versus temperature limited emission current approximately linear
● Extrapolate inflection point to zero emission current
● Noise increases uncertainty, but using multiple emission levels reduces it
● Uncertainty ~0.1Te/e
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The floating potential of a highly emitting probe in a Hall thruster was ~2Tep below the
plasma potential
J. P. Sheehan, Y. Raitses, N. Hershkowitz, I. Kaganovich and N. J. Fisch, "A comparison of emissive probe techniques for electric potential measurements in a complex plasma," Phys. Plasmas 18, 073501 (2011).
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Motivation
● Emissive probe measurement of plasma potential● Floating potential of a highly emitting probe is near the
plasma potential● Knowledge of emissive sheath yields more accurate
measurements
● Secondary electron emission in laboratory plasmas● Significant in determining plasma potential and EVDF in
low temperature plasmas● Increase electron loss to divertors in tokamaks● Modify operation of Hall thrusters, etc....
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A fully kinetic model of the planar emitted sheath was developed
● Plasma electron loss cone: modification of EVDF due to electrons lost to the boundary
● Kinetic emitted electrons: half-Maxwellian distribution with temperature parameter Tee
● Ions are assumed to be cold● Poisson's equation and the generalized Bohm
criterion solved simultaneously● Highly nonlinear equations were solved
numerically
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Kinetic Theory: plasma electrons donot follow the Boltzmann relation
● Boltzmann relation
●
● Assumes fraction of electrons lost to surface is small
● Valid for collecting sheath, not for emissive sheath
● Full kinetic model
●
● Accounts for electrons lost to surface
● Close to surface, lost electrons are significant
● Boltzmann relation over-estimates the plasma electron density in the sheath
● Considering electrons lost to the surface reduces net charge in the sheath, reduces the sheath potential
nep(Φ)
nep(0)=exp(−Φ)
nep(Φ)
nep(0)=exp(−Φ)(1+erf (√Φw−Φ)
1+erf (√Φw) )
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Emitted Electrons: account for kinetic effects of non-zero emitted electron temperature (Tee)
● Plasma to emitted electron temperature ratio Tep/Tee = Θe
● Fluid expression
●
● Assumes Θe → ∞
● Kinetic expression
●
● Maxwellian emitted electrons (Tee)
● Fluid equations over estimate emitted electron density in the sheath
● Higher emitted electron temperature reduces emitted electron density in sheath, reduces sheath potential
nee (Φ)
nee(0)=(1− Φ
Φw )−12
nee(Φ)
nee(0)=exp (Θe(Φw−Φ))erfc(√Θe (Φw−Φ))
exp (ΘeΦw)erfc(√ΘeΦw)
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EVDFs of emitted and plasmaelectrons are modified Maxwellians
Plasma Electrons Emitted Electrons
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Emitted electrons modifythe Bohm criterion
● For arbitrary electron distribution
● Required for positive space-charge in sheath
● Solved for E0
● Since ions are cold in all descriptions, defines simple condition for ion energy
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Higher temperature emitted electrons reduce net electron density in sheath
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Emissive sheath potential is reducedby the emitted electron temperature
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Emitted electrons only slightlyaffect the Bohm criterion
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Emissive sheath wassimulated using EDIPIC
● (Performed by Hongyue “Della” Wang)
● Argon
● System length of 5 mm
● Plasma source electron temperature: 1 eV
● Plasma source ion temperature: 0.025 eV
● Collisionless
● No magnetic field
● Simulated time: 100 μs
● At source (x = 0 mm)
● Escaping particles thermalized and reflected
● Zero electric field● At emitter (x = 5 mm)
● Fixed potential of 0 V● Constant emission
current● Emitted electron
temperatures of 0.2 – 0.001 eV
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Potential profiles of emissive sheath calculated from PIC simulations
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Kinetic theory was confirmed using particle in cell simulations
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Enhanced EEDF tail (>eΦw)increases the sheath potential
● Bi-Maxwellian electron energy distribution function (EEDF)
● Two electron temperatures (Tep2/Tep = Θp)
● Hot electron fraction
● Sheath potential normalized to colder electron temperature Tep
● 5% hot electrons in figure
● Hot electrons can significantly affect the sheath potential even at low concentrations
β=nep2(0)
nep (0)+nep2(0)
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Emissive sheath potential depends nonlinearly on the hot electron fraction
● Above a certain fraction of hot electrons, the temperature of the hot species begins to dominate
● This break point depends on the plasma electron temperature ratio Θp = Tep2/Tep
● In figure, Θe = Tee/Tep = 10
● In laboratory plasmas, secondary electrons can be source of hot electrons and constitute a significant fraction of the plasma electrons
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Sheath potential has a non-monotonic dependance on the hot electron fraction● For data shown
● Θe = Tee/Tep = 10
● Θp = Tep2/Tep = 10
● Sheath potential normalized to colder plasma electron temperature
● The colder electrons define the ion flux via Bohm's criterion
● The hotter electrons dictate the electron flux through the sheath
● Sheath must be large to reduce electron current to maintain current balance through the sheath
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Planar dispenser cathode wasinstalled in GEC reference cell
● Working gas: Helium
● Neutral pressure: 25 mTorr
● Electron density: ~109 cm-3
● RF frequency: 10 MHz
● Pulse frequency: 60 Hz
● Afterglow time: 2.5 ms
● Barium tungsten dispenser cathode
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Dispenser cathode floating potential vs. time at various heating currents
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Langmuir Probe
● 1 cm long, 250 μm diameter● Positioned 3 cm above the edge of the
dispenser cathode● Aluminum tube protected against displacement
currents● I-V traces to measure electron temperature
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Emissive Probe
● 1 cm long, 76 μm
● Thoriated tungsten wire was secured by crushing the ends of copper tubes around it
● Aluminum tube reduced displacement currents for emissive probe, as well
● I-V traces to measure plasma potential using inflection point in the limit of zero emission
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Slow-sweep emissive probe method measured Vp versus time in afterglow
● Measured current vs time at many probe biases
● Transpose to determine I-V trace vs time
● Easy, inexpensive to execute
● Used for both Langmuir probe and emissive probe I-V traces
● First time inflection point in the limit of zero emission technique was used to measure temporally varying plasma potential
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Measuring Te
● Slope of semilog Langmuir probe I-V trace● Requires good signal to
noise ratio● Number averaging and
smoothing may be necessary
● Approximated by sheath potential of floating Langmuir probe● Many assumptions for
this method
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Electron temperature decaymeasured versus time
● RF ring down affected measurements tens of μs into the afterglow
● Langmuir probe could not be used for Te measurements later than ~250 μs into afterglow
● Collecting sheath potential was used to approximate the electron temperature
● Remarkable agreement between these two measurements
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Floating potential of heated electron falls, then rises in afterglow
● Afterglow: 0 – 2.5 ms
● Floating potential initially drops as plasma cools and loses density
● Increases as emitted electrons begin to dominate the discharge
● Only data before the minimum (870 μs) is relevant to compare to theory
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Plasma potential decreases monotonically in afterglow
● Plasma potential drops to a few volts in the first 100 μs
● Decays slowly through afterglow
● Becomes negative at 1150 μs, after emitted electrons begin to dominate discharge
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Electron temperaturedecays in afterglow
● Electron temperature decays rapidly once RF heating is turned off
● Monotonic decay in afterglow
● Measurement become negative after 1240 μs when floating potential exceeds plasma potential
● “Negative temperature” measurements excluded since it is in the emission dominated discharge
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Normalized emissive sheath potential is greatly reduced at low electron temperatures
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Data qualitatively follows trend predicted by theory
● Cannot directly compare: experimental measurements include presheath
● Sheath disappears when plasma electron temperature equals emitted electron temperature
● For intermediate temperatures, measured sheath is larger than expected from kinetic theory
0.1 1 10 100 1000 10 4
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Conclusions
● Kinetic theory of emissive sheaths
● Considering the plasma electrons lost to the surface reduces the emissive sheath potential by 10%
● Considering the non-zero emitted electron temperature reduces the emissive sheath potential by up to 50% for some low temperature plasmas
● Validated with particle in cell simulations
● Measurements of emissive sheath in afterglow
● Confirms that as plasma electron temperature approaches emitted electron temperature emissive sheath disappears
● Emissive sheath was larger than expected for intermediate electron temperatures
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Acknowledgments
● This work was supported by US Department of Energy grants No. DE-AC02-09CH11466 and No. DE-FG02-97ER54437, the DOE Office of Fusion Energy Science Contract DE-SC0001939, and the Fusion Energy Sciences Fellowship Program administered by Oak Ridge Institute for Science and Education under a contract between the US Department of Energy and the Oak Ridge Associated Universities