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Smoky Plasma

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Time for sedimentation (pressure dependent) is longer than the observation time. ... Meteoritic smoke particles may be nucleation sites for noctilucent clouds. ... – PowerPoint PPT presentation

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Title: Smoky Plasma


1
Smoky Plasma
  • Scott Robertson
  • Zoltan Sternovsky
  • University of Colorado, Boulder CO
  • Thanks to Plasma Science Initiative
  • and Mihaly Horanyi

2
What is smoke?
  • Standard definitions
  • Smoke particles are held aloft by weak air
    currents.
  • 2) Smoke particle diameter is lt 1 mm.
  • My definition
  • Time for sedimentation (pressure dependent) is
    longer than the observation time.

3
Motivation
  • The mesosphere has smoke particles from ablation
    of meteors.
  • Meteoritic smoke particles may be nucleation
    sites for noctilucent clouds. (NLC) particles
    (they are also smoke-like).
  • Observational evidence (from rockets) is sparse
    for meteoritic smoke.

4
The summer polar mesosphere
NLC/PMC Condensation of water into nm sized
aerosols (T lt130K) PMSE strong radar echoes
Aerosols are a dusty plasma Indicator of global
change? Required
longer term observations
NLC
PMC
Donald Petit, Space Station
5
Physics issues for NLC layers
  • Why are some NLC particles positive?
  • Why are there sometimes strong DC and AC electric
    fields?
  • Does the mesosphere support dusty plasma waves or
    instabilities?In the lab
  • How do we make a smoky plasma?
  • How do we diagnose a smoky plasma?
  • What experiments can we do? An experiment we
    cannot do strong coupling.

6
1. Why are some NLC particles positive?
  • Reduced work function?
  • Ooops! Positive particles are also observed at
    night.
  • Is electron mobility reduced?
  • Electrons may have disappeared onto negative
    ions.
  • Experiments with UV illumination,
  • with recombining smoky plasmas,
  • with electronegative gas (SF6 ),
  • will help decide among theories.

7
2. Why do rockets see strong AC DC electric
fields?
  • DC fields arise in NLC
  • Reduced electron and ion mobility increases
    resistivity locally interrupting global electric
    circuit.
  • Can this be modeled?
  • AC fields are seen in electron bite-outs
  • Does acoustic turbulence drive electric fields?
  • Why are the fields larger in bite-outs?
  • Experiments on electron and ion mobility are
    needed, as well as on the coupling of acoustic
    turbulence to electric fields

8
3. Does the ionosphere support dusty plasma waves
or instabilities?
  • High neutral density heavily damps plasma waves
    in the ionosphere.
  • Smoky plasma experiments with high neutral
    density can reveal the role of neutral damping.
  • Does Epstein formula correctly give wave damping?

9
4. Can we make smoky plasma in the lab
  • It has been done!
  • RF plasmas in silane grow smoke particles in
    situ, e.g., (Selwyn et al.)
  • Metal evaporation sources have been used to
    create nanoparticles, and UV charging was
    observed (Yokota et al., Hazelton and Yadlowsky,
    1980s)

10
4a. How to make smoke particles
  • Evaporate metal into 5 Torr inert gas.

Source characteristics 3-300 nm
particles Depends on P, T, flow log-normal
distribution 1012 cm-3 of particles 1015
particles / second
Heated crucible with metal
Differential pumping port
Heat shield
Inert gas inlet
C. G. Granqvist and R. A. Buhrman, J. Appl. Phys.
47, pp. 2200-2219 (1976) J. D. Eversole and H. P.
Broida, Phys. Rev. B 15, pp. 1644-1655 (1977).
11
4b.Getting smoke particles into the plasma
  • Smoke particles are entrained in the gas flow.
  • Gas flow rate in the source is too large
  • (5 Torr-liters/second), necessitates
    differential pumping.
  • 1 of particles are used, but this is 1013 /sec.
  • Plasma volume may be 100 liters, so this is 108
    cm-3 / sec.

12
4c. Is the smoke confined?
  • The positive plasma potential that contains
    electrons can also contain the negative smoke.
  • Suppose radius 4 nm (104 atoms). Te 1 eV,
  • then Q -8 e.
  • Presheath potential 1 eV implies 8 eV potential
    well.
  • Gravitation difference for r 4 nm Zn particle
    is 0.1 eV.
  • Smoke is electrostatically confined to the
    central presheath region for sizes up to 15 nm
    radius.
  • But we must solve self-consistently for the
    presheath with the smoke present.

13
4d. Will there be a void?
  • Theory says no, Ion drag scales with r2
  • Experiment says no, RF discharges with silane
    have no void until particles get big (Kovacevic
    et al. 2000)
  • Also, thermophoresis is small Low gas pressure
    does not support ?T

14
Photo of experiment
15
5. Diagnostics for smoke particles
  • Laser light scattering
  • Probes
  • Mobility and diffusion
  • Waves

16
5a. Laser diagnostics for particles
  • Mie scattering regime applies.Particles are not
    seen individually.Smallest size seen is r 4 nm
    _at_ 107 cm-3 (A. Gallagher lab, Proc. 3rd Intl
    Conf.)s scales as r 6, largest particles are
    seen
  • Can we get size information from angular
    dependence of light scattering?Only a
    characteristic size, weighted by r6

17
5b. Probes as diagnostics
Magnetic insulation can prevent electron
collection by a positively biased probe, so that
negative smoke particles are collected.
Rocket probe with magnetic insulation
Langmuir probe with magnetic insulation from
current I
I
B
18
5c. Mobility and diffusion as a size diagnostic
tool
  • In neutral gas, smoke particle density decay time
    reveals diffusivity and hence size

UV flash lamp

I(t)
-
UV charged smoke particles electric drift reveals
mobility (vdrift m E) and hence size.
19
5d. Smoky plasma wavescan be a diagnostic
  • Dust acoustic mode is easily driven unstable
    Theory Rosenberg, Planet Sp. Sci. 41, 229
    (1993)Most recent Trottenberg, et al., Phys.
    Plasmas 13, 042105 (2006)
  • Ion acoustic shocks with dust Nakamura et al.,
    Phys. Rev. Lett. 83, 1602 (1999)
  • Dust acoustic solitonsIvlev and Morfill, Phys.
    Rev. E 63, 026412 (2001)Kompaneetz, Tsytovich
    and Morfill, IEEE TPS 32, 561 (2004)

20
6a. Smoke plasma recombination experiments
UV induced smoke plasma (not smoky plasma)
UV flashlamp
? Measure recombination and density decay after
the flash.
21
6b. Smoky plasma particle and energy balance
Add smoke to hot-filament discharge at 0.5 mTorr
Ar.
What densities can be obtained ne, ni, nd ,
nd/ne? Is recombination on smoke particles or the
wall?
22
6c. Smoky plasmawave experiments
Add smoke to hot-filament discharge at 0.5 mTorr
Ar.
Grid antenna
? Launch smoke acoustic waves? solitons?
23
6d. Acoustic (ordinary sound) wave experiments in
smoky plasma
Add sound waves for wave coupling.
P gt 1 mTorr
Loud speakers
? How are sound waves and electrostatic waves
coupled?
24
6e. Theory for coupling of acoustic and plasma
waves
  • is the Epstein drag coefficient that couples
    particles and neutrals.The momentum equation for
    each of the species j (i, e, or a)

Poisson couples all charged species
The electric field driven by the acoustic waves
is (see poster paper)
n0 and u0 are fluctuation air density and
velocity.
25
Conclusion
  • Look for experimental results
  • at the next Dusty Plasma Workshop.
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