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Noctilucent Clouds, Polar Mesospheric Summer Echoes, and Dusty Plasmas

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R. B. Sheldon (1), H. D. Voss (2), P. A. Webb (3), W. D. Pesnell (3),R. A. Goldberg (3), J. Gumbel (4), M. P. Assis (2) 1) NSSTC, 2) Taylor University 3) NASA/GSFC, 4 ... – PowerPoint PPT presentation

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Title: Noctilucent Clouds, Polar Mesospheric Summer Echoes, and Dusty Plasmas


1
Noctilucent Clouds, Polar Mesospheric Summer
Echoes, and Dusty Plasmas
  • R. B. Sheldon (1), H. D. Voss (2), P. A. Webb
    (3), W. D. Pesnell (3),R. A. Goldberg (3), J.
    Gumbel (4), M. P. Assis (2)
  • 1) NSSTC, 2) Taylor University 3) NASA/GSFC, 4)
    Stockholm University
  • November 3, 2006

2
NLC gallery
3
NLC viewing geometry
4
ISS, Courtesy NASA
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6
Radar, Lidar observations
7
Observations Open Questions
  • NLC are gt20nm ice grains forming at the mesopause
    140K. Reported since 1885. Peak occurrence after
    summer solstices. Explained by mesosphere weather
  • PMSE first observed in 1979 at Poker Flat, are
    related to lt10nm charged ice grains usually in a
    layer 2 km above NLC, that reflect radar
    (50MHz-2GHz or 2'-100' wavelengths). Strongest
    at midnight, weakest at dusk.
  • PMSE How do they reflect? Why do they form? What
    relation to NLC?

8
How can aerosols reflect radar?
  • Charged aerosols? large plasma density?
  • If they are positive, then electron density rises
  • Draine Sutin 87 argued for nm dust to become
    positive (because of large E-fields)
  • Havnes flies retarding grids, Gumbel flies
    alternating plates, Rapp, Horanyi, et al fly
    magnets to exclude electrons and trap positive
    ions/aerosols
  • PMSEs have negative dust, NLCs maybe positive?
  • Charged aerosols? large plasma gradients?
  • Langmuir probes see bite-outs
  • Havnes argues for dust vortices to make holes
  • Multiple Langmuir probes never agree on
    bite-outs
  • Reflections are coherent Bragg, not incoherent
    turbulence

9
DROPPS Rocket Concept
Rocket in ram, 1 km/s Particle Impact, PID
Particle Trap, PAT Particle Spect., SSD
Probes and Plasma Optical sensors, e-
precip. Wake effects Sublimation Rocket
Interactions Goldberg et al. GRL 2001
10
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11
PID Charge/Mass Telescopes and PAT
Sun
RAM
RAM
SUN
SUN
RAM
12
Particle Trap (PAT) instrument
PMSE
NLC
13
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14
Sun-illumination Model
15
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17
Positively Charged Aerosols??
18
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20
Calculated Work Functions
21
Particle Trap (PAT) instrument
PMSE
NLC
22
Water Cluster Ion Charging
Vostrikov 87, Andersson 97
23
Water Work Function
  • Assuming the rocket work function 5.04V
  • Gold 5.3 ?wet 4.92 eV
  • Carbon 4.9?wet 4.87 eV

24
Electron Density Bite-outs??
25
DEMETERLangmuir Probes
26
DROPPSLangmuir Probes
Bite-outs are sharp decrease Nelt 1/10
27
Upleg and Downleg for Charge Telescope grids 1, 2
3
28
Big Bite-out, where's the PMSE?
29
Langmuir Probe Theory
30
PID Upleg profile
31
PID Downleg profile
32
PID TelescopesShockLangmuir Plasma ProbeX10
DensityCushioned Deceleration HeatingSublimatio
nClean Time (200ms )
Gumbel and Smiley Simulations
33
Chamber Clean Out Time
  •  t x2 / D  where x 8cm length of telescope
    (or back plate to CGRID2)              and D
    diffusion constant. D 1/3 ltvgt L  where ltvgt is
    average thermal speed and L is mean free path L
    1 / (n s)  where the density (from Smiley) is
    4e21/m3                and s cross section for
    water molecules or clusters. Guessing for s
    pi (r), where r (cube root of density) 0.3
    nm           (and of course, water cluster ions
    might be bigger)   s 3e-19 m2Giving   L
    8e-4 mThen ltvgt sqrt(3kT/m) where m 30 AMU,
    T 500K (from Smiley)        giving 642
    m/sFinally, D 0.18and the diffusion time
    x2/D 0.082/0.18 36ms

34
Mitchell et al (2001) analysis
Upleg vs downleg PMSE observed with blunt probes
and Aft probe. Note blunt temporally PRECEDES
aft biteout. -blunt nearly simultaneous. UV
Spin modulation strong on upleg, and contributes
to biteout signature, less so on downleg.
35
Charged Dust Collection
36
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38
PID and PAT compared
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41
Ionospheric Chapman layer
42
Ice charging Model
  • Ice grains are in equilibrium with UV and Ne.
    ltqgt -1
  • Chapman layer e- are 10eV ltqgt gt -1
  • Abbas--proposal

43
Range and Secondary e- in Ice
Minima!
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45
PIXIE Xray vs Kp,Dst(1996-98)
Petrinec, GRL 1999
46
Precipitating Electron effects
  • The dusk side is depleted in electrons
  • The energy of the electrons changes the
    Chapman-layer altitude. Double peaked energy
    spetra would produce double layers in atmosphere.
  • Electron energy is a function of MLT
    magnetosphere activity.

47
Dust Acoustic Waves
Thomas, 2002
U Iowa, Physics Today, 2004
48
Conclusions
  • There is no evidence for positive charged
    aerosols. Water work function explains current.
  • Electron density bite-outs are likely
    instrumental
  • PMSE's are subvisible lt10nm ice that has a high
    charge state. The charge state may be a direct
    result of gt10 keV electron precipitation
  • Dust Acoustic Waves may be responsible for the
    Bragg-reflected radar returns
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