MHD Dynamos in the Lab and Dynamos Beyond MHD. The lab plasma dynamo does Generate current locally...
Transcript of MHD Dynamos in the Lab and Dynamos Beyond MHD. The lab plasma dynamo does Generate current locally...
MHD Dynamos in the Lab
and
Dynamos Beyond MHD
The lab plasma dynamo does• Generate current locally • Increase toroidal magnetic flux• Conserve magnetic helicity• Act through alpha and other effects• Arise from fluctuations superposed on the mean
field• Achieve a nonlinearly saturated steady state
(with full backreaction)
The lab plasma dynamo does NOT• Generate magnetic field from a small seed field• Increase magnetic energy (it redistributes
magnetic field)
in experiment
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V/m
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0.0 0.2 0.4 0.6 0.8 1.0ρ/a
E||
ηneo J||(Zeff = 2)
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E ≠ η j
E||
ηj||
radius
additional current drive mechanism (dynamo)
Measure quantities during discrete dynamo event
ToroidalMagneticFlux(Wb)
MST
time (ms)
The MHD Dynamo
The nonlinear dynamo
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⟨E⟩
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⟨ j⟩
⟨B⟩
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⟨ ˜ v ⟩,⟨ ˜ B ⟩energysource
instability
dynamo
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E + ˜ v × ˜ B = η jMHD
dynamo
analytical quasilinear theory, nonlinear MHD computation
tasks
• Measurements of dynamo
• Active flow drive
• Connections to more general
problem
MHD Dynamo: Status of Past Measurements
• edge measurements with probes, core with passive Doppler spectroscopy
• Important in edge and core, but not full story
time (ms)
r/a = 0.9
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⟨ ˜ v × ˜ B ⟩
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η⟨ j⟩− ⟨E⟩
MHD dynamo dominant at some radii, not everywhere
r/a = 0.8
Measurement of MHD dynamo
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Volts m
Volts m
-0.5 0 0.5time (ms)
r/a = 0.9
r/a = 0.8
MHD Dynamo Measurements(~ 3 year project)
• Measure spatial profile of <v x B> in MST
good progress in CHERS for v - now debuting
laser Faraday rotation improving (B)motional Stark effect in several years (B)probes for edge
• Measure dynamo and helicity changes in MRX
probes
SXR imaging of dynamo instabilities
information on 3D structure of magnetic field,
collaboration with RFX team (P. Franz, P. Martin, L. Mirelli)
QuickTime™ and aTIFF (LZW) decompressor
are needed to see this picture.
spatial resolution being improved
Active Flow Drive
• Present experiments:
• Flow drive experiments
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j ⇒ ˜ v ⇒ B
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v ⇒ B
Exploratory: flow drive via neutral beam injection,
inject ~ 25 keV beam of neutral atoms,
transfers momentum to plasma
Test experimental feasibility in MST
Beam installed;
momentum transfer tested in few months
If good absorption, then model with MHD computation, implement in MST and MRX
from Novosibirsk
Investigate why alpha effect (<v x B>) large in lab, small in geometrically simpler computation
Specifics of flow pattern?
dynamo effects beyond MHD
Effects from Two-Fluid Theory
parallel mean-field component,
Linear part,
Using in top eqn,
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E + v × B −j × B
ne−∇pe
ne= ηj
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E||+ ˜ v × ˜ B
||+
˜ j × ˜ B ||
ne= η j
||
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˜ v −˜ j
ne≈
˜ E × B
B2 −
∇˜ p e × B
B2
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E||+
˜ E ⊥˜ B ⊥
B2 +
(∇⊥˜ p e ) ˜ B ⊥
B2 = η j
||
MHD Hall
Pressureless MHD
diamagnetic
<E>|| + dynamo = η<j>||
Dynamo theory statusMHD QL, NL comp
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˜ v × ˜ B
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˜ j × ˜ B
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˜ B ⊥∇˜ p ⊥
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˜ B r ˜ p ||
Hall QL
Diamagnetic very little
Kinetic RR, constraints fromLandau resonances
Status of non-MHD effects
• Diamagnetic dynamo observed in edge probe measurements under some conditions
• Hall dynamo observed in MST recently
Hall dynamo measured by laser Faraday rotation
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~ nB ⋅dl∫
(Ding, Brower, Deng)
11-chordFIR laser
rotation angle
Experimental Goal
Determine locations and conditions at which different dynamo mechanisms dominate
Experimental Plans
• Measure diamagnetic dynamo (probes in MST and MRX, explore Thomson scattering for pe)
• Measure ve x B (= v x B + j x B/ne)(explore laser Fizeau effect for ve,)
• Measure Hall dynamo with improved spatial resoluton
(Faraday rotation, MSE, probes)
Hall Dynamo Theory and Computation
• Expand quaslinear calculation to finite pressure
• Develop early nonlinear theory (Rutherford theory)
• Develop two-fluid computation for lab plasma (Nimrod)
Related work:
Two-fluid computation in a box shows Hall dynamo important under some conditions(Minnini, Gomez, Mahajan)
Ongoing
Assessment of astrophysical relevance of various dynamo effects