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Experimental Study of Radial Wire Arrays with Added Axial Magnetic Fields

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Title: Experimental Study of Radial Wire Arrays with Added Axial Magnetic Fields


1
Experimental Study of Radial Wire Arrays with
Added Axial Magnetic Fields
Jet Experiments, Simulations and Theory
  • F. Suzuki Vidal, S.V. Lebedev, S.N. Bland, S.C.
    Bott,
  • J.P. Chittenden, G.N. Hall, A. Marocchino, J.B.A.
    Palmer
  • Imperial College London

A. Ciardi LObservatoire de Paris

2
Outline
  • Laboratory astrophysics
  • Radial wire arrays
  • Experimental setup
  • Results
  • Radial wire arrays with added BZ
  • Experimental setup
  • Results
  • Comparison with no-BZ case
  • Conclusions
  • Future aims

3
Laboratory astrophysics
  • Plasma jets are observed in large scale phenomena
  • Supernovae, Active Galactic Nuclei,Young Stellar
    Objects
  • Laboratory astrophysics with z-pinches (small
    scales!)
  • Conical wire array
  • Radial wire array
  • Dimensionless parametersare similar in both
    cases
  • Mach number, density contrast, cooling
    parameter, b parameter, etc.

4
Experimental setup
  • MAGPIE generator
  • Current of 1 MA in 240 ns

5
Experimental setup
  • MAGPIE generator
  • Current of 1 MA in 240 ns
  • Radial wire array
  • Z-pinch configuration
  • 16 tungsten wires (13mm diameter) held
    horizontally
  • 6.3 mm diameter cylindrical cathode

6
Experimental setup
  • MAGPIE generator
  • Current of 1 MA in 240 ns
  • Diagnostics
  • XUV imaging
  • X-ray detectors
  • Laser shadowgraphy and schlieren
  • Optical streak camera
  • Magnetic probes

7
Radial wire array Dynamics
(Lebedev et al, 2005)
8
Radial wire array Results
  • Formation of bubbleand axial jet
  • Typical z-pinch MHDinstabilities observed on
    the central plasma jet

9
Radial wire array Results
  • Measured expansion velocities of emitting
    boundary
  • VR 36 km/s
  • VZ 144 km/s

10
Radial wire array with added BZ
  • Why BZ?
  • An axial magnetic field can stabilise the z-pinch
    from instabilities (Felber, 1988)
  • Jet rotation? (Lebedev et al, 2002)

11
Radial wire array with added BZ
  • BZ introduced with solenoids, using the same
    current passing through the wires
  • 2 configurations

1. Solenoid replacing the standard returns posts
2. Solenoid replacing the central cathode
12
Added axial BZ Setup
  • Calculated magnetic field on axis for maximum
    current
  • Return solenoid has a more constant magnetic
    field along the axis
  • Cathode solenoid has a stronger BZ, decaying
    faster with distance
  • In both cases, BZ field is small compared with
    Btoroidal
  • BZ lt 10 Btoroidal

13
Added BZ Results
  • XUV emission
  • Bubble behaviour ismaintained
  • Expansion velocities increased with BZ
  • Features from the jet are observed with soft
    x-ray filters

Soft x-ray emission
14
Added BZ Results (comparison)
  • XUV emission
  • Central jet diameterincreased with appliedBZ
  • MHD instabilities are still observed

15
Added BZ Results (comparison)
  • XUV emission
  • Evolution of features formed in the jet can be
    measured
  • Features moving fasterwith axial distance?

16
Radial wire array Results
  • Dynamics of the bubbleare observed from
    streakimages
  • X-ray emission nearcompression of the
    centralplasma column

Optical streak camera
R
t
17
Added BZ Results
  • Optical streak camera
  • With added BZ
  • Axial jet is stable for longer times
  • Larger diameter of central plasma jet
  • Decrease of x-ray emission
  • Bounce of compressing plasma
  • Compression of magneticfield?
  • Jet rotation?

18
Conclusions
  • Experiments with radial wire arrays have been
    performed on MAGPIE, producing plasma jets
    magnetically confined by a predominant toroidal
    field.
  • Additional axial magnetic fields BZ were applied
    to a wire radial array with and compared with a
    no applied BZ case.
  • The dynamics of the magnetic bubble were
    maintained, observing an increase in the diameter
    of the central plasma jet. This suggests a
    compression of the added axial field BZ by the
    toroidal magnetic field or possible jet rotation.

19
Conclusions
  • Further analysis from present and future results
    will provide measurements of parameters for
    comparison with simulations (A. Ciardi and A.
    Marocchino) and for obtaining dimensionless
    parameters.

20
Future aims
  • New experiments are being conducted with
    different cathode diameters and wire materials
  • Jet dynamics and expansion velocities of bubble
  • X-ray emission study
  • Improvement of magnetic diagnostics to measure BZ
  • Measurement of mass density profiles in the
    ambient plasma.
  • Have the dimensionless parameters changed
    significantly from previous experiments?
  • New geometries for adding BZ!

21
Future aims
  • Twisting of anode structure to produce BZ

22
Thank you!
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