J.H. Degnan- Compression of Field Reversed Configurations for Magnetized Target Fusion

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    COMPRESSION OF FIELD REVERSED CONFIGURATIONS

    FOR MAGNETIZED TARGET FUSION

    presented by

    Dr J. H. Degnan

    Air Force Research Laboratory

    Directed Energy Directorate

    Presented at Symposium on Current Trends in International

    Fusion Research7-11 March 2005

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    2

    COMPRESSION OF FIELD REVERSED CONFIGURATIONS

    FOR MAGNETIZED TARGET FUSION

    J.H.Degnan, A. Brown (2), T.Cavazos (1), S.K.Coffey (2), M.Frese (2), S. Frese (2), D.Gale (1),

    C.Gilman (1), C. Grabowski (1), B. Guffey (2), T.P.Intrator (3), R.Kirkpatrick (3), G.F.Kiuttu,

    F.M.Lehr, R.E.Peterkin, Jr (1), N.F.Roderick (4), E.L.Ruden, R.E.Siemon (5), W.Sommars (1), Y F.

    Thio (6), P.J.Turchi (3), G.AWurden (3), S. Zhang (3)

    Directed Energy Directorate, Air Force Research Laboratory, Kirtland AFB, NM, USA

    (1) SAIC, Albuquerque, NM, USA

    (2) NumerEx, Albuquerque, NM, USA

    (3) Los Alamos National Laboratory, Los Alamos, NM, USA

    (4) Permanent address: Department of Chemical and Nuclear Engineering, University of New Mexico,

    Albuquerque, NM, USA

    (5) University of Nevada Reno, Reno, NV, USA

    (6) DOE-OFES

    This research was sponsored by DOE-OFES

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    3

    Elements Of Magnetized Plasma Compression, akaMagnetized Target Fusion (MTF)

    Thin i mploding liner

    Mega-ampere current

    10 k eV plasma

    Magnetic

    guide field

    Typical parameters:Initial Final

    n 10 17 cm-3 10 20 cm-3

    T 300 eV 10 keVB 100 kG 10 MG

    Guide-field co ils

    Plasma preheater and i njector Liner implosion sys tem

    FRC

    Conical theta pinch

    Thin i mploding liner

    Mega-ampere current

    10 k eV plasma

    Magnetic

    guide field

    Typical parameters:Initial Final

    n 10 17 cm-3 10 20 cm-3

    T 300 eV 10 keVB 100 kG 10 MG

    Guide-field co ils

    Plasma preheater and i njector Liner implosion sys temPlasma preheater and i njector Liner implosion sys tem

    FRC

    Conical theta pinch

    ~10

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    MTF Is A Hybrid Of ICF And MFE

    ICF relies on rapid imploding boundary to achieve adiabaticcompression of fuel

    - requires driver to deliver megajoules in nanoseconds

    - requires several 10s cm/microsecond implosion velocity

    - validated by underground tests

    MFE relies on magnetic field to confine modest density, hightemperature plasma for seconds or longer

    - problems are instabilities and impurities

    - has achieved gain ~ 0.5 (gain = energy out/energy in)

    MTF uses magnetic field to suppress thermal conduction , imploding

    boundary to compress plasma

    - requires 10s of megajoules in ~1 to 10 microseconds- requires ~ 1 cm/microsecond implosion velocity

    - greatly reduced driver power (x100 to 1000) relative to ICF

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    Magnetized Target Fusion

    Magnetized target fusion (MTF)

    identified in US and Russia as an

    alternate approach intermediate between

    MFE and ICF parameter regimes

    Closed magnetic field configurations

    reduce electron thermal conductionlosses

    Enables (slower) adiabatic compression

    with modest driver requirements

    ~10X radial compression required

    Typical precompression plasma

    parameters: 100 eV, 1017 cm-3, 5 T

    Required Plasma Energy vs. Density

    for various transport assumptions

    1

    103

    106

    109

    1012

    1014

    1016

    1018

    1020

    1022

    1024

    1026

    Density (cm-3)

    PlasmaEnergy(Joules)

    CT Classical

    CT Bohm

    ICF electron

    thermal cond.

    Chi=1m2/sec

    MFE

    MTF

    ICF

    LANL

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    Closed magnetic field lines

    Magnetic field line tension squeezes axially when radially compressed

    Particles that drift across flux surfaces are lost to open field lines beyond

    separatrix

    Equilibrium lifetime is anomalously long (many Alfven times), but nottheoretically understood

    LANL

    Field Reversed Configuration

    Self Organized Magnetic Equilibrium

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    Initial diagnostics for FRC formation Diamagnetic field exclusion magnetic probe

    array

    Radial view laser interferometry

    Axial view fast photography Current and voltage probes on all discharges

    Later additional FRC formation diagnostics Vacuum ultraviolet (VUV) probe arrays for

    purity monitoring and temperature, density

    information

    LANL

    Diagnostics

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    AFRL eight chord laser interferometer installed on

    FRC formation system at LANL

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    time (Qs)10 12 14 16 18 20 22

    n

    /1016(cm-3

    )

    0

    2

    4

    6

    8

    10

    12r! 0.0 cm

    r! 0.7 cm

    r!1.9 cm

    r!2.4 cm

    r!3.0 cm

    r!3.4 cm

    r!3.6 cm

    r!4.2 cmr!5.2 cm

    Density vs. time at various radii via Abel Inversion.

    The radii chosen correspond to the closest approach of each laser

    chord to the FRC axis (impact parameters). Shot 1973

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    radius (cm)0 1 2 3 4 5

    n

    /1016(c

    m-3

    )

    -2

    0

    2

    4

    6

    8

    10

    10 Qs

    12 Qs

    14 Qs

    16 Qs

    18 Qs

    20 Qs

    impact parameters

    Density vs. radius at various times for FRC

    inferred from Abel Inversion algorithm.

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    FRC

    parameter

    How

    measured

    goal Experiment

    peak

    Experiment

    equilibrium

    comments

    density laser

    interfer-

    ometry

    1017 cm-3 ~ 6 x 1016 ~ 2 x 1016 has toroidal

    profile

    Temperature

    Ti } Te

    via

    density

    and

    pressure

    from field

    exclusion

    ~ 200 eV~ 200300

    eV

    ~ 100 eV

    lifetime via

    n, p vs t

    ~ 20 Qsec ~ 10 Qsec may be

    limited by

    crowbar

    ripple

    FRC status as of mid 2003: achieved parameters are

    approaching pre-compression goals

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    ASSEMBLY DRAWING

    SOLID LINER

    PP-99028-1A

    1999 SHOT SERIESr = 5 cm, 1 m/m < t < 2 m/m

    30 cm TALL CYLINDRICAL LINERENGINEER:

    CHECKER:

    DRAFTSMAN: U.S. AIR FORCE

    SCALE:

    DRAWING NO.

    TITLE:

    PL-WSP

    D.GALE

    COMPUTER FILE NAME: :

    D.GALE

    1/3S99ASY6A.DWG

    SHT 1 OF 1

    FRC Compatible Imploding

    Liner Hardware Design

    - The 30 cm long liner

    implosion experiments

    extend our experience to

    longer liners

    - The diagnostics on these

    initial shots include flash

    radiography, interior

    magnetic field

    compression, dischargecurrent and voltage, and an

    interior instrumented

    impact package

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    Shiva Star Facility at AFRL

    Shiva Star Capacitor Bank (up to 9 Megajoules, 3 Qsec)

    available now for implosion - compression experiments

    82 kV, 1300 uF, 44 nH

    for first Z-pinch driven

    long liner experiments

    ~12 Megamp, ~10Qsec

    risetime discharge

    implodes 30 cm long, 10

    cm diameter, 1.1 mm

    thick Al liner in 24Qsec

    4.4 MJ energy storage

    gives 1.5 MJ in liner KE

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    Radiographs from FRC compatible

    Liner Implosion on Shiva Star

    t = 0.0Qsec, diam = 10 cm

    Achieved velocity, radial convergence, symmetry, stability

    needed for compression of FRCs to MPC conditions

    13 x radial

    convergence

    Shot 1

    20.0Qsec

    Shot 2

    22.0

    Qsec

    Shot 2

    23.0Qsec

    Adjacent

    lower

    electrodeMid-gap

    Central probe

    package (1

    cmdia.)

    LinerLower electrode

    Liner

    Central probe

    package

    (0.64 cm dia.)

    Shot 1

    23.5Qsec

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    Avoiding Sliding Liner-electrode

    Contact

    Avoiding the sliding liner-electrode

    contact is desirable in order to:

    - Avoid impeding FRC injection into

    interior of liner- Improve purity of injected FRC

    - Improve axial diagnostic access

    Two approaches to achieving this are:- Using deformable liner-electrode

    contact for Z-pinch driven liner

    - Using a theta-pinch driven liner

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    Connecting current to the liner

    Uniform-thickness liner Variable-thickness or shaped liner

    Glide-plane electrodes

    used in 1999 Shiva-Star experiments

    would interfere with FRC injection Shaped liner recently tested

    Liner

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    2D-MHD simulations indicate feasibilty of

    deformable liner-electrode concept

    Deformable Liner-Electrode Contacts Offer Advantages in Purity of the

    Compressed Plasma and Diagnostics Access for Z-pinch Driven Liner;

    these examples are for8 cm diameter electrode apertures

    Double frustrum and smooth liner

    initial thickness profiles

    Double frustrum profiled

    liner density contours at ~ 1

    Qs before peak compression

    Smooth profiled liner

    density contours at ~ 1 Qs

    before peak compression

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    2D-MHD simulated density contours for similar

    parameter liner implosion, at 0.5 Qs before stagnation.

    Experimental radiograph for portion of liner

    adjacent to electrode, at 22 Qs after start of current,

    approximately 0.5 Qs prior to peak compression.

    Bottom of liner to top of field of view is

    approximately 4.5 cm.

    Static radiograph of portion of liner adjacent

    to electrode, prior to experiment. Innerdiameter = 9.78 cm.

    Overlay of 2D-MHD simulation density contours and radiographs at

    approximately same size scales.

    Deformable contact liner implosion performed with 8 cm

    diameter electrode apertures; results indicate that Z-

    pinch imploded liner approach is feasible

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    Top: radiograph of liner at t=0, near mid-gap,

    ID = 9.78 cm, OD = 10.0 cm.

    Bottom: radiograph of liner at t = 22 Qsec, near

    mid-gap. ID of non-m=0 portion $ 0.58 cm,

    corresponding to radial compression of innersurface ~ 17. We believe that the m=0 portion

    is right at mid-gap. If there had been an FRC

    inside, it would be compressed > 10x radially

    prior to significant growth of this instability.

    Mid-gap radiograph indicates ~ 17 x radial

    compression of inner surface

    We suspect this late m = 0 feature is due to release of initial axial compression,

    combined with thickness derivative discontinuity (from double frustrum thickness

    profile) at 9 cm from mid-gap. Both the initial axial compression and the thickness

    derivative can be removed by design change.

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    20

    Left: 200 nanosec optical framing photo, axial view, of load. Inner

    diameter of opening is 8.0 cm. Photo used Xenon flash backlighting.

    Right: 200 nanosec optical framing photo, axial view, of load at

    21Qsec into implosion discharge. Inner diameter of smallest part of

    liner (most imploded part) is 1.5 cm.

    Axial view fast optical photos indicate symmetric

    implosion of inner surface of liner with inner

    diameter consistent with simulation

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    Mach2 2D-MHD simulation density contours for half height of liner at t =21 Qs and 22 Qs for double frustrum liner thickness profile from z = 0 to 6

    cm, uniform thickness 1.1 mm from z = 6 to z = 14.5 cm, thickness tapers

    from 1.10 to 1.075 mm from z = 14.5 cm to mid-gap. Electrode aperture

    radius is 4 cm.

    t = 21 Qs t = 22 Qs

    R = 4.0 cmR = 0 cm

    Z = 0 cm

    Z = 15 cm = mid-gap

    An ~ 1 mil (.025 mm) thinning of liner over central cm

    near mid-gap would explain late m = 0 feature

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    22

    Alternative liner thickness vs profiles are being

    examined via Mach2 simulations

    A family of such simulations uses an analytic profile which includes Gaussian

    thinning region a few cm from electrodes

    -

    -

    (

    E

    -

    !2

    00n/1n/1

    3zz

    exp1

    zB

    A

    zB

    ARzr

    Z0 = distance from liner midplane. Zo = 11.5 corresponds to 3.5 cm up from electrode. Z00 = 3.5

    ( is the half width at half max and E is a measure of the amplitude.

    Other parameters are defined in following table (next slide)

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    4 cm electrode inner radius

    Baseline 01 03 05 06 07

    07-1 07-2 08 08-1 09 09-1

    Contour plots show half (15 cm) of 30 cm tall, 5 cm initial outer radius, Al liner position and shape at 21

    microseconds after start of 1300 microfarad, 80 KV, 44 nanoHenry initial inductance Shiva Star discharge,

    with standard safety fuse. Initial liner thickness is 1.1 mm at mid-gap (15 cm above lower electrode).

    2D-MHD simulations indicate that use of Gaussian thinning

    regions a few cm from electrodes controls divergence of liner

    ends; variants of this are being investigated computationally

    15 cm

    mid-gap

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    Current peaked at ~ 12 megamps, at ~ 10 Qs after start of current

    rise. Insulator crowbar occurred at ~ 17 Qs, as expected.

    Normal current delivery to liner and symmetry were

    obtained for experimental Bi-frustrum profile)case

    1.40E+7

    -1.10E+7

    -7.50E+6

    -5.00E+6

    -2.50E+6

    0.00E+0

    2.50E+6

    5.00E+6

    7.50E+6

    1.00E+7

    1.25E+7

    30.000E-60.000E+0 5.000E-6 10.000E-6 15.000E-6 20.000E-6 25.000E-6

    I_corrected CCW.dat

    I_sum_arms.dat

    I_bdot1.dat

    I_bdot2.dat

    I_bdot3.dat

    MTF shot on Dec 09, 2003

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    Simulation Details: FRC Formation

    and Translation

    The FRC formation uses a flux-basedresistive diffusion model.

    The simulation includes

    Thermal diffusion Radiative emission

    After about 2 Qs, the forming FRCtranslates itself down the formation region

    into the liner implosion region. We generally use an FRC from ~ 4 Qs into the

    formation simulation to insert (interpolate) intothe imploding liner simulation.

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    FRC Formation and Injection Setup

    Formation

    And

    TranslationRegion

    Implosion

    Region

    Schematic

    (not to scale)

    axis

    axis

    Liner (not in

    formation/translation

    phase)

    Actual Block Structure

    Flux Input: 1

    Flux Input: 2

    Flux Input: 3

    Flux Input: 5

    Flux Input: 4

    m

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    FRC Formation and Translation: Te

    & Flux

    t = 0Qs t = 1Qs t = 2Qs t = 3 Qs t = 4Qs t = 5Qs

    Liner

    Implosion

    R

    egion

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    Integration of the Two Simulations

    Around 13 to 14 Qs, we interpolatethe FRC simulation data into theliner implosion simulation andcontinue the implosion.

    We can vary the time of the insertion(relative to the liner implosion) andthe age of the FRC.

    The following series of figuresshows the liner (in white), the

    temperature, and the flux lines asthe liner implodes.

    In this particular simulation, an FRC4.2 Qs old is inserted into the liner at

    13 Qs as shown at right.

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    Early Liner Evolution with Injected FRC

    t = 13 Qs t = 13.5Qs t = 14Qs t = 14.5Qs

    The downwardmomentum of theFRC tries to forceit out the bottomof the liner.

    The mirror fieldtrapped in theimploding linercaptures it, butsome mass

    escapes.

    The white line is the liner.

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    Liner Evolution with Injected FRC

    t = 15Qs t = 16Qs t = 17Qs t = 18Qs t = 19 Qs

    This combination of timings seems to captureand re-center the FRC.

    The grid motion is stopped at 17.4Qs

    The lower portion of the grid is shown in the inset

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    Late Liner Evolution with Injected FRC

    By 20Qs, theliner has com-pressed to aninner radius of0.5 cm. The temperature

    in the center ofthe FRC is over8 keV.

    There are

    temperatures ashigh as 13 keVwithin the FRC,near the axis.

    t = 19.5Qs t = 20Qs

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    Design concept for integratedFRC formation hardware with

    imploding liner compression

    hardware is evolving

    - adequate space for existing

    FRC formation load hardwaredesign in vertical orientation

    under Shiva Star center section

    with implosion load hardware

    - even more space available with

    re-positioning of FRC vacuumpump

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    Presently planned layout of FRC Formation

    Hardware Under and Around Shiva Star

    Main = single re-configured

    Shiva Star module

    PI = pre-ionization bank

    Bias, guide, and cusp banks

    in NE sextant of floor space

    rail mounted FRC formation

    train is under Shiva Star B

    transmission line when mated

    to implosion chamber

    rail mounted FRC formation

    train is withdrawn to NE

    corner of workspace for FRC

    formation experiments with

    greater formation diagnostics

    complement, allowing other

    uses of Shiva Star

    Re-configured Shiva Star module

    FRC formation load in axial orientation

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    Can Imploding Liner Magnetized Plasma

    Compression Be Made Repetitive?

    Implosion-compression of several-cm-radius shells on the 1 to 10 microsecond timescale can be used for magnetized target fusion (MTF)

    This can be done in a manner with standoff of the driver, e.g., using arrays of laseror particle beams, which enables repetitive operation (for power plants orpropulsion)

    Similar to inertial confinement fusion (ICF) drivers, but with 103 to 104 times

    slower pulses, hence easier There are also schemes for repetitive operation of magnetic pressure driven liner

    implosions (R.W. Moses et al, LA-7683-MS, 1979), and for pneumatic pressuredriven implosions of rotationally stabilized, re-usable liquid Li liners (P.J. Turchi etal, Phys. Rev. Lett. 36, 1613 (1976))

    A plasma jet spherical array compression scheme has also been proposed(Y.C.F.Thio et al, Proceedings of Second Symposium of Current Trends inInternational Fusion Research, 1999)

    Single shot versions of such implosion-compression can be done now via magneticpressure implosions, using our existing large capacitor bank

    Such single shot implosion-compression experiments can be used to investigatecritical technical issues before developing and building more expensive, repetitivedrivers