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Overview of JET Asymmetrical binacci, Francesco Maviglia · 2014. 7. 24. · asimov “Overview of...

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32
TSD meeting PPPL 9-11 July 2014 S Gerasimov “Overview of JET asymmetrical disruptions” 1 /32 Overview of JET Asymmetrical Disruptions Sergei Gerasimov, CCFE Acknowledgements to: - Tim Hender, Leonid Zakharov, James Morris, Valeria Riccardo, Maximus Tsalas, Matteo Baruzzo, Fabio Villone, Raffaele Albanese, Guglielmo Rubinacci, Francesco Maviglia . Theory and Simulation of Disruptions Workshop Princeton Plasma Physics Laboratory July 9- 11, 2014
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    Tim

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    Tim

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    1

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    Oct.

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    T P

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    CPS14.352-11c

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    Tim

    e (

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    ruptions

    IL-

    wall,

    w/o

    MG

    I

    C-

    wall,

    w/o

    MG

    I

    IL-

    wall,

    MG

    I

    C-

    wall,

    MG

    I

  • TS

    Dm

    ee

    tin

    g P

    PP

    L9

    -11

    Ju

    ly 2

    01

    4

    S

    Ge

    rasim

    ov “O

    ve

    rvie

    w o

    f J

    ET

    asym

    me

    tric

    al d

    isru

    ptio

    ns”

    2

    6/3

    2

    0.4

    0.3

    0.2

    0.1 0

    0.5

    -5

    -4-

    3-

    2-

    10

    12

    34

    56

    78

    Density of occurances

    68

    3 d

    isru

    ptio

    ns in

    th

    e r

    an

    ge

    80

    18

    1-8

    59

    78

    , IL-

    wa

    ll

    A =

    d

    t >

    0.2

    5m

    s

    > 0

    .5%

    , 2

    14

    sh

    ots

    > 1

    .0%

    , 2

    13

    sh

    ots

    > 2

    .0%

    , 2

    07

    sh

    ots

    > 5

    .0%

    , 11

    3 s

    ho

    ts

    Ap

    a

    sym

    ∫Ap

    a

    sym

    N t

    urn

    s

    CPS14.352-18c

    Nu

    mb

    er

    of

    Ro

    tati

    on

    s

    Fo

    rce d

    yn

    am

    ic a

    mp

    lifi

    cati

    on

    :

    1.

    Ro

    tati

    on

    occu

    rs a

    t n

    ear

    a

    reso

    nan

    ce f

    req

    uen

    cy

    2.

    Mo

    re t

    hen

    2 p

    eri

    od

    s t

    ake

    pla

    ce, see J

    ET

    data

    Re

    so

    na

    nce

    Re

    so

    na

    nce

    On J

    ET, ro

    tation is m

    ost

    com

    monly

    seen in

    the e

    lectr

    on d

    rift

    direction

    •F

    or

    JE

    T t

    he

    du

    ratio

    n o

    f th

    e r

    ota

    tio

    n is s

    ho

    rt

    co

    mp

    are

    d t

    o r

    eso

    na

    nce

    pe

    rio

    d o

    f th

    e v

    esse

    l

    (∼1

    /(1

    4–

    17

    Hz))

    , a

    nd

    so

    dyn

    am

    ic a

    mp

    lific

    ation

    is n

    ot

    an

    issu

    e.

    •F

    or

    ITE

    Rth

    e s

    itu

    atio

    n c

    an

    be

    re

    ve

    rse

    d (

    the

    du

    ratio

    n o

    f ro

    tatio

    n is g

    rea

    ter

    tha

    n t

    he

    me

    ch

    an

    ica

    l re

    so

    na

    nce

    pe

    rio

    d)

    ma

    kin

    g t

    his

    an

    issu

    e.

  • TS

    Dm

    ee

    tin

    g P

    PP

    L9

    -11

    Ju

    ly 2

    01

    4

    S

    Ge

    rasim

    ov “O

    ve

    rvie

    w o

    f J

    ET

    asym

    me

    tric

    al d

    isru

    ptio

    ns”

    2

    7/3

    2

    Ou

    tlin

    e

    �D

    iag

    no

    sti

    cs

    �S

    ign

    al

    pro

    ce

    ss

    ing

    �D

    ata

    ba

    se

    �S

    ide

    wa

    ys

    fo

    rce

    , im

    pu

    lse

    an

    d v

    es

    se

    l d

    isp

    lac

    em

    en

    t

    �R

    ota

    tio

    n

    �O

    uts

    tan

    din

    g i

    ss

    ue

    s

    �S

    um

    ma

    ry a

    nd

    dis

    cu

    ssio

    n

  • TS

    Dm

    ee

    tin

    g P

    PP

    L9

    -11

    Ju

    ly 2

    01

    4

    S

    Ge

    rasim

    ov “O

    ve

    rvie

    w o

    f J

    ET

    asym

    me

    tric

    al d

    isru

    ptio

    ns”

    2

    8/3

    2

    As

    ym

    me

    try o

    f P

    olo

    ida

    l L

    oo

    p V

    olt

    ag

    es

    Uniform

    rota

    tion –

    polo

    idal

    voltage a

    sym

    metr

    y follo

    wed

    by t

    oro

    idal curr

    ent asym

    metr

    y

    Tripped (

    locked)

    mode –

    rise a

    nd

    decay o

    f polo

    idal voltage

    asym

    metr

    y (

    ~ p

    olo

    idal curr

    ent ?)

    -0

    .5

    -1

    .0

    -1

    .5

    0.1 0

    -0

    .1 2 1 15

    10 50

    -1

    -2 00

    00

    .01

    0.0

    20

    .03

    -0

    .01

    0.0

    4

    Tim

    e (

    s)

    JE

    T P

    uls

    e N

    o:

    72

    92

    6

    CPS14.352-15c

    Ip (MA)

    I p5

    - I p

    1

    Vd

    l5 -

    Vd

    l1

    ∆Ip (MA) ∆Vdl (V) ϕ (π)

    Oct.

    1O

    ct.

    3O

    ct.

    5O

    ct.

    7

    -1

    .0

    -2

    .00

    .1 0

    -0

    .1

    -0

    .2 1 2 00 -1

    -2

    -20

    0.0

    20

    .03

    0.0

    10

    .04

    Tim

    e (

    s)

    JE

    T P

    uls

    e N

    o: 7

    01

    00

    CPS14.352-16c

    Ip (MA)

    I p5

    - I p

    1

    Vd

    l5 -

    Vd

    l1

    ∆Ip (MA) ∆Vdl (V) ϕ (π)

    Oct. 1

    Oct. 3

    Oct. 5

    Oct. 7

  • TS

    Dm

    ee

    tin

    g P

    PP

    L9

    -11

    Ju

    ly 2

    01

    4

    S

    Ge

    rasim

    ov “O

    ve

    rvie

    w o

    f J

    ET

    asym

    me

    tric

    al d

    isru

    ptio

    ns”

    2

    9/3

    2

    Wh

    at

    is t

    he R

    easo

    n f

    or

    Po

    loid

    al L

    oo

    p V

    olt

    ag

    e

    Asym

    metr

    y?

    Bt

    1.

    Pla

    sm

    a r

    adia

    lly s

    hifte

    d b

    ecause o

    f

    the m

    /n=

    1/1

    (3D

    effect)

    ;

    2.

    Leads t

    o p

    lasm

    a c

    ontr

    action a

    nd

    expansio

    n (

    toro

    idal flux

    conserv

    ation);

    3.

    Pla

    sm

    a c

    ontr

    action /

    expansio

    n

    leads t

    o v

    ariation o

    f to

    roid

    al flux

    insid

    e t

    he v

    essel;

    4.

    Variation o

    f to

    roid

    al flux c

    reate

    s

    the p

    olo

    idal voltage w

    hic

    h

    genera

    tes t

    he p

    olo

    idal vessel

    curr

    ent.

    Sim

    ilar

    mo

    de

    l ca

    n b

    e a

    pp

    lied

    to

    po

    loid

    al lo

    op

    vo

    lta

    ge

    be

    ha

    vio

    ur

    du

    rin

    g E

    LM

    s(2

    D e

    ffe

    ct)

    wh

    ere

    (1

    .)e

    ve

    nt is

    be

    ta d

    rop

    an

    d r

    eco

    ve

    ryR

  • TS

    Dm

    ee

    tin

    g P

    PP

    L9

    -11

    Ju

    ly 2

    01

    4

    S

    Ge

    rasim

    ov “O

    ve

    rvie

    w o

    f J

    ET

    asym

    me

    tric

    al d

    isru

    ptio

    ns”

    3

    0/3

    2

    Vessel

    Po

    loid

    al C

    urr

    en

    t In

    du

    ced

    by E

    LM

    -

    CarM

    a0N

    L C

    od

    e S

    imu

    lati

    on

    *

    Verify

    ing t

    he C

    arM

    a0N

    L 3

    D J

    ET

    vessel m

    odel

    �T

    he d

    ecay t

    ime o

    f polo

    idal curr

    ents

    in t

    he v

    essel m

    odel is

    slig

    htly less (

    30 m

    s)

    than in J

    ET

    estim

    ation f

    rom

    TF

    variation (

    38-3

    9 m

    s);

    �N

    ext

    ste

    p –

    sim

    ula

    te t

    oro

    idal flux v

    ariation d

    uring t

    he E

    LM

    ;

    �N

    ext

    ste

    p –

    quasi 3D

    asym

    metr

    y s

    imula

    tion d

    uring

    dis

    ruption.

    *F

    ab

    io V

    illo

    ne

    , F

    ran

    ce

    sc

    o M

    av

    igli

    a,

    Ra

    ffa

    ele

    Alb

    an

    ese

    , G

    ug

    lie

    lmo

    Ru

    bin

    ac

    ci

    9

    10 5

    0.1 0

    -0.1

    -0.20

    14.1

    614.2

    014.2

    414.1

    2

    V

    Tim

    e (

    s)

    CPS14.352-23c

    Dα (a.u.)

    Vdl1

    Vdl5

  • TS

    Dm

    ee

    tin

    g P

    PP

    L9

    -11

    Ju

    ly 2

    01

    4

    S

    Ge

    rasim

    ov “O

    ve

    rvie

    w o

    f J

    ET

    asym

    me

    tric

    al d

    isru

    ptio

    ns”

    3

    1/3

    2

    Ou

    tlin

    e

    �D

    iag

    no

    sti

    cs

    �S

    ign

    al

    pro

    ce

    ss

    ing

    �D

    ata

    ba

    se

    �S

    ide

    wa

    ys

    fo

    rce

    , im

    pu

    lse

    an

    d v

    es

    se

    l d

    isp

    lac

    em

    en

    t

    �R

    ota

    tio

    n

    �O

    uts

    tan

    din

    g i

    ss

    ue

    s

    �S

    um

    ma

    ry a

    nd

    dis

    cu

    ss

    ion

  • TS

    Dm

    ee

    tin

    g P

    PP

    L9

    -11

    Ju

    ly 2

    01

    4

    S

    Ge

    rasim

    ov “O

    ve

    rvie

    w o

    f J

    ET

    asym

    me

    tric

    al d

    isru

    ptio

    ns”

    3

    2/3

    2

    Su

    mm

    ary

    an

    d D

    iscu

    ssio

    n

    •P

    las

    ma

    cu

    rre

    nt

    as

    ym

    me

    trie

    s d

    uri

    ng

    cu

    rre

    nt

    qu

    en

    ch

    an

    d h

    en

    ce

    sid

    ew

    ays

    fo

    rce

    s c

    an

    be

    su

    cc

    es

    sfu

    lly

    mit

    iga

    ted

    by M

    GI

    –1

    00

    % (

    23

    2 s

    ho

    ts)

    su

    cc

    es

    s s

    o f

    ar;

    •M

    ult

    i-tu

    rn I

    pa

    sym

    me

    try r

    ota

    tio

    n i

    n b

    oth

    to

    roid

    al

    dir

    ec

    tio

    ns

    ha

    s b

    ee

    n o

    bs

    erv

    ed

    on

    JE

    T t

    ha

    t c

    an

    le

    ad

    to

    res

    on

    an

    ce

    co

    nd

    itio

    n o

    n I

    TE

    R;

    •J

    ET

    ra

    dia

    l v

    es

    se

    l d

    isp

    lac

    em

    en

    t c

    orr

    ela

    tes

    wit

    h

    sid

    ew

    ays

    fo

    rce

    dir

    ec

    tio

    na

    l im

    pu

    lse

    , w

    hic

    h i

    s

    es

    tim

    ate

    d o

    nly

    fro

    m m

    ag

    ne

    tic

    dia

    gn

    os

    tic

    .


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