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Магнитосферные магнитные возмущения во время взрывной фазы суббури - экспериментальная проверка новой модели токового клина суббури В.А.Сергеев, Н.А.Цыганенко, М.В.Смирнов, А.В. Николаев (СПбГУ), Г. Сингер (NOAA, Boulder), В. Баумйоханн (IWF, Graz)

В.А.Сергеев, Н.А.Цыганенко , М.В.Смирнов, А.В. Николаев ( СПбГУ ) ,

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Магнитосферные магнитные возмущения во время взрывной фазы суббури - экспериментальная проверка новой модели токового клина суббури. В.А.Сергеев, Н.А.Цыганенко , М.В.Смирнов, А.В. Николаев ( СПбГУ ) , Г. Сингер ( NOAA, Boulder ), В. Баумйоханн ( IWF, Graz). - PowerPoint PPT Presentation

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  • -

    .., .., .., .. (),

    . (NOAA, Boulder), . (IWF, Graz)

  • Birkeland (1908), Bostrom (1964), Atkinson (1967), McPherron (1972 ) ground-ATS-1, Caan et (1973) lobe-ground McPherron et al. (1973) Substorm Current Wedge

    -- n*106 -

  • Horning et al., 1974 SCW ; . , 2008 . Craymosan et al.,1995 Sergeev et al., 1996 74, IGRF SCW !! ( I, . ) (87- .,1986), Tsyganenko (1997) SCW . - (? , ) SCW ; SCW

  • , , (FW) ( 6.6Re) . ;

  • Mthod: Economical Biot-Savart summation, with a possibility to flexibly deform electric current distributions within wide limits. 2. Calculate A by integrating along flow lines of J and remove singularity by assuming a variable transverse thickness of the electric current flow tube: From the very beginning, work with a vector potential, in order to keep divB=0 when spreading out the currents over a finite volume in space:so that at |r-r|>>D the field remains currrent- free, while at |r-r|
  • 3. Common problem of the Biot-Savart approach: the summation requires a very fine grid of current elements, which often results in prohibitevely slow algorithms. We overcome that difficulty by replacing many point elements by much fewer number of rectilinear segments:replacing the integralwhreby the sum: (FW) 2

  • Flow lines of spread-out model electric current, based on a loop with 245 segments and D=0.1R3/2. Volume current density is calculated as j ~ rot B, B = rot A, with derived by summation over individual segments.The model allows any arbitrary deformation of both the circuit geometry and the variable loop thickness D=D(s), without violating div B=0 and without any undesired artificial currents outside of the loop. NB: By contrast to the above method, deforming the magnetic field [Stern, 1987; Tsyganenko, 1998] conserves only div B=0, but not rot B ! (FW) 3

  • ( FW ) - 4

    IGRF + T89, - ,

    :

    Pw, Pe ; Iscw . RT - ; RCF 89; D :~ B-1/2 ,

  • SCW ( FW) YZ XZ Bz X GSM

  • INTERMAGNET

  • , Cluster (XY) \ Sergeev et al., JGR, 1996

    3-. SCW + DRP + DR

    (20-50 ) INTERMAGNET

    Iscw, Pe, Pw,

  • , , (FW) ( 6.6Re) . (Iscw, RT - , Pe, Pw ) ( Iscw, Pe, Pw )

  • 02.10.2006 ( 05:08, 06:17 07:14)

  • - Cluster-1, Cluster-2, Geotail RT, Iscw iobs-imod2 14-18RE (12 ), ; RT =15RE Bobs/Bmod SCW 1,5-2 , , PS

  • - Bx Bz (I ..) ( 14 , t=3min ) :

    (~0.7) ;

    Bobs/Bmod >1

  • 25 2006-2010 ., GOES-10,-11,-12, t=3min

    RWA . . SCW; , RT=15Re

    : - ~ 25-30 1 , . C D RWA ;

    :

    , SCW, . - 6.6 Re

  • , , (FW) ( 6.6Re) .

  • SCW 6.6Re Hobs/Hmod :

    Hobs/Hmod 1 ( 10 );

    Hobs/Hmod 2.5 ( 10 );

  • Hobs/Hmod (6.6Re) Hobs/Hmod :

    (1) (RCF);(2) ;

  • FW SCW ( R1) .

    Hobs/Hmod SCW

    ( R2)

  • Hobs/Hmod 6.6 Re Hobs/Hmod 1

  • Hobs/Hmod .Baumjohann et al., JGR 1999: . . Hobs/Hmod

  • R2 ? (BBF) - R2

    . Birn et al., JGR 1999:

  • E N D ?V. A. Sergeev, N. A. Tsyganenko, M.V. Smirnov, A.V. Nikolaev, H.J. Singer, W. Baumjohann, Magnetic effects of the substorm current wedge in a 'spread-out wire' model and their comparison with ground, geosynchronous, and tail lobe data, JGR, submitted, 2011.

  • ( FW ) - 4 :Pw, Pe ;Iscw .RCF .

    D (~ R3/2 ) .

    SCW = IGRF + T89

  • (Bx, By, Bz ):

  • T89 model field lines for FAC routeRegulate stretching by 1 parameter (RC) Main parameters : I, Pw,Pe, R RT to be determined later (~ 15Re)

    Some further details

  • SCW (T09SCW) Bx Z GSM (X = -15RE , Y = 0)

  • 2006.09.27 09:28 10:00, 2 : - GSM ( ); - ; - .

  • TW09 . Sergeev et al., JGR, 1996

    3-. SCW + DRP + DR

    (20-50 ) INTERMAGNET

    Iscw, Pe, Pw,

  • , : 14-18RE ( Cluster Geotail), ; , 1.5-3.0 ; (TW09) , 8-18RE, TW09 ; Bx Bz ~1.5 , , .

    *****