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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) . ;
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 , , .
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