ilya silin
DESCRIPTION
Anomalous resistivity due to lower-hybrid drift waves. Results of Vlasov-code simulations and Cluster observations. Ilya Silin. Department of Physics University of Alberta [email protected]. - PowerPoint PPT PresentationTRANSCRIPT
Anomalous resistivity due to lower-hybrid drift waves.
Results of Vlasov-code simulations and Cluster observations.
Ilya Silin
Department of Physics
University of Alberta
Cluster results are courtesy of
A. Vaivads and Yu. KhotyaintsevIRFU,Uppsala, Sweden
K.-H. Glaßmeier TU Braunschweig
and E. PanovMPI für Sonnensystemforschung
Outline
• Thin current sheets and reconnection
• Instabilities of current sheets
• General perturbation theory
• Vlasov-code simulations
• Cluster measurements at magnetopause
• Sheared magnetopause models
Thin current sheets: dynamical regions
Magnetotail
MagnetopauseSolar corona
Current sheets - regions of plasma accumulation in magnetic “traps”.
Magnetic reconnection
E. Priest, A&A, 2001
C. T. Russell, Adv. Sp. Res., 2002
Thin current sheets: separation of regions of oppositely directed magnetic field
Biot-Savart law:
or
jc
B 4
yx j
cz
B 4
Instabilities of thin current sheets
P. Yoon et al., Phys. Plasmas, 2002
General perturbation theory
Vlasov equation 0)(1
v
fBv
cE
m
e
r
fv
t
f j
j
jjj
Wave-like perturbations
BBB
EEE
fff jjj
0
0
0
Perturbations of density and current
jj
jjj
vfdvej
vdfe
0 BEf j
jj ff ~
After ensemble averaging
General perturbation theory
v
f
c
BvE
m
e
t
f
v
fBv
cE
m
e
r
fv
t
f j
j
j
an
jj
j
jjj
0
0000 )(
1
Collision term integrated over velocities
Effective anomalous collision frequency
c
BjBjEvmn
tzjxxjz
jyan
jyjj
,,
,
c
BjBjE
vmnvmn
tvmnzjxxjz
jy
jyjjanjyjj
jyjj
eff
,,
,
,
,
11
Normalized to LH frequency
Anomalous collision rates
CeCiLH
Quasi-linear estimate (Davidson and Gladd, Phys. Fluids, 1975)
LHeff
eBLH
peeff Tnk
E
8
22
)/( 2nem effean
Anomalous resistivity
Vlasov-code simulations• initial equilibrium - Harris current sheet (Harris, Nuovo Cim., 1962)
• normalization
• distribution function moments
vdfvej
vdfe
ei
Veijei
V
eieij
ei
3,
,,
3,
,,
NrvddfRV
ei 33
,
,
Vlasov-code simulations• equations for potentials
• Coulomb gauge
• equations for electromagnetic fields
• Vlasov equation
jct
A
cA
41
4
2
2
2
0 A
AB
t
A
cE
1
0)(1 ,
,
,,,
v
fBv
cE
m
e
r
fv
t
f ei
ei
eieiei
tc
1
Vlasov-code simulations
Simulation results: lower-hybrid drift (LHD) waves
LHD waves grow at the edges of the current sheet and gradually penetrate towards the central plane.
Simulation results: kink and sausage modes
The interaction of LHD waves from the edges can trigger either global kink or sausage eigen-mode.
Simulation results: effective collision ratesions electrons
2D simulations with mi/me=100
electrostatic part
electromagnetic part
Simulation results: effective collision rates3D simulations with mi/me=16
yyean Ej 5.0
Bale et al., GRL (2002): yyean Ej 005.0
Our Vlasov-simulations:
Cluster magnetopause encounter March 30th 2002, 13:11:46
X
ZZ
Y
Cluster measurements at magnetopause
tangential magnetic fields
electric fields
normal magnetic field
LHD electric fields
plasma density
tangential magnetic fields
electric fields
average momentum
density fluctuations
electric field fluctuations
p1049 28-Nov-2004 23:04:23 Vmp=31.25*[-0.94 -0.21 -0.25]km/s, dt=[0.00 1.61 2.81 -0.50]s L=[-0.25 -0.05 0.97]N=[0.94 0.21 0.25]M=[-0.22 0.98 0.00]f
filter=[20 100].
-100
0
100
BL [
nT]
C1 C2 C3 C4
a)
0
20
40
60
NV
ps [
cc]
sc2 b)
-100
-50
0
50
En [
mV
/m]
sc2 c)
-5
0
5
dn [
cc]
sc2
d)
-100
-50
0
50
dE [
mV
/m]
sc2 e)
.6 .8 13:11:46.0 .2 .4 -50
0
50
100
dn d
E [
cc m
V/m
] sc
2
30-Mar-2002
f) product of density and electric field fluctuations
Cluster: νeff due to e/s fluctuations
Hzeff 70~ HzfLH 60~
Cluster: νeff due to e/m fluctuations
magnetic field fluctuations
current fluctuations
product of current and magnetic field fluctuations
-2
-1
0
1
2
B [
nT
]
-2
-1
0
1
2
j [u
A/m
2 ]
0
5
10
15
20
25
jxB
/e [
cc m
V/m
]
.6 .8 13:11:46.0 .2 .4 0
5
10
15
20
25
jxB
/e [
cc m
V/m
]
30-Mar-2002
Hzeff 30~
Observations of the magnetopausemagnetic field component hodographs
in local magnetopause frame:
BL and BM – tangential components, BN – normal component
(from Cluster s/c1 06.16.02, 00:54-00:58 and 01.15.03 00:30-01:30, courtesy of K.-H. Glaßmeier and E. Panov)
Magnetopause current sheet model
BxB
ByB
vxvthi
vyvthi
magnetic field hodograph
ion drift velocity hodograph
t i
zLz
BzB
LHD waves at the sheared magnetopause
zLz
BzB
Conclusions• The effective collision frequency calculated from
results of numerical simulations and Cluster measurements is of the order of νeff ~ ΩLH
• Anomalous collisions become significant only when LHD waves reach a non-linear phase
• Contributions to νeff from e/s and e/m fluctuations are comparable
• The dissipation due to microscopic kinetic effects becomes significant for large-scale processes, e.g., reconnection at Earth magnetopause
• However, for more realistic magnetopause configuration, the situation is still not quite clear