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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]

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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 Presentation

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Page 1: Ilya Silin

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]

Page 2: Ilya Silin

Cluster results are courtesy of

A. Vaivads and Yu. KhotyaintsevIRFU,Uppsala, Sweden

K.-H. Glaßmeier TU Braunschweig

and E. PanovMPI für Sonnensystemforschung

Page 3: Ilya Silin

Outline

• Thin current sheets and reconnection

• Instabilities of current sheets

• General perturbation theory

• Vlasov-code simulations

• Cluster measurements at magnetopause

• Sheared magnetopause models

Page 4: Ilya Silin

Thin current sheets: dynamical regions

Magnetotail

MagnetopauseSolar corona

Current sheets - regions of plasma accumulation in magnetic “traps”.

Page 5: Ilya Silin

Magnetic reconnection

E. Priest, A&A, 2001

C. T. Russell, Adv. Sp. Res., 2002

Page 6: Ilya Silin

Thin current sheets: separation of regions of oppositely directed magnetic field

Biot-Savart law:

or

jc

B 4

yx j

cz

B 4

Page 7: Ilya Silin

Instabilities of thin current sheets

P. Yoon et al., Phys. Plasmas, 2002

Page 8: Ilya Silin

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 ~

Page 9: Ilya Silin

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

Page 10: Ilya Silin

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

Page 11: Ilya Silin

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

,

,

Page 12: Ilya Silin

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

Page 13: Ilya Silin

Vlasov-code simulations

Page 14: Ilya Silin

Simulation results: lower-hybrid drift (LHD) waves

LHD waves grow at the edges of the current sheet and gradually penetrate towards the central plane.

Page 15: Ilya Silin

Simulation results: kink and sausage modes

The interaction of LHD waves from the edges can trigger either global kink or sausage eigen-mode.

Page 16: Ilya Silin

Simulation results: effective collision ratesions electrons

2D simulations with mi/me=100

electrostatic part

electromagnetic part

Page 17: Ilya Silin

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:

Page 18: Ilya Silin

Cluster magnetopause encounter March 30th 2002, 13:11:46

X

ZZ

Y

Page 19: Ilya Silin

Cluster measurements at magnetopause

tangential magnetic fields

electric fields

normal magnetic field

LHD electric fields

plasma density

Page 20: Ilya Silin

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~

Page 21: Ilya Silin

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~

Page 22: Ilya Silin

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)

Page 23: Ilya Silin

Magnetopause current sheet model

BxB

ByB

vxvthi

vyvthi

magnetic field hodograph

ion drift velocity hodograph

Page 24: Ilya Silin

t i

zLz

BzB

LHD waves at the sheared magnetopause

zLz

BzB

Page 25: Ilya Silin

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