Upload
clare-bennett
View
24
Download
1
Tags:
Embed Size (px)
DESCRIPTION
The Structure of Thin Current Sheets Associated with Reconnection X-lines. Marc Swisdak The Second Workshop on Thin Current Sheets April 20, 2004. Collaborators. U. of Maryland. J. Drake M. Shay J. McIlhargey B. Rogers A. Zeiler. UMBC. Dartmouth College. MPP-Garching. z. y. x. - PowerPoint PPT Presentation
Citation preview
The Structure of Thin Current Sheets Associated with Reconnection X-lines
Marc Swisdak
The Second Workshop on Thin Current Sheets
April 20, 2004
Collaborators
• J. Drake• M. Shay
• J. McIlhargey
• B. Rogers
• A. Zeiler
U. of Maryland
Dartmouth College
MPP-Garching
UMBC
BguideJ
Breconn
xy
zSimulation:
Reconnecting field: xInflow velocity: yGuide field/Current: z
p3d Details
• Relativistic PIC code• Boris algorithm for particles• Trapezoidal leapfrog for fields
• Multigrid for Poisson’s equation• MPI parallelization• Biggest runs:
• 512x256x256• 2048 processors• ~109 particles
• How we cheat:• me/mi large• c/cA small
• Also:• Double Harris sheet• Periodic BCs
The Point
Q: At what strength does the guide field become important?
A: Bg 0.1 B0
zJx
y
y
No Guide Field: Overview
0
0
Box size: 6.4 6.4 / 20
Guide field: 0 / 100
Grid: 1024 1024 / 10
Background Density: 0.2
2D Simulation
i A
i e
i e
d c c
B m m
T T
n
zJ
x
y
Development of Bifurcation
1Total time: 4.5 ci
Temperature
y
y
y
y
x
x
x
xxT yyT
zzT
Velocity Distributions
yv
zv
@ x-line: Beams are due to Speiser figure-8 orbits
@ bifurcation: Multiple peaks from two beams
Balancing the Reconnection Electric Field
,,
1(
)
)
)
1
(
( e y
z ex
e ez e
ze
y e
xz
y
z eex ey
x
zm v v vv
PP
E v B
ne z
ve t
Bc
z
y
v
x
Ideal MHD
Pressure tensor
Electron Inertia
1( )ex y ey xv B v B
c
e ezm v
e t
,,1( )e yze xz PP
ne z z
* zE
( )e ez ezex ey
m v vv v
e x y
Balancing the Reconnection Electric Field
zJx
y
y
Guide Field: Bg=1B0
• Current sheet not bifurcated• Electrons magnetized at the x-line
• Canted separtrices• E|| interacting with Bg
T T
yv
Temperature, Bg=1
1( )ex y ey xv B v B
c
e ezm v
e t
,,1( )e yze xz PP
ne z z
* zE
( )e ez ezex ey
m v vv v
e x y
Balancing the Reconnection Electric Field
Guide Field Criterion
• What is the minimum Bg so that the e- excursions are less than de?
in0
0
0.1vv 0.1
( / )Ae
L gce ce g pe
cB B
B B
edid Aec Ac
0.1 Aec
0.1 AcReconnection Rate:
0
z
A
cE
t c B
ExBv
~ 0.1Ac
X-line Structure: Bg = 0, 0.2, 1
Temperature, Bg=0.2T T
yv
Off-Diagonal Pressure Tensor, Pyz
Why is this important? Development of x-line turbulence.Why does it happen? Bg means longer acceleration times.
1gB
0gB
Ions
0.2gB
X-line Distribution Functions
zv
Conclusions
• Bg ~ 0.1B0 is enough to influence the structure of x-lines.– Affects: Flow geometries, separatrices, particle
orbits (temperatures), particle energization, development of turbulence (?)
– Doesn’t affect: Reconnection rate, breaking of frozen-in condition
• Implication: Anti-parallel reconnection is rare in real systems. Most reconnection is component reconnection
xxT
yyT
zzT
Cut Through the X-line
Reconnection Rate & Guide FieldR
econ
nect
ed F
lux
Time
1gB
0gB
Anti-parallel reconnection
Guide field reconnection
Why the difference?
Within the diffusion region electrons are unmagnetized & execute wandering orbits.
Electrons are always magnetized and are not heated.
Tfinal
Tinit
1( )ex y ey xv B v B
c
,,1( )e yze xz PP
ne z z
( )e ez ez ezex ey
m v v vv v
e t x y
zE
Generalized Ohm’s Law
The final three terms become important at different scales:
i c/pi s, ei e
What terms does MHD neglect?
1 1 e eie
nec
m d
e dtc ne + J B
vE B J P
v��
Ideal MHD
Pressure tensorResistive MHD
Hall term Electron Inertia
3D Reconnection with Guide Field
zJy
x0
9
Box size: 4 2 1 / 20
Guide field: 5 / 100
Number of Particles: (10 )
i A
i e
d c c
B m m
O
z
zJ
zE
z
y
vez
Buneman Instability
• Electron-ion two-stream instability. If the distribution functions do not (roughly) overlap then the system is unstable.
1/3 ( / )e i pem m
d/vpek IonsElectrons
~J
3D Reconnection w/o Guide Field
vez
• Initial turbulence (LHDI) disappears as reconnection strengthens.• X-line shows no sign of instability at late times.
zJ
early
late
Temperature
y
y
y
y
x
x
x
xxT yyT
zzT
Temperature, Bg=0.2T T
T T
yv
Temperature, Bg=1
Dissipation mechanism• What balances Ep during guide field reconnection?
• Scaling with electron Larmor scale suggests the non-gyrotropic pressure can balance Ep (Hesse, et al, 2002).
4 pe
2
dJz
dtE z
1
c(v e
B )z
1
ne(
p e )z
Bz=0 Bz=1.0
y y
Transition from anti-parallel to guide field reconnection
• Structure of non-gyrotropic part of the pressure tensor, Pyz
– Remove gyrotropic portion– Significant changes for Bz0=0.1
Bz0=0 Bz0=1.0Bz0=0.1