magnetic structures in electron-scale reconnection domain ilan roth space sciences uc berkeley, ca...
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Magnetic Structures in Electron-scale Reconnection Domain
Ilan Roth
Space Sciences
UC Berkeley, CA
Thanks: Forrest Mozer
Phil Pritchett
Dynamical Processes in Space Plasmas
Eyn Bokkek, Israel, 10-17 April 2010
Fundamental plasma processes with global
implications may occur in a narrow layer
Magnetic Reconnection
Magnetic shears - electron dominated region
What can we learn about
electron scale structures without (full) simulations?
Symmetric Configuration à la texbook cartoon
Classical Symmetric Crossing à la observations- Mozer, 2002
Hall
Hall
reconnect
reconnect
Collective plasma scales determine the different (nested) layers:
Outer: - Hall effect – ions decouple from B
Intermediate: e- inertia (pressure)
Inner: break(s) the e-
Innermost: frozen-in condition
Main purpose: assessing the non ideal effects of Ohms Law
Environment: electron (current) velocity >> mass velocity
ee cd /
ii cd /
eie dmm )/(eieie dmmdd 2/12 )/(/
4)
8(
2 )B(BBJv
Bp
cp
dt
d
Two Fluid: coupling (B,v)
“Ion” fluid
Electron fluid
cne
p
necdt
d
e
m eee BvEj
BJv
Sheared field, Inhomogeneous Plasma
General coupling between
Shear Alfven
Compressional Alfven
Slow Magneto-Acoustic
modified on short scales by
(mainly) electron effects
Two (extreme) approaches
• Lowest approximation of the electron dynamics + follow ion dynamics
• Lowest approximation of the ion dynamics + follow electron dynamics
A. Faraday and Ohm’s law couple
magnetic and velocity fields
MHD:
Magnetic field is frozen in the fluid drift
}{ BVB t
jΒVE c/
EB ct
Magnetic field – fictitious diagram of lines in R3
satisfying specific rules. MHD – approximate description of magnetic field motion in a plasma fluid.
Knot - closed loop of a non-self-intersecting curve, transformed via continuous deformation of R3 upon itself, following laws of knot topology - pushed smoothly in the surrounding viscous fluid, without intersecting itself (stretching or bending).
MHD field evolves as a topological transformation of a knot. MHD dynamics forms equivalent knot configurations with a set of knot invariants.
All KNOT deformations can be reduced to a sequence of Reidemeister “moves”: (I) twist (II) poke , and (III) slide.
Type 1 Type 2
Type 3
Knot topology described through knot diagrams
Reidemeister moves
Reidemeister moves preserve several invariants of the knot or link represented by their diagram - topological information.
MHD invariants: (cross) helicity, generalized vorticity, Ertel,…
Every knot can be uniquely decomposed as a knot sum of prime knots, which cannot themselves be further decomposed - Schubert (1949)
Prime knots
Characterization based on crossing number – Tait 1877
Flux-rope is a KNOT
MHD Turbulence forms a LINK- Collection of knots
Reconnection is NOT a KNOT: it forms a KNOT SUM
HELIOSPHERE
MHD (KNOT) can be broken via several physical processes
Various physical regions
Reconnection: topological transition
Diffusion: violation of frozen–in condition
Dissipation: conversion of em energy
(no consensus on definitions)
Parallel electric field is observed in tandem with density gradients
Localized electric field over
scale ≤ de=c/ωe – electron inertia effect?
Mozer +, 2005
Electron diffusion region: 0 BvE e
filamentary currents on scale ≤ de=c/ωe – dissipation region due to electron inertia effect?
ELECTRON PHYSICS COVERS LARGE SPATIAL SCALES.
Asymmetric Simulation – Pritchett, 2009
Violation of electron frozen-in condition
Elongated Electron Diffusion regions
?0/ vB mce
Magnetic field vs Electron Vorticity vs dissipation
B. Faraday and Ohm’s law couple
magnetic and velocity fields
eMHD:
Generalized vorticity field is frozen in
the electron fluid drift
jpnm
udt
d
e
mBu
cE e
11
}{EB t
uBGGuG
)/(};{ emct
vorticity
eMHD: Electron fluid:
}{ GuG t
MHD: “Ion” fluid
}{ BVB t
jBBB
cddt ee })1(){(]1[ 2222
coeffHallenc
une
4/
BuJ
Electron inertia Hall ee cd /
Homogeneous, incompressible electron fluid
BuBG )1()/( 22 edemc
Magnetic field slips with respect to the electron fluid
Generalized vorticity G is frozen in the electron drift u
Inhomogeneous electron fluid
Bnxn
Bxen
cu
Bc
uxenJ
oo
o
/)(]
)(4[
4)(
pe
c
t
)/1(})/{( GBG
ee cd /
ln))(/(])/(1[ 222 BBG ee dd
nxnx o /)()(
)1(
)()(
22edk
kBkk
Linear homogeneous
infinite plasma waves
Whistler branch
Generalized Vorticity – Inhomogeneous fluid
A. Incompressible Homogeneous Plasma; [n(x)=no]
zzyyo eBexBxB )()('; yoo BUUenJ
uenjlinearized o:
zyxe
xyxyze
bxGkbdx
dkd
bxBbdx
dkxBb
dx
dkd
)()](1[
)())(()](1[
22
222
''2
22
2
222
Electron inertia effect is manifested on the small spatial scale
Inclusion of ion dynamics in the limit
zyxe
xyxyze
bxBkbdx
dkd
bxBbdx
dkxBb
dx
dkd
)()](1[
)())(()](1[
22
222
''2
22
2
222
eMHD limit:
yzixxe
x"
xyi
ze
BbkdkVbdγτ
bBbBγτ
db)ετ/γ(d
y
][1[
][]11[
222
222222
1)/( 222 sc
Coupling of shear Alfven and compressional Alfven
im
Mirnov+, 2004
2/12/11 ~/;~~ iiiia mcdmLV
Eigenmodes: two components of the magnetic field
Unstable mode in a whistler regime
Califano, 1999
By=tanh(x/L)
de/L=1
bx
bz
'2222
''222
22
~)(]1[
)(])1(1[
Bn
ndikbxGkbd
bBbxBbd
ezyxe
xyxyze
ce
Increase in the effective electron skin depth
Compressibility - “Guiding” field: enhance the electron inertia effect
B. Compressible Homogeneous Plasma
nnnUnunejlinearized oo~;)~(:
C. Inhomogeneous, compressible plasma
zzyyo eBexBxB )()(
')](/[)();()()( yBx
oxUxUx
oenx
oJ
nxnx oo /)()(
o
yezyxeo
ozx
xyxyze
ceo
B
n
ndikbxGkbdx
dxxdnkbiiUbd
bBbBbdx
'2222
2
''222
22
~)(])([
)/)()()(/1(
])1()([
Density dips enhance the electron inertia effect
D. Inhomogeneous, compressible plasma – generalized configuration
zzyyo exBexBxB )()()(
')](/[)(;')](/[)(z
Bxo
xUyBx
oxU yz
nnnxnx oo /~~;/)()(
zyxeo
xyxyzozzee
ceo
bxGkbd
bBbBbBBdx
ddd
)(][
})]/1(1[{
222
''22'22
22
3D structure may enhance the electron inertia effect
E. Kinetic, incompressible, inhomogeneous plasma
xyexI
Rz
Ithe
zI
Rexex
I
IR
th
bdbZ
Zb
Zkv
k
dx
dd
bZ
Zkdbdb
Z
ZZ
kv
''22
2
22
222222
)])/(
1(1[
Attico +, 2002
SUMMARY
A. MHD satisfies the axioms of knot theory – both evolve preserving various invariants. Knot sum is equivalent to violation of frozen-in condition.
B. Density gradients/dips, compressibility, and thermal effects may have a significant effect on the electron vorticity, which determines the slipping of the magnetic field with respect to the electrons. These effects modify the structure of the magnetic field on the short-scale, forming current filaments, parallel electric fields, which violate the frozen-in condition and contribute to electron heating. These regions are ubiquitous and are observed outside of the x-points in the reconnection domain.