56
Current sheets formation along magnetic separators in 3d Dana Longcope Montana State University Thanks: I Klapper, A.A. Van Ballegooijen NSF-ATM

Current sheets formation along magnetic separators in 3d

  • Upload
    inge

  • View
    41

  • Download
    0

Embed Size (px)

DESCRIPTION

Current sheets formation along magnetic separators in 3d. Dana Longcope Montana State University. Thanks: I Klapper, A.A. Van Ballegooijen NSF-ATM. The Coronal Field. 8/11/01 9:25. 1 MK plasma (TRACE 171A). Corona : complex inter-connections between sources. B z =0. Lower boundary : - PowerPoint PPT Presentation

Citation preview

Page 1: Current sheets formation along magnetic separators in 3d

Current sheets formation along magnetic separators in 3d

Dana Longcope

Montana State University

Thanks: I Klapper, A.A. Van BallegooijenNSF-ATM

Page 2: Current sheets formation along magnetic separators in 3d

The Coronal Field1 MK plasma(TRACE 171A)

Magnetic field @ photosphere (MDI)

8/10/01 12:51

8/11/01 9:25

Lower boundary: Bz confined to source regions

Corona: complexinter-connectionsbetween sources

Bz=0

Page 3: Current sheets formation along magnetic separators in 3d

The Coronal Field

8/10/01 12:51 8/11/01 17:39

8/11/01 9:25 1 MK plasma(TRACE 171A)

Magnetic field @ photosphere (MDI)

Evolution: lowerboundary changesslowly

(+30 hrs)

Page 4: Current sheets formation along magnetic separators in 3d

Outline

I. Lowest energy magnetic field contains current sheets localized to separators (Flux-Constrained Equilibrium)

II. Boundary motion drives field singular equilibrium via repeated Alfven wave reflection

Page 5: Current sheets formation along magnetic separators in 3d

I. EquilibriumForce-Free Equilibrium: Minimizes Mag. Energy*

xdWz

32

0

||2

1)}({

AxA

Constraints: (minimize subject to…)• None

• Ideal motion (line-tied to boundary)

AAA 0 B

BξA 0)( BB

potential

general FFF

*subject to BC: Bz(x,y,0) = f(x,y)

Page 6: Current sheets formation along magnetic separators in 3d

A new type of constraint

Boundary field Bz(x,y,0) = f(x,y): assume discrete sources

Bz=0

(Longcope 2001, Longcope & Klapper 2002)

Page 7: Current sheets formation along magnetic separators in 3d

A new type of constraint

The domain graph

Summarizes the Magnetic connectivity

N5

N4

N6 P3

P2

P1

Constrain coronal flux interconnecting sources

Page 8: Current sheets formation along magnetic separators in 3d

Structure of Constraint

N5

N4

N6 P3

P2

P1• Domain D16 connects P1 N6

• Flux in Domain D16:

(want to specify this)

• Flux in source 6:

(set by BC)

Page 9: Current sheets formation along magnetic separators in 3d

Structure of Constraint

N5

N4

N6 P3

P2

P1• Domain D16 connects P1 N6

• Flux in Domain D16:

(want to specify this)

• Flux in source 6:

(set by BC)

• Inter-related through

incidence matrix of graph:

i.e. �

A

Page 10: Current sheets formation along magnetic separators in 3d

A: Nc = Nd – Ns + 1

Structure of Constraint

N5

N4

N6 P3

P2

P1Q: How many domain fluxes

ab may be independantly specified?

Number of domains

Number of sources

here Nc = 7 – 6 + 1 = 2

Page 11: Current sheets formation along magnetic separators in 3d

Structure of Constraint

N5

N4

N6 P3

P2

P1

A: Nc = Nd – Ns + 1

Specifying fluxes of Nc chords reduces graph to a tree

Q: How many domain fluxes

ab may be independantly specified?

Page 12: Current sheets formation along magnetic separators in 3d

Structure of Constraint

N5

N4

N6 P3

P2

P1

A: Nc = Nd – Ns + 1

Specifying fluxes of Nc chords reduces graph to a tree … all remaining fluxes follow from flux balance: … etc.

Q: How many domain fluxes

ab may be independantly specified?

Page 13: Current sheets formation along magnetic separators in 3d

How to apply constraintsTopology of the potential field:*

• Extrapolate from bndry:

• Locate all magnetic null points B=0

0 B

• Trace spine field lines to spine sources

*same topology will apply to non-potential fields

Page 14: Current sheets formation along magnetic separators in 3d

The skeleton of the field

• Trace all fan field lines from null• Form sectors• Joined at separators• A separator connects + - null points

Page 15: Current sheets formation along magnetic separators in 3d

The skeleton of the field

• Trace all fan field lines from null• Form sectors• Joined at separators• A separator connects + - null points

Page 16: Current sheets formation along magnetic separators in 3d

The skeleton of the field

• Trace all fan field lines from null• Form sectors• Joined at separators• A separator connects + - null points

Page 17: Current sheets formation along magnetic separators in 3d

The skeleton of the field

• Trace all fan field lines from null• Form sectors• Joined at separators• A separator connects + - null points

Page 18: Current sheets formation along magnetic separators in 3d

Individual Domains Domain linking PaNb must be bounded by sectors +’ve sectors: Pa @ apex -’ve sectors: Nb @ apex

Sectors intersect @ closed separator circuitCircuit encircles domain

Page 19: Current sheets formation along magnetic separators in 3d

N5

N4

N6 P3

P2

P1

Formulating the constraint

Locate separator circuit Qi encircling domain Di:

0)}({ iQ

ii dF lAxAConstraint functional:

Page 20: Current sheets formation along magnetic separators in 3d

The Constrained Minimization

Minimize:Lagrange multiplier

Non-potential field: separator curve: Qi

annular ribbon xi(

xdScN

ii

iii

3

1

)()(

xA

ddFiQ

iii

ii

ii

xAxA )()}({

Singular density

-function

cN

iii FWC

1

)}({)}({)}({ xAxAxA All con-straints

Page 21: Current sheets formation along magnetic separators in 3d

• Vary

• Require stationarity: C = 0

• Get Euler-Lagrange equation

The Variation)()()( xAxAxA

CCC )}({)}({ xAxA

cc N

ii

N

ii

ii S

11

)()()( xJx

B

Singular current density, confined to separator ribbon i

Page 22: Current sheets formation along magnetic separators in 3d

Flux Constrained Equilibria

• Potential field (w/o constraints): i=i(v)

• Non-potential field: i=i(v) +i i=1,…,Nc

• Free Energy in flux-constrained field:

• General FFF:

0)()v( iWWW

)()v()(i

FFF WWW

N4

N2 P3

P1

23= 1

Page 23: Current sheets formation along magnetic separators in 3d

Flux Constrained Equilibria

• Min’m energy subject to Nc constraints

Nc fluxes are parameters: i

• Current-free within each domain

• Singular currents* on all separatorsN4

N2 P3

P1

1 1(v)

* Always ideally stable!

Page 24: Current sheets formation along magnetic separators in 3d

II. Approach to Equilibrium

• Separator defined

through footpoints

No locally

distinguishing

property*

• Singularity must build up through repeated reflection of information between footpoints

* In contrast to 2 dimensions: B=0 @ X-point

(Longcope & van Ballegooijen 2002)

Page 25: Current sheets formation along magnetic separators in 3d

Dynamics Illustrated

Equilib. fieldmaps sources tomerging layer

Long (almost straight)coronal field (RMHD)Maps between merging layers

Sourceson end planes

Page 26: Current sheets formation along magnetic separators in 3d

Dynamics Illustrated

N3

N4

Sep’x from nullon p-sphere

Page 27: Current sheets formation along magnetic separators in 3d

Dynamics Illustrated

Sources move (rotation)

N3

N4

Page 28: Current sheets formation along magnetic separators in 3d

Dynamics Illustrated

Sources move (rotation)

N3

N4

Page 29: Current sheets formation along magnetic separators in 3d

Dynamics Illustrated

Sources move (rotation)v

B

Initiates Alfven pulse (uniform rotation)

N3

N4

Page 30: Current sheets formation along magnetic separators in 3d

Dynamics Illustrated

Sources move (rotation)v

B

Initiates Alfven pulse (uniform rotation)

N3

N4

Page 31: Current sheets formation along magnetic separators in 3d

Dynamics Illustrated

Sources move (rotation)v

B

Initiates Alfven pulse (uniform rotation)

N3

N4

Page 32: Current sheets formation along magnetic separators in 3d

Dynamics Illustrated

Sources move (rotation)v

B

Initiates Alfven pulse (uniform rotation)

N3

N4

Page 33: Current sheets formation along magnetic separators in 3d

Dynamics Illustrated

v

B

Page 34: Current sheets formation along magnetic separators in 3d

Impact at Opposing End

v

B

P2

P1

Motion at mergingheight mapped down to photosphere

c.c rotation

Page 35: Current sheets formation along magnetic separators in 3d

Impact at Opposing End

P2

P1

Photosphere:fixed source positions,

moveable interiors

Merging height:No motion across sep’x

Free motion w/in source-regions

Page 36: Current sheets formation along magnetic separators in 3d

Impact at Opposing End

P2

P1

Photosphere:fixed source positions,

moveable interiors

Vorticitysheet @ sep’x

Merging height:No motion across sep’x

Free motion w/in source-regions

c.clockwise motion ineach region

Page 37: Current sheets formation along magnetic separators in 3d

Impact at Opposing End

P2

P1 N3

N4

Image of opposing separator is distortedby boundary motion

Page 38: Current sheets formation along magnetic separators in 3d

Impact at Opposing End

P2

P1 N3

N4

Image of opposing separator is distortedby boundary motion

Page 39: Current sheets formation along magnetic separators in 3d

Impact at Opposing End

P2

P1 N3

N4

Image of opposing separator is distortedby boundary motion

Page 40: Current sheets formation along magnetic separators in 3d

Impact at Opposing End

P2

P1 N3

N4

Intersection of separatrices: The Separator Ribbon

Page 41: Current sheets formation along magnetic separators in 3d

The Reflected Wave

Singular Alfven pulse:Voricity/Current sheetconfined to

P2

P1

Page 42: Current sheets formation along magnetic separators in 3d

The Reflected Wave

Separator ribbon left in wake of reflection

Page 43: Current sheets formation along magnetic separators in 3d

Repeated Reflection

z=0 z=L

• CS along reflects from z=0• CS along reflects from z=L• Repeated reflection retains only current on separator ribbon• Wave w/ current on ribbon - perfectly reflected

Page 44: Current sheets formation along magnetic separators in 3d

The Final Current Sheet

Interior CS(z=0)

B

Helical pitch, maps

z=0 z=L

Page 45: Current sheets formation along magnetic separators in 3d

The Final Current Sheet

Interior CS Helical pitch, maps

z=0 z=L

B

Page 46: Current sheets formation along magnetic separators in 3d

The Final Current Sheet

Interior CS Helical pitch, maps

z=0 z=L

B

Page 47: Current sheets formation along magnetic separators in 3d

The Final Current Sheet

Interior CS Helical pitch, maps

z=0 z=L

B

Page 48: Current sheets formation along magnetic separators in 3d

The Final Current Sheet

Interior CS Helical pitch, maps

z=0 z=L

Flux constrainedequilib.I set by e.g 23

B

Page 49: Current sheets formation along magnetic separators in 3d

Conclusions

• New class of constraints: domain fluxes

• Flux constrained equilibria have CS on

all separators

• Equilibrium is approached by repeated

Alfven wave reflections from boundary

Page 50: Current sheets formation along magnetic separators in 3d

Implications

• Coronal field tends toward singular state

• Current sheets are ideally stable

• Magnetic reconnection can– Eliminate constraint– Decrease magnetic energy

• Free energy depends on flux in NC different fluxes within corona.

Page 51: Current sheets formation along magnetic separators in 3d

Individual Domains• Field lines from one source fan outward… topological ball of field lines• Opposing sources at surface of ball• Sectors partition ball

Page 52: Current sheets formation along magnetic separators in 3d

Individual Domains• Field lines from one source fan outward… topological ball of field lines• Opposing sources at surface of ball• Sectors partition ball

Page 53: Current sheets formation along magnetic separators in 3d

Individual Domains• Field lines from one source fan outward… topological ball of field lines• Opposing sources at surface of ball• Sectors partition ball

Page 54: Current sheets formation along magnetic separators in 3d

Individual Domains

Domain = Intersection of 2 balls… Intersection is a closed separator circuit

Circuit girdles domain

Negative sector in negative ball

Positive sector in positive ball

Page 55: Current sheets formation along magnetic separators in 3d

A 3d example•Ns=6 sources•Nd=7 domainsNc=2 circuits•4 nulls (A1 …B2)•2 null-null lines C2

C1

Page 56: Current sheets formation along magnetic separators in 3d

A current sheet

• Isolating loop Q1 links domain D34

• Current ribbon for (v) -- vertical