Magnetic Topology and the Corona- Heliosphere Connection Background: –Frozen-in flux (τ D ~ L 2 /...

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Magnetic Topology and the Corona-Heliosphere Connection • Background: Frozen-in flux (τ D ~ L 2 / η >> τ L ) implies that magnetic topology constrains plasma structure and dynamics Determines how photo/corona connects to heliosphere • Importance: Restricts possible topology of coronal holes (CH) Insight into 3D CME models – breakout Predictions for LWS and especially SDO Spiro K. Antiochos Code 7675, Naval Research Lab, Washington DC 20375 [email protected]
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Transcript of Magnetic Topology and the Corona- Heliosphere Connection Background: –Frozen-in flux (τ D ~ L 2 /...

Page 1: Magnetic Topology and the Corona- Heliosphere Connection Background: –Frozen-in flux (τ D ~ L 2 / η >> τ L ) implies that magnetic topology constrains.

Magnetic Topology and the Corona-Heliosphere Connection

• Background:– Frozen-in flux (τD ~ L2 / η >> τL ) implies that magnetic

topology constrains plasma structure and dynamics

– Determines how photo/corona connects to heliosphere

• Importance:– Restricts possible topology of coronal holes (CH)

– Insight into 3D CME models – breakout

– Predictions for LWS and especially SDO

Spiro K. AntiochosCode 7675, Naval Research Lab, Washington DC 20375 [email protected]

Page 2: Magnetic Topology and the Corona- Heliosphere Connection Background: –Frozen-in flux (τ D ~ L 2 / η >> τ L ) implies that magnetic topology constrains.

Basic Assumptions

• Continuous polarity distribution at ‘photosphere’ – Structure given by neutral line geometry

– Neglect small-scale dipoles/structure

• No current singularities in closed field region– Basically assuming quasi-static equilibrium

– Extension of source-surface model

– Field-line mapping smooth except at separatrices

Page 3: Magnetic Topology and the Corona- Heliosphere Connection Background: –Frozen-in flux (τ D ~ L 2 / η >> τ L ) implies that magnetic topology constrains.

• Canonical coronal magnetic topology – Two large-scale neutral lines on photosphere – Three separatix curves and two points on photosphere– Field defines smooth volume mapping, except at separatrix

lines/points, even if J = 0.

Field line equations:dx/ds = Bx/B

dy/ds = By/B

dz/ds = Bz/B

Singularity e.g., splitting, only if,Bx, By, or Bz

discontinuous or B vanishes

Page 4: Magnetic Topology and the Corona- Heliosphere Connection Background: –Frozen-in flux (τ D ~ L 2 / η >> τ L ) implies that magnetic topology constrains.

Conjecture: One CH per Polarity Region• Consider simple polarity region with one CH

• Consider annulus of closed flux surrounding CH

• Cannot map to adjacent area,– Requires line splitting, current singularity in closed field region

Page 5: Magnetic Topology and the Corona- Heliosphere Connection Background: –Frozen-in flux (τ D ~ L 2 / η >> τ L ) implies that magnetic topology constrains.

• Must map to surrounding annulus

• But then, second CH would split closed lines

Page 6: Magnetic Topology and the Corona- Heliosphere Connection Background: –Frozen-in flux (τ D ~ L 2 / η >> τ L ) implies that magnetic topology constrains.

• Consider embedded polarity region – If region closed, annulus maps over the top– If region contains coronal hole?– Problem with both CH and spine

Page 7: Magnetic Topology and the Corona- Heliosphere Connection Background: –Frozen-in flux (τ D ~ L 2 / η >> τ L ) implies that magnetic topology constrains.

If polarity regions embedded, CHs are embedded – Opening of CH in embedded region drives external CH

• Creates coronal hole corridor

– CH in embedded region must extend to spine – CMEs?

Page 8: Magnetic Topology and the Corona- Heliosphere Connection Background: –Frozen-in flux (τ D ~ L 2 / η >> τ L ) implies that magnetic topology constrains.

• Interaction of AR with CH – Begin with AR fully in closed region– Apply photo motion that moves AR into CH– Interchange reconnection opens spine– Creates open field corridor surrounding spot (movie)

Page 9: Magnetic Topology and the Corona- Heliosphere Connection Background: –Frozen-in flux (τ D ~ L 2 / η >> τ L ) implies that magnetic topology constrains.

Topology of 3D Breakout Eruption• Any long-lived opening must extend to separatrix

Page 10: Magnetic Topology and the Corona- Heliosphere Connection Background: –Frozen-in flux (τ D ~ L 2 / η >> τ L ) implies that magnetic topology constrains.

Topology of Fully 3D Breakout• Minimize required energy by rearranging

separatrices (reconnection)

Page 11: Magnetic Topology and the Corona- Heliosphere Connection Background: –Frozen-in flux (τ D ~ L 2 / η >> τ L ) implies that magnetic topology constrains.

CONCLUSIONS

• Topology provides strong constraints on corona-heliosphere connection– One CH per polarity region – CH corridors– Embedded polarities imply embedded CHs

• Topology plays critical role in 3D eruptions – Mechanism underlying breakout– Predicts spine movement, dimming areas, …

• Fascinating field for Theory/SDO studies