Solar Magnetic Field Reversal V J Pizzo SHINE Workshop August 18, 2002.

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Presentation transcript:

Solar Magnetic Field Reversal V J Pizzo SHINE Workshop August 18, 2002

Overview Historical Perspective Sorting through the Issues Challenges and Opportunities

Observational Basis (Babcock, ApJ, 133, 572, 1961) –Sunspot cycle –Butterfly diagram (latitudinal progression) –Leader/follower asymmetry and polarities –BMRs: death by expansion –Poleward migration of prominence chain –Reversal of global solar magnetic field –Differential rotation –[Supergranular motions, meridional flows] Historical Perspective (1)

Leighton model (ApJ, 140, 1547, 1964) –Erupted flux disperses via supergranular random walk –Differential rotation, but no meridional flow –Surface dynamics only, smooth diffusive cancellation of expanding BMR fields –Pre-CME & HCS –Results: Basics “explained”: Polar reversal, leader/follower expansion, poleward prominence migration Shortcomings: Heavily idealized, too slow, smooth +/- transitions, de facto dynamo, no corona Historical Perspective (2)

Wang, Sheeley, & Lean (GRL, 27, 621, 2000; + previous publ.) –Include systematic meridional flows (e.g., Komm et al., Sol. Phys., 147, 207, 1993) –More realistic inputs –Main results: Meridional flows speed latitudinal dispersal of flux Evolution of open flux, relation to total flux –Emerging BMRs can be source of new open flux –Effects of nonuniform distribution of erupted flux Historical Perspective (3)

Fisk Mechanism (heliospheric) Fisk, Schwadron, & Zurbuchen – Reconcile observations of rigid rotation in corona with surface differential rotation – Follow consequences of magnetic fieldline footpoint motion due to differential rotation (long-lived footpoints) – Restricted to high-latitude field – Produce non-Parker field topology (N/S particle transport)

Fisk Mechanism (Corona) Account for interaction of differential rotation with HCS & streamers Consider “interchange” reconnection (driven by differential rotation) in open and closed regions Model for field reversal – “constancy” of open flux – rotation of HCS

Fisk Mechanism (Corona) Account for interaction of differential rotation with streamers Consider “interchange” reconnection (driven by differential rotation) in open and closed regions Model for field reversal – “constancy” of open flux – rotation of HCS

Open flux as the key Suess et al

Arge et al., JGR (in press)

Fox, McIntosh, & Wilson

Richardson et al., GRL, 21, , 1994

WSO Classic Source Surface Field

*

MWO Photospheric Field

Sub-surface Driver? Torsional Oscillation Solar weather via helioseismology – Role of systematic subsurface motions – “Gulf stream” analogy?

Haber et al.

1.3 year Coronal “Cycle” Heliospheric identification driven by dynamo (photospheric field)? relation to torsional oscillation? relation to polar field reversal? relation to Fisk mechanism? heliospheric manifestation?

*

Role of CMEs Why are they there? (Earthquake analogy) Remove flux? (flux catastrophy: how well can we identify detached field in situ?) Remove helicity? Driver or agent of exchange reconnection? Relation to large scale coronal topological evolution – Location (streamer belt, switch-backs, delta config.) – Frequency (temporal clustering?) – Type (complex, fast vs slow, polar crown, etc.) Coronal source of GMIRs?

Challenges and Opportunities Timescale and pattern of coronal topological changes Frequency and distribution of CMEs relative to coronal topological changes Open flux  hole vs open region STEREO target: location of CMEs – surface activity poor indicator of longitude HCS and heliospheric structure during major episode of change

Arge, K Harvey, Hudson, & Kahler

Challenges and Opportunities Timescale and pattern of coronal topological changes Frequency and distribution of CMEs relative to coronal topological changes Open flux  hole vs open region STEREO target: location of CMEs – surface activity poor indicator of longitude HCS and heliospheric structure during major episode of change