Dynamical Implications Juri Toomre, JILA Helioseis: Deborah Haber, Brad Hindman + Rick Bogart,...

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Dynamical Implications Dynamical Implications Juri Toomre, JILA Juri Toomre, JILA Helioseis: Helioseis: Deborah Haber, Brad Deborah Haber, Brad Hindman + Rick Bogart, Douglas Gough, Frank Hill, Hindman + Rick Bogart, Douglas Gough, Frank Hill, Jesper Schou, Mike Thompson Jesper Schou, Mike Thompson Dynamics: Dynamics: Nic Brummell, Sacha Brun, Marc Nic Brummell, Sacha Brun, Marc DeRosa, Mark Miesch DeRosa, Mark Miesch
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Transcript of Dynamical Implications Juri Toomre, JILA Helioseis: Deborah Haber, Brad Hindman + Rick Bogart,...

Page 1: Dynamical Implications Juri Toomre, JILA Helioseis: Deborah Haber, Brad Hindman + Rick Bogart, Douglas Gough, Frank Hill, Jesper Schou, Mike Thompson Dynamics:

Dynamical ImplicationsDynamical Implications

Juri Toomre, JILA Juri Toomre, JILA Helioseis:Helioseis: Deborah Haber, Deborah Haber, Brad Hindman + Rick Bogart, Douglas Gough, Brad Hindman + Rick Bogart, Douglas Gough,

Frank Hill, Jesper Schou, Mike ThompsonFrank Hill, Jesper Schou, Mike Thompson

Dynamics:Dynamics: Nic Brummell, Sacha Brun, Nic Brummell, Sacha Brun, Marc DeRosa, Mark MieschMarc DeRosa, Mark Miesch

Page 2: Dynamical Implications Juri Toomre, JILA Helioseis: Deborah Haber, Brad Hindman + Rick Bogart, Douglas Gough, Frank Hill, Jesper Schou, Mike Thompson Dynamics:

Just what is inside a star ?Just what is inside a star ?

ArnaldoArnaldoPOMODOROPOMODORO

Page 3: Dynamical Implications Juri Toomre, JILA Helioseis: Deborah Haber, Brad Hindman + Rick Bogart, Douglas Gough, Frank Hill, Jesper Schou, Mike Thompson Dynamics:

Objective 1:Objective 1: CZ dynamics & solar dynamo CZ dynamics & solar dynamo

• A. Structure and dynamics of A. Structure and dynamics of tachoclinetachocline

• B. Variations in B. Variations in differential rotationdifferential rotation

• C. Evolution in C. Evolution in meridional circulationmeridional circulation

• D. Dynamics in D. Dynamics in near-surface shear layernear-surface shear layer

Objective 2:Objective 2: Evolution of complexes of activity Evolution of complexes of activity

Page 4: Dynamical Implications Juri Toomre, JILA Helioseis: Deborah Haber, Brad Hindman + Rick Bogart, Douglas Gough, Frank Hill, Jesper Schou, Mike Thompson Dynamics:

Mean Angular Velocity ProfilesMean Angular Velocity Profiles

TACHOCLINETACHOCLINE NEAR-SURFACENEAR-SURFACESHEAR LAYERSHEAR LAYER

CZ BOTTOMCZ BOTTOM

HMI-landHMI-land

Page 5: Dynamical Implications Juri Toomre, JILA Helioseis: Deborah Haber, Brad Hindman + Rick Bogart, Douglas Gough, Frank Hill, Jesper Schou, Mike Thompson Dynamics:

Theoretical Solar CycleTheoretical Solar Cycle

PHOTOSPHEREPHOTOSPHERE

CONVECTIONCONVECTION ZONEZONE

TACHOCLINETACHOCLINE

RADIATIVE RADIATIVE INTERIORINTERIOR

LOCALLOCALDYNAMODYNAMO

GLOBALGLOBALDYNAMODYNAMOBUOYANCYBUOYANCY

PUMPINGPUMPING

EMERGINGEMERGING LOOPLOOP

ROTATION ROTATION

Page 6: Dynamical Implications Juri Toomre, JILA Helioseis: Deborah Haber, Brad Hindman + Rick Bogart, Douglas Gough, Frank Hill, Jesper Schou, Mike Thompson Dynamics:

Evolution in Radial Velocity (0.96 R)Evolution in Radial Velocity (0.96 R)

VIEWED INVIEWED IN`CARRINGTON’`CARRINGTON’ FRAMEFRAME

Case ECase EBrun, MieschBrun, Miesch & Toomre& Toomre

NEAR TOPNEAR TOPOF LAYEROF LAYER

Page 7: Dynamical Implications Juri Toomre, JILA Helioseis: Deborah Haber, Brad Hindman + Rick Bogart, Douglas Gough, Frank Hill, Jesper Schou, Mike Thompson Dynamics:

Global View of Radial VelocityGlobal View of Radial Velocity

Page 8: Dynamical Implications Juri Toomre, JILA Helioseis: Deborah Haber, Brad Hindman + Rick Bogart, Douglas Gough, Frank Hill, Jesper Schou, Mike Thompson Dynamics:

But can we detect such giant cells by But can we detect such giant cells by helioseismic observation?helioseismic observation?

Page 9: Dynamical Implications Juri Toomre, JILA Helioseis: Deborah Haber, Brad Hindman + Rick Bogart, Douglas Gough, Frank Hill, Jesper Schou, Mike Thompson Dynamics:

Giant cells:Giant cells:complex complex evolving evolving structuresstructures

Page 10: Dynamical Implications Juri Toomre, JILA Helioseis: Deborah Haber, Brad Hindman + Rick Bogart, Douglas Gough, Frank Hill, Jesper Schou, Mike Thompson Dynamics:

Propagating and evolving velocity patternsPropagating and evolving velocity patterns

Time-longitude mapTime-longitude map (relative to Carrington) at 20 degrees north

+5d +10d

Page 11: Dynamical Implications Juri Toomre, JILA Helioseis: Deborah Haber, Brad Hindman + Rick Bogart, Douglas Gough, Frank Hill, Jesper Schou, Mike Thompson Dynamics:

Big Questions:Big Questions: Global-Scale Convection Global-Scale Convection

• Why no clear or direct detectionWhy no clear or direct detection of giant convection cells?

• Does intense near-surface turbulenceDoes intense near-surface turbulence of granulation and supergranulation yield transport barrier to deflect such flows?

• May simply be very tough to detectMay simply be very tough to detect since narrow downflows but wide cell scales, and they both evolve and propagate

Page 12: Dynamical Implications Juri Toomre, JILA Helioseis: Deborah Haber, Brad Hindman + Rick Bogart, Douglas Gough, Frank Hill, Jesper Schou, Mike Thompson Dynamics:

Ring AnalysesRing Analyses: Two Successive Rotations: Two Successive Rotations

7 Mm7 Mm

19971997

CRCR19231923

CRCR19221922

Page 13: Dynamical Implications Juri Toomre, JILA Helioseis: Deborah Haber, Brad Hindman + Rick Bogart, Douglas Gough, Frank Hill, Jesper Schou, Mike Thompson Dynamics:

Changing Meridional Circulation CellsChanging Meridional Circulation Cells

20002000

19991999

19981998

NORTH:NORTH:DOUBLEDOUBLECELLCELL

NORTHNORTHSOUTHSOUTH

20012001

SOUTH:SOUTH:SINGLESINGLECELLCELL

POLEWARDPOLEWARDFLOW NEARFLOW NEARSURFACESURFACE

REVERSED REVERSED FLOWFLOWAT DEPTHAT DEPTH

19971997

19961996

Haber et al Haber et al (2002)(2002)

Page 14: Dynamical Implications Juri Toomre, JILA Helioseis: Deborah Haber, Brad Hindman + Rick Bogart, Douglas Gough, Frank Hill, Jesper Schou, Mike Thompson Dynamics:

SSW Evolution Near Active ComplexesSSW Evolution Near Active Complexes

Page 15: Dynamical Implications Juri Toomre, JILA Helioseis: Deborah Haber, Brad Hindman + Rick Bogart, Douglas Gough, Frank Hill, Jesper Schou, Mike Thompson Dynamics:

High-Resolution Ring AnalysisHigh-Resolution Ring Analysis

Page 16: Dynamical Implications Juri Toomre, JILA Helioseis: Deborah Haber, Brad Hindman + Rick Bogart, Douglas Gough, Frank Hill, Jesper Schou, Mike Thompson Dynamics:

Evolution in Doppler Correlation TrackingEvolution in Doppler Correlation Tracking Lisle, DeRosa Lisle, DeRosa

Page 17: Dynamical Implications Juri Toomre, JILA Helioseis: Deborah Haber, Brad Hindman + Rick Bogart, Douglas Gough, Frank Hill, Jesper Schou, Mike Thompson Dynamics:

Analysis StrategyAnalysis Strategy

• Devise some Devise some combinationcombination of local-domain of local-domain helioseismic probings to provide:helioseismic probings to provide:

• Nearly soon(real)-time, continuous Nearly soon(real)-time, continuous subsurface flow mappingssubsurface flow mappings in upper in upper 20+ Mm -- fast analysis pipes20+ Mm -- fast analysis pipes

Page 18: Dynamical Implications Juri Toomre, JILA Helioseis: Deborah Haber, Brad Hindman + Rick Bogart, Douglas Gough, Frank Hill, Jesper Schou, Mike Thompson Dynamics:

Our thrusts with rings (and time-distance)Our thrusts with rings (and time-distance)

• Re-evaluate ALL elementsRe-evaluate ALL elements in current ring procedures: mappings, ridge or ring fits, varying resolution across disk, line asymmetries vs varying background …

• Devise multi-scale tiling analysesDevise multi-scale tiling analyses, and build mature 3-D inversions for flow fields

• Test all with high-resolution MDITest all with high-resolution MDI Doppler data to verify procedures and codes