SECCHI Observations Constraining The Initiation of Polar Coronal Jets Spiros Patsourakos, NRL with: E. Pariat A. Vourlidas S. Antiochos R. Howard SHOW.

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Presentation transcript:

SECCHI Observations Constraining The Initiation of Polar Coronal Jets Spiros Patsourakos, NRL with: E. Pariat A. Vourlidas S. Antiochos R. Howard SHOW HOW SECCHI CAN CONSTRAIN JET INITIATION

Why Care About Jets ? Very possibly driven by magnetic reconnection Ideal prototype to study reconnection in simple magnetic setups Could be an important contributor to solar wind mass

Magnetic Twist as a Driver of Polar Jets Magnetic Twist as a Driver of Polar Jets Axissymetric configuration 3D MHD simulations Apply twist kink A high speed ~ V A forms with helical structure a fraction of observed jets exhibit similar properties Pariat et al. 2007

Critical Elements of The Twist Model Kink instability - High Speed Outflow - Helical structure Can SECCHI 3D Observations constrain those elements ?

Recap of the Observations multipolar topology  slow rise  kink  rapid acceleration & helical structure 7 June 2007 ~ 05:00 UT North Polar Coronal Hole A-B ~ 11 degrees Observed by EUVI, COR1, COR2

Height-time plot of the Jet

‘Real’ Velocity of the Jet ‘Real’ Velocity of the Jet slow rise Rapid fraction of Va

3D Trajectory of the Jet evidence of kink

Helical Structure of the Jet I Helical Structure of the Jet I Small but noticeable differences between A & B which increase with time

Helical Structure of the Jet II Helical Structure of the Jet II Edge-on Face-on The Helical Structure is REAL !

Helical Structure of the Jet III Edge-enhanced Images

Emulating SECCHI Observations Emulating SECCHI Observations mass isosurfaces ~ 10 degrees evident differences

Work in Progress Assemble a database of jets More realistic comparisons between obs-modeling Establish a firm link between jets observations from EUVI & CORs t=1060 t=1120t=1080t=1200t=1160 X X Y Y  los 22

Summary Taking advantage of the unique characteristics of STEREO to: (1)Calculate ‘real’ v (2)Demonstrate kink in action (3)Demonstrate evidence of helical structure twist can drive polar jets Performed the first 3D observations of polar jets SECCHISECCHI CAN STRONGLY CONSTRAIN JET INITIATION

Work In Progress: More Realistic Model-Obs Comparisons t=1060 t=1120t=1080t=1200t=1160 X X Y Y  los 22

Acceleration of the Jet Acceleration of the Jet

Other Examples of Helical Jets

Difference Images base diff run diff

Observing Strategies with SECCHI Probably focus on 195 & 304 : higher constrast Coordinate with Hinode Run a pilot program soon. The SC seperation gets too big Synop cadence in 171 probably OK. But higher cadence (~30 s) in required in order to see in 3D the jet oscillations that XRT sees. PFIs ? Deeper exposures with CORs ? Anything in HIs ?

171, 195, 304 Movies 171, 195, 304 Movies