Determining flows from magnetic field evolution An outline of the approach we’ve adopted at UCB (Welsch, Fisher, Abbett, Regnier)

Slides:



Advertisements
Similar presentations
Bayesian Belief Propagation
Advertisements

Motion.
Estimating Surface Flows from HMI Magnetograms Brian Welsch, SSL UC-Berkeley GOAL: Consider techniques available to estimate flows from HMI vector magnetograms,
Time Series of Magnetograms: Evolution, Interpretations, Inferring Flows G. Fisher, Y. Li, B. Welsch.
Inductive Flow Estimation for HMI Brian Welsch, Dave Bercik, and George Fisher, SSL UC-Berkeley.
Using HMI to Understand Flux Cancellation by Brian Welsch 1, George Fisher 1, Yan Li 1, and Xudong Sun 2 1 Space Sciences Lab, UC-Berkeley, 2 Stanford.
Can We Determine Electric Fields and Poynting Fluxes from Vector Magnetograms and Doppler Shifts? by George Fisher, Brian Welsch, and Bill Abbett Space.
SSPVE Discussion Group B Question 5 To what extent is it possible to predict the emergence of active regions before they reach the photosphere, or to predict.
“Assimilating” Solar Data into MHD Models of the Solar Atmosphere W.P. Abbett SSL UC Berkeley HMI Team Meeting, Jan 2005.
SHINE Campaign Event: 1-2 May 1998 Brian Welsch (& Yan Li) Space Sciences Laboratory, UC Berkeley Introduction: Data, Context, etc. Work: Completed & Ongoing.
Using Photospheric Flows Estimated from Vector Magnetogram Sequences to Drive MHD Simulations B.T. Welsch, G.H. Fisher, W.P. Abbett, D.J. Bercik, Space.
1 A New Technique for Deriving Electric Fields from Sequences of Vector Magnetograms George H. Fisher Brian T. Welsch William P. Abbett David J. Bercik.
Reducing the Divergence of Optimization-Generated Magnetic Fields J.M. McTiernan, B.T. Welsch, G.H. Fisher, D.J. Bercik, W.P. Abbett Space Sciences Lab.
HMI, Photospheric Flows and ILCT Brian Welsch, George Fisher, Yan Li, & the UCB/SSL MURI & CISM Teams HMI Team Mtg., 2006M3: Mag Data Products Correlation.
Local Data-driven MHD Simulations of Active Regions W.P. Abbett MURI 8210 Workshop Mar 2004.
Estimating Electric Fields from Sequences of Vector Magnetograms George H. Fisher, Brian T. Welsch, William P. Abbett, and David J. Bercik University of.
HMI & Photospheric Flows 1.Review of methods to determine surface plasma flow; 2.Comparisons between methods; 3.Data requirements; 4.Necessary computational.
Dec. 10, 2004RHESSI/SOHO/TRACE The Minimum Energy Fit Consistent with Induction at Minimum Possible Cost Dana Longcope Montana State University Work supported.
M3 Session AIA/HMI Science Meeting D-1 : M3-Magnetic Field Data Products Data Product Development Session Chairs: R. Larsen/Y. Liu Status: [draft]
HMI – Synoptic Data Sets HMI Team Meeting Jan. 26, 2005 Stanford, CA.
1 SDO/HMI Products From Vector Magnetograms Yang Liu – Stanford University
ILCT-Derived Flows are Consistent with Induction Eqn’s Normal Component. Directly measured Derived by ILCT.
Estimating Electric Fields from Vector Magnetogram Sequences G. H. Fisher, B. T. Welsch, W. P. Abbett, D. J. Bercik University of California, Berkeley.
1 FLCT: A Fast, Efficient Method for Performing Local Correlation Tracking George H. Fisher Brian T. Welsch Space Sciences Laboratory, UC Berkeley.
Electric and Velocity Field Determination in the Solar Atmosphere George H. Fisher, University of California, Berkeley Collaborators: Brian Welsch (UCB),
Free Energies via Velocity Estimates B.T. Welsch & G.H. Fisher, Space Sciences Lab, UC Berkeley.
Incorporating Vector Magnetic Field Measurements into MHD models of the Solar Atmosphere W.P. Abbett Space Sciences Laboratory, UC Berkeley and B.T. Welsch,
Inductive Local Correlation Tracking or, Getting from One Magnetogram to the Next Goal (MURI grant): Realistically simulate coronal magnetic field in eruptive.
UCB-SSL Progress Report for the Joint CCHM/CWMM Workshop W.P. Abbett, G.H. Fisher, and B.T. Welsch.
Understanding the Connection Between Magnetic Fields in the Solar Interior and the Solar Corona George H. Fisher Space Sciences Laboratory UC Berkeley.
Finding Photospheric Flows with I+LCT or,“Everything you always wanted to know about velocity at the photosphere, but were afraid to ask.” B. T. Welsch,
Summary of workshop on AR May One of the MURI candidate active regions selected for detailed study and modeling.
Tracking using the Kalman Filter. Point Tracking Estimate the location of a given point along a sequence of images. (x 0,y 0 ) (x n,y n )
SSL (UC Berkeley): Prospective Codes to Transfer to the CCMC Developers: W.P. Abbett, D.J. Bercik, G.H. Fisher, B.T. Welsch, and Y. Fan (HAO/NCAR)
LCT Active Region Survey: Preliminary Results We proposed to calculate LCT flows (Li et al. 2004, Welsch et al., 2004) in N > 30 ARs, some of which produced.
Magnetogram Evolution Near Polarity Inversion Lines Brian Welsch and Yan Li Space Sciences Lab, UC-Berkeley, 7 Gauss Way, Berkeley, CA , USA.
Measuring, Understanding, and Using Flows and Electric Fields in the Solar Atmosphere to Improve Space Weather Prediction George H. Fisher Space Sciences.
Flows in NOAA AR 8210: An overview of MURI progress to thru Feb.’04 Modelers prescribe fields and flows (B, v) to drive eruptions in MHD simulations MURI.
Using HMI to Understand Flux Cancellation by Brian Welsch 1, George Fisher 1, Yan Li 1, and Xudong Sun 2 1 Space Sciences Lab, UC-Berkeley, 2 Stanford.
Surface Flows From Magnetograms Brian Welsch, George Fisher, Bill Abbett, & Yan Li Space Sciences Laboratory, UC-Berkeley Marc DeRosa Lockheed-Martin Advanced.
Flows and the Photospheric Magnetic Field Dynamics at Interior – Corona Interface Brian Welsch, George Fisher, Yan Li, & the UCB/SSL MURI & CISM Teams.
Data-Driven Simulations of AR8210 W.P. Abbett Space Sciences Laboratory, UC Berkeley SHINE Workshop 2004.
Understanding the Connection Between Magnetic Fields in the Solar Interior and Magnetic Activity in the Corona W.P. Abbett and G.H. Fisher, B.T. Welsch,
Jan. 27, 2005HMI team meeting The Minimum Energy Fit The Slowest Motion Required by Induction Dana Longcope Montana State University Work supported by.
Motion Estimation Today’s Readings Trucco & Verri, 8.3 – 8.4 (skip 8.3.3, read only top half of p. 199) Numerical Recipes (Newton-Raphson), 9.4 (first.
Using Photospheric Flows Estimated from Vector Magnetogram Sequences to Drive MHD Simulations B.T. Welsch, G.H. Fisher, W.P. Abbett, D.J. Bercik, Space.
Surface Flows From Magnetograms Brian Welsch, George Fisher, Bill Abbett, & Yan Li Space Sciences Laboratory, UC-Berkeley M.K. Georgoulis Applied Physics.
COMP 290 Computer Vision - Spring Motion II - Estimation of Motion field / 3-D construction from motion Yongjik Kim.
The Effect of Sub-surface Fields on the Dynamic Evolution of a Model Corona Goals :  To predict the onset of a CME based upon reliable measurements of.
Active Region Flux Transport Observational Techniques, Results, & Implications B. T. Welsch G. H. Fisher
1 A New Technique for Deriving Electric Fields from Sequences of Vector Magnetograms George H. Fisher Brian T. Welsch William P. Abbett David J. Bercik.
B. T. Welsch Space Sciences Lab, Univ. of California, Berkeley, CA J. M. McTiernan Space Sciences.
Using Simulations to Test Methods for Measuring Photospheric Velocity Fields W. P. Abbett, B. T. Welsch, & G. H. Fisher W. P. Abbett, B. T. Welsch, & G.
Finding the Flow Field Need flow information! –ideal evolution of coronal B(x,y,z,t) determined entirely by B(x,y,z,0) and v(x,y,0) – get v wrong and get.
Motion Vectors. Displacement Vector  The position vector is often designated by.  A change in position is a displacement.  The displacement vector.
UCB MURI Team Introduction An overview of ongoing work to understand a well observed, eruptive active region, along with closely related studies…..
2002 May 1MURI VMG mini-workshop1` Solar MURI Vector Magnetogram Mini-Workshop Using Vector Magnetograms in Theoretical Models: Plan of Action.
Summary of UCB MURI workshop on vector magnetograms Have picked 2 observed events for targeted study and modeling: AR8210 (May 1, 1998), and AR8038 (May.
The Physical Significance of Time-Averaged Doppler Shifts Along Magnetic Polarity Inversion Lines (PILs) Brian Welsch Space Sciences Laboratory, UC-Berkeley.
EE369C Final Project: Accelerated Flip Angle Sequences Jan 9, 2012 Jason Su.
Introduction to the FLCT code George Fisher Brian Welsch Space Sciences Lab, UC Berkeley Purpose: Given two images separated in time, determine an estimate.
Photospheric Flows & Flare Forecasting tentative plans for Welsch & Kazachenko.
Motion Estimation Today’s Readings Trucco & Verri, 8.3 – 8.4 (skip 8.3.3, read only top half of p. 199) Newton's method Wikpedia page
A Non-iterative Hyperbolic, First-order Conservation Law Approach to Divergence-free Solutions to Maxwell’s Equations Richard J. Thompson 1 and Trevor.
Vectors in the Plane Objectives: Define a vector What are the basic terms associated with vectors?
Motion Estimation Today’s Readings Trucco & Verri, 8.3 – 8.4 (skip 8.3.3, read only top half of p. 199) Newton's method Wikpedia page
Motion Estimation Today’s Readings
The Moat Flow Observed in Two Different TRACE-Filters
Announcements more panorama slots available now
Announcements more panorama slots available now
Presentation transcript:

Determining flows from magnetic field evolution An outline of the approach we’ve adopted at UCB (Welsch, Fisher, Abbett, Regnier)

Determining a physically reasonable flow field is essential for data-driven MHD models. To what extent can flow velocities be inverted from time sequences of magnetogram data? We believe the ideal MHD induction equation should be obeyed…

The standard technique for determining horizontal motions is Local Correlation Tracking… There are many different implementations in use today. The original idea was described in November & Simon (1988) – try to define a velocity by moving sub-images of an image taken at an earlier time to best fit corresponding sub-images of an image taken later. No physics involved. Other versions in use at BBSO, LMSAL We developed our own implementation. For each pixel location, multiply the image by a gaussian centered at the given pixel location, and find the shift between the resulting 2 images that maximizes the cross-correlation function. The cross-correlation function is determined using standard FFT techniques. Our IDL LCT code is publicly available:

LCT tests show it works under a wide variety of conditions … Apply a velocity field to an image consisting of random hash – can LCT correctly recover the velocity?

Recovered velocity fields… Here, it did correctly find the applied horizontal velocity field… VxVx VyVy

Induction equation (z component) Define a new quantity U  such that then

Decomposing vertical and horizontal flow components: Once is known, are known if

Induction + LCT (ILCT) Welsch, Fisher, Abbett (UCB), Regnier (MSU) Induction Eqn. Constrains  Induction Eqn. Constrains  LCT Constrains 

Note that knowledge of transverse fields not needed to solve induction equation! Caveats: If knowledge of real vertical and horizontal velocities needed (as in an MHD code), then need B  to determine v z and v . The vertical component of induction equation doesn’t apply if the LOS and vertical direction differ substantially ILCT formalism needs to be extended away from disk center if it is to be used with scalar magnetograms

Warts, problems with LCT, ILCT With ILCT, velocity is poorly determined near neutral lines or in magnetically featureless areas LCT performs reasonably well in “moving paint” experiments, but does poorly in recovering flows from many MHD simulations. Our LCT algorithm is too slow. It needs to be made faster (is now written in IDL, should probably be re-written in Fortran or C. LCT, ILCT are unconstrained by flows parallel to the field. Magnetic evolution provides no constraint on parallel flows.