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American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and Space Research Department of Physics

American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and

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Page 1: American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and

American Physical Society March 6, 2007

The MIT TEAL Simulations and Visualizations in

Electromagnetism

John W. Belcher

Kavli Center for Astrophysics and Space Research

Department of Physics

Page 2: American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and

American Physical Society March 6, 2007

Funding Sources

NSF DUE-0618558

Davis Educational Foundation

d’Arbeloff Fund

iCampus

Helena Foundation

MIT Classes of 51, 55, 60

Page 3: American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and

American Physical Society March 6, 2007

Who Am I?PI on the Voyager Plasma Science Instrument on the Voyager Spacecraft

I have spent a lot of time trying to explain the unseen to reporters at Voyager press conferences since 1979

I have taught E&M at all levels at MIT for 30 years

I have helped reform freshman level E&M for the last six years

Neptune’s Magnetosphere 1989

Page 4: American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and

American Physical Society March 6, 2007

Outline of TalkA Brief Explanation of TEAL

How do visualizations fit into TEAL?

How do we represent fields:Vector Field Grid

Field Lines (“Eppur Si Mouve”) Line Integral Convolution (LIC)—the best thing since sliced bread

Moving Field LinesWhen does this make sense? (E, B perpendicular)

What does it represent? (test particle motion)

Why it gives access to high level concepts, e.g. Maxwell stresses

Dynamic Line Integral Convolution and examples

How Does This Contribute to E&M Understanding?

Page 5: American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and

American Physical Society March 6, 2007

TEAL: Technology Enabled Active Learning

Large freshman physics courses have inherent problems

Lecture/recitations are passive

No labs (at MIT) leads to lack of physical intuition

Math is abstract, hard to visualize (esp. E&M)

TEAL/Studio addresses these by

Replacing large lectures with interactive, collaborative pedagogy

Incorporating desk top experiments

Incorporating visualization/simulations

Page 6: American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and

American Physical Society March 6, 2007

One of the two MIT TEAL Classrooms

Modeled after NCSU’s SCALE-UP Classroom

Page 7: American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and

American Physical Society March 6, 2007

Page 8: American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and

American Physical Society March 6, 2007

Ideal TEAL Sequence(instructor’s fantasy)

1.Lecture2.Pre-Experiment Predictions3.Experiment4.Visualization of ExperimentI will illustrate this sequence

for Faraday’s Law

Page 9: American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and

American Physical Society March 6, 2007

Magnetic Flux

Move down

1. Lecture: Faraday’s Law

Bd

dt

Page 10: American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and

American Physical Society March 6, 2007

Magnetic Flux

Move down

2. Pre-Experiment Predictions

Personal Response System used for pre-experiment questions and responses

Page 11: American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and

American Physical Society March 6, 2007

3. Experiment

Experiment includes sliding an aluminum sleeve over the magnet and feeling the slowdown due to

eddy currents

Page 12: American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and

American Physical Society March 6, 2007

4.Visualization of Experiment

Show a virtual model of the real experiment

Add field representationShow the field three ways:

Vector Field GridField Lines Line Integral Convolution

Page 13: American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and

American Physical Society March 6, 2007

Loop of wire has inductance L and

resistance R and a decay time of L/R

Page 14: American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and

American Physical Society March 6, 2007

Line Integral Convolution (LIC) Introduced by Cabral and Leedom

(computer scientists) in 1993 Uses a texture pattern where the streaks

in the texture are parallel to the local field direction

Shows the structure of the field close to the resolution of the display!

Vastly superior to either vector field or field lines in showing structure of 2D fields

Page 15: American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and

American Physical Society March 6, 2007

Line Integral Convolution: How? Take array of NxN pixels of random brightness At any point, average the random pattern along a

line in the direction of the local field for n pixels, n << N

Move to an adjacent new point and do this again If you move parallel to the field to get to the new

point, the resulting average is almost the same as for the old point, e.g. highly correlated

If you move perpendicular to the field to get to the new point, the resulting average is not correlated at all with the average at the previous point

This produces correlations along the field direction

Page 16: American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and

American Physical Society March 6, 2007

Page 17: American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and

American Physical Society March 6, 2007

Page 18: American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and

American Physical Society March 6, 2007

What does a LIC of this functionlook like?

This function has zero divergence and non-zero curl, so you expect no sources and

lots of circulation

2 2ˆ ˆ( , ) sin( ) cos( )x y y x F i j

Page 19: American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and

American Physical Society March 6, 2007

We had a full page of Wired

Magazine devoted to

one of these in

Sept 2004

Page 20: American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and

American Physical Society March 6, 2007

Mapping Fields Applet

(http://web.mit.edu/viz/soft/

Page 21: American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and

American Physical Society March 6, 2007

Moving Field Lines (nothing to do with plasma physics)

Will the proton gyrating about

the B field move with the solenoid if you

slowly start pushing the cart? Why or why not?

Page 22: American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and

American Physical Society March 6, 2007

Moving Field Lines (nothing to do with plasma physics)

Yes the gyrating proton will move with the cart because of the ExB drift

2 2 drift B B

V B BE B

E V B V V

Page 23: American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and

American Physical Society March 6, 2007

Moving Field Lines (nothing to do with plasma physics)

Valid in situations where E and B are everywhere perpendicular

In magneto-statics, field motion defined to be motion of test electric monopoles

In electrostatics, field motion defined be motion of test magnetic monopoles

Useful even in e.g. radiation because the motion is in the direction of the Poynting flux vector

2drift B

E B

V

22drift cE

E BV

Page 24: American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and

American Physical Society March 6, 2007

Moving Field Lines (nothing to do with plasma physics)

In both the electrostatic and magneto-static case, for symmetric cases you can relatively easily get the motion of field lines simply by conserving flux in source free regions

2 2

2 2

( / ) 0

when /

electric

S C

d dc c

dt dt

c E

E dA B v E dl

v E B

2

( ) 0

when /

magnetic

S C

d d

dt dt

B

B dA E v B dl

v E B

Page 25: American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and

American Physical Society March 6, 2007

Moving Field LinesHelps with higher order concepts, most obviously the

flow of electromagnetic energy, but also the flow of electromagnetic momentum and the stresses transmitted by fields, that is, the Maxwell Stress Tensor

Fields transmit a pressure perpendicular to themselves and a tension parallel to themselves—that is you, can intuit their dynamical effects by looking at their shape!

0 S

emmech dVdt

ddATPP

IBBIEET

���22

2

11

2

1BE

oo

Page 26: American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and

American Physical Society March 6, 2007

Moving Field LinesHelps with higher order concepts, most obviously the

flow of electromagnetic energy, but also the flow of electromagnetic momentum and the stresses transmitted by fields, that is, the Maxwell Stress Tensor

Fields transmit a pressure perpendicular to themselves and a tension parallel to themselves—that is you can intuit their dynamical effects by looking at their shape!

0 S

emmech dVdt

ddATPP

IBBIEET

���22

2

11

2

1BE

oo

Page 27: American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and

American Physical Society March 6, 2007

Dynamic Line Integral Convolution

Can also impose the same field line motion defined above on the line integral convolution method by having the underlying random pattern move with the test particle drift velocity

This is called Dynamic Line Integral Convolution (DLIC), and was originated by Andreas Sundquist

Examples:Falling MagnetOscillating Electric DipoleElectric Dipole turning onLight charges around heavy charge

Page 28: American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and

American Physical Society March 6, 2007

DLIC: Falling Magnet

Page 29: American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and

American Physical Society March 6, 2007

DLIC: Oscillating Electric Dipole

4

ˆ)ˆ(

4

)ˆ(ˆ3

4

)ˆ(ˆ3),(

223 rcrcrt

ooo nxnxppnpnpnpn

rE

Page 30: American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and

American Physical Society March 6, 2007

DLIC: Turning On An Electric Dipole

4

ˆ)ˆ(

4

)ˆ(ˆ3

4

)ˆ(ˆ3),(

223 rcrcrt

ooo nxnxppnpnpnpn

rE

Page 31: American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and

American Physical Society March 6, 2007

DLIC: Light charges around heavy charge

The Seen Versus The Unseen

Link to 10 Meg AviLink to 1 Meg Avi

Page 32: American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and

American Physical Society March 6, 2007

Two Other Visualizations

Electrostatic Video Game Interactive

Page 33: American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and

American Physical Society March 6, 2007

Two Other Visualizations

Generating Plane Waves Interactive

Page 34: American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and

American Physical Society March 6, 2007

How Much Does This Contribute to E&M Understanding?

1. No clear evidence they are useful in the way we have been using them in TEAL

2. Need “Guided Inquiry” with these animations and visualizations, not just accessibility and exploration

3. Build the guided inquiry into e.g. Mastering Physics?4. Carolann Koleci and I have been doing just that in a

junior/senior Griffiths based course at WPI and plan to do a similar study in the corresponding course at MIT

5. Students have to use the visualizations to answer the Mastering Physics questions

6. We are just beginning to explore how to do this effectively and how to evaluate it

Page 35: American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and

American Physical Society March 6, 2007

Page 36: American Physical Society March 6, 2007 The MIT TEAL Simulations and Visualizations in Electromagnetism John W. Belcher Kavli Center for Astrophysics and

American Physical Society March 6, 2007

Applications and software are open source

http://web.mit.edu/viz/soft/