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p3d: Magnetic Reconnection via an Electromagnetic PIC Code

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J. Drake, M. Shay Magnetic Reconnection. Hall MHD. B. Dorland Collisionless magnetized turbulence ... It only agrees with real-life reconnection after some ... – PowerPoint PPT presentation

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Title: p3d: Magnetic Reconnection via an Electromagnetic PIC Code


1
p3d Magnetic Reconnection via an Electromagnetic
PIC Code
  • Marc Swisdak
  • IREAP, University of Maryland
  • NERSC User Group Meeting
  • Argonne National Laboratory
  • May 29, 2003

2
One of Many Codes
  • J. Drake, M. Shay Magnetic Reconnection
  • Hall MHD
  • B. Dorland Collisionless magnetized turbulence
  • Gyrokinetic
  • B. Kleva Tokamak edge turbulence
  • Braginskii fluid

3
Magnetic Reconnection A process whereby magnetic
energy, B2, is converted into thermal and
kinetic energy, kBT and ?v2.
4
Cartoon Reconnection
5
Magnetic Reconnection is Ubiquitous
6
Q Why PIC? A Its closer to the real physics.
  • The major alternative, MHD, is a fluid
    approximation. It only agrees with real-life
    reconnection after some unnatural tweaking.
  • Small spatial and short temporal scales,
    turbulence and wave-particle interactions in
    particular, are completely missed.

7
Equations
Maxwell
Newton-Lorentz
8
Algorithms
  • Gridded electromagnetic fields advanced by
    trapezoidal leapfrog, the (possibly relativistic)
    particles with a Boris algorithm.
  • Discretization errors accumulate to form a
    secular violation of Poissons equation
  • This can be solved via FFTs, but they make BCs
    more difficult and have some parallelization
    issues. The multigrid treats the different
    scales on different grids, each with an
    appropriate timestep.

9
Scaling
  • ? 50 slower at 1024 than at 16 processors
  • Efficiency About 20 of maximum at 1 processor,
    ? 8 for 1024 processors

10
3-D Magnetic Reconnection
  • Recent work Drake et al. Formation of
    Electron Holes and Particle Energization in
    Magnetic Reconnection, Science, 299, 873, 2003.
  • Followup run 15 hours on 64 nodes (1024
    processors)

Jz
11
Turbulence at the X-line
  • Electron holes and associated wave-particle
    interactions can have a significant effect on the
    progression of reconnection.

Ez
12
Future Challenges
  • Comparisons with data
  • Particle heating
  • Observations of turbulence
  • Larger domains
  • Connect with fluid codes
  • What can be said about the global aspects of
    reconnection?
  • Managing output
  • Movies
  • Initialization/restart files

13
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