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Coupling the RCM to LFM

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Pressure in the inner magnetosphere starts to symmetrize as particles gradient ... flux tubes low pVg flux tubes being squirted into the inner magnetosphere ... – PowerPoint PPT presentation

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Tags: lfm | rcm | coupling | inner | populate

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Title: Coupling the RCM to LFM


1
Coupling the RCM to LFM
  • Frank Toffoletto (Rice)
  • and
  • John Lyon (Dartmouth)

2
RCM - LFM Coupling
  • This is the result of a prelimimary test on
    one-way coupling
  • We have used 1 MHD snapshot to provide input data
    to the RCM
  • RCM uses MHD computed magnetic field (for flux
    tube volumes), pressure and density
  • Pressure and density are used to estimate
    temperature
  • These variables in turn are used to populate the
    initial distribution function

3
The RCM equations
  • The RCM advects each fluid by solving

4
Coupling process
  • LFM data is interpolated onto a regular grid
  • This allows for reasonably fast calculations when
    computing such RCM variables as flux tube volume
  • The ionospheric electric field for these runs is
    not taken from the MHD

5
Mapped RCM grid (equatorial plane) using LFM
Magnetic field
6
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7
RCM pressure
8
RCM Computed ion temperatures
9
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10
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11
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12
Results
  • After 4hours R-2 currents form leading to some
    shielding of the electric field
  • Pressure in the inner magnetosphere starts to
    symmetrize as particles gradient and curvature
    drift
  • Channels of low content flux tubes low pVg flux
    tubes being squirted into the inner magnetosphere

13
Next Step
  • Incorporate MHD computed potential boundary
    conditions and conductivities
  • Use a time-sequence of MHD inputs to do a more
    realistic run

14
Final Comment
  • This was a test to see how the RCM would react to
    MHD input data
  • Two way coupling is a ways off, but some of the
    computational machinery is in place and just
    needs to be turned out
  • Exchange will be with data files
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