Doug Nychka, CISL Sarah Gibson, HAO Kevin Dalmasse, HAO, CISL - - PowerPoint PPT Presentation

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Doug Nychka, CISL Sarah Gibson, HAO Kevin Dalmasse, HAO, CISL - - PowerPoint PPT Presentation

Doug Nychka, CISL Sarah Gibson, HAO Kevin Dalmasse, HAO, CISL Variations over time Flares CMEs Small-scale variation Corona Hydrogen ~ 91% Helium ~ 8.7% Oxygen ~ .078% Carbon ~ .043% Silicon ~ .0045%


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SLIDE 1

Doug Nychka, CISL Sarah Gibson, HAO Kevin Dalmasse, HAO, CISL

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SLIDE 2

Variations over time

  • Flares
  • CMEs
  • Small-scale variation
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SLIDE 3

Corona

  • Hydrogen ~ 91%
  • Helium ~ 8.7%
  • Oxygen ~ .078%
  • Carbon ~ .043%
  • Silicon ~ .0045%
  • Iron ~ .0030%
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SLIDE 4

What we have to work with:

  • White-light images
  • 2-D images at different angles
  • Projection on the “plane of sky”

(POS defined by observer’s location)

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SLIDE 5

Optically Thin Optically Thick

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SLIDE 6

Sun Corona Us

Brightness Electron Density Scattering

View from north pole Plane of Sky

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SLIDE 7

Tomography

The reconstruction of an object

  • f N dimensions through a series
  • f M-dimensional slices or
  • bservations where M < N.

Examples:

  • MRI
  • Ocean Acoustic Tomography
  • Quantum State Tomography
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SLIDE 8

Radial Basis Functions

Basis vectors spanning a vector space Sines and cosines describing a function

Combination of functions X constants

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SLIDE 9

3D Lattice

Spatial Dimensions “radius” defined by α

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Basis Functions

Basis function node location Point in space Value of basis function Distance in normalized space α = “radius” of influence

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SLIDE 11

x (points in space) b (node locations) b (node locations)

Looking down from north pole (polar plot)

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SLIDE 12

Basis Functions

Integral and Sum Form

Kth line of sight

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SLIDE 13

Matrix Form

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SLIDE 14

Major algorithms in program

  • Determine LOS sample points
  • Find basis functions in range
  • Compute integral

Computing A

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Determining LOS sample points

View from north pole

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Find Basis Functions in Range

Radial Polar

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  • 1. Can invert pB to get c, and thus Ne
  • 2. Allows us to check accuracy of the modeling method
  • Model with known density
  • Get c coefficients
  • Use c coefficients to get pB
  • Do inversion with pB to get new set of c coefficients (c*)
  • Compare c to c*
  • Minimize:
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SLIDE 18

Ground truth

Reconstructed density with 24522 basis functions

Step 1: Model with known density Step 2: Obtain c coefficients

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SLIDE 19

Step 3: Use c coefficients to get pB

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Step 4: Do inversion with pB to get new set of c coefficients (c*)

426 Basis Functions 12 Viewing angles 100 LOS per angle 10873 Basis Functions 18 Viewing angles 360 LOS per angle 24522 Basis Functions 30 Viewing angles 400 LOS per angle

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SLIDE 21

Mean square error: 3.1 Average error: -.27 Mean square error: .24 Average error: .0017 Mean square error: .012 Average error: -.00014

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SLIDE 22

Predictive Science Model

  • Boundary-driven model
  • Solve through MHD equations
  • Provides density at all points
  • Datacube available for each

solar rotation (chosen to match data)

View from Earth

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SLIDE 23

Mean square error: 1.01 e8 Average error: -2.6 e6

View from north pole

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SLIDE 24

Final Milestone

Applying our method to actual data Completed Future Work

  • Some assessment of accuracy
  • Data Collection
  • Program to build A-matrix
  • Finish 2D testing
  • Extend testing to three dimensions
  • Finish R-C interface
  • Perform method with real data
  • Consider further improvements (?)

View from Earth (pB)