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Artificial ‘Physics- light’ Ring Data Rachel Howe, Irene Gonzalez-Hernandez, and Frank Hill

Artificial ‘Physics-light’ Ring Data Rachel Howe, Irene Gonzalez-Hernandez, and Frank Hill

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Page 1: Artificial ‘Physics-light’ Ring Data Rachel Howe, Irene Gonzalez-Hernandez, and Frank Hill

Artificial ‘Physics-light’ Ring Data

Rachel Howe,

Irene Gonzalez-Hernandez, and

Frank Hill

Page 2: Artificial ‘Physics-light’ Ring Data Rachel Howe, Irene Gonzalez-Hernandez, and Frank Hill

Roadmap

1. Noise free power spectra, with and without uniform flow field

2. Power spectra with realization noise

3. Inverse transform to wave fields with realization noise.

4. Projection effects

5. Seeing

Page 3: Artificial ‘Physics-light’ Ring Data Rachel Howe, Irene Gonzalez-Hernandez, and Frank Hill

Noise-free power spectra

• Based on Frank Hill’s old code• Lorentzian peaks• 2arcsec/pixel, 60s cadence, k=3.338e-5• 128 128 2048 power spec.• 0 n 11, 100 l 1440• Kernels from model S to put in flows• Widths and amplitudes based on simple model• Second attempt with reduced widths

Page 4: Artificial ‘Physics-light’ Ring Data Rachel Howe, Irene Gonzalez-Hernandez, and Frank Hill

Noisy Power Spectra

• Add two normally-distributed pseudo-random numbers in quadrature, multiply by power spectrum (to give 2d.o.f. statistics).

• Both clean and noisy spectra, with and without a flow field, are available as FITS files (67Mb)

• Realization noise only, no instrumental or ‘background’.

Page 5: Artificial ‘Physics-light’ Ring Data Rachel Howe, Irene Gonzalez-Hernandez, and Frank Hill

Rings at bin 500/2048 (4mHz)

Wide Rings Narrow Rings

Page 6: Artificial ‘Physics-light’ Ring Data Rachel Howe, Irene Gonzalez-Hernandez, and Frank Hill

l- slices

Wide Rings Narrow Rings

Page 7: Artificial ‘Physics-light’ Ring Data Rachel Howe, Irene Gonzalez-Hernandez, and Frank Hill

Fitting/Inversion Tests

• Power spectra were fitted with the ‘doglegfit’ code used for the real data.

• RLS inversions, as for real data.

Page 8: Artificial ‘Physics-light’ Ring Data Rachel Howe, Irene Gonzalez-Hernandez, and Frank Hill

Fit results – frequencies

WideWide Narrow

Page 9: Artificial ‘Physics-light’ Ring Data Rachel Howe, Irene Gonzalez-Hernandez, and Frank Hill

Frequency differences from ‘truth’

Page 10: Artificial ‘Physics-light’ Ring Data Rachel Howe, Irene Gonzalez-Hernandez, and Frank Hill

Widths from single power spectra

Page 11: Artificial ‘Physics-light’ Ring Data Rachel Howe, Irene Gonzalez-Hernandez, and Frank Hill

Amplitudes from single power spectra

Page 12: Artificial ‘Physics-light’ Ring Data Rachel Howe, Irene Gonzalez-Hernandez, and Frank Hill

Inferred Flows (wide rings)

Page 13: Artificial ‘Physics-light’ Ring Data Rachel Howe, Irene Gonzalez-Hernandez, and Frank Hill

Inferred Flows (narrow rings)

Page 14: Artificial ‘Physics-light’ Ring Data Rachel Howe, Irene Gonzalez-Hernandez, and Frank Hill

Thoughts on results so far

• Narrower rings give fewer successful fits, but better-quality ones.

• Narrow rings are probably too narrow to be realistic.

• Effects of error correlations evident in inversions of noisy results.

Page 15: Artificial ‘Physics-light’ Ring Data Rachel Howe, Irene Gonzalez-Hernandez, and Frank Hill

Noisy Wave Field• NB – un-noisy wave fields no good, need random

phases to make it work.• Make 1024 1024 2048 power spectrum, one

layer at a time.• Make real and imaginary parts by multiplying

spectrum by Gaussian random numbers• 2 Fourier transforms in space, store spatial

transforms.• Make Hermitian and do transform in time• Save as 128 128 2048 FITS files (64 off) –

134Mb each, rudimentary headers

Page 16: Artificial ‘Physics-light’ Ring Data Rachel Howe, Irene Gonzalez-Hernandez, and Frank Hill

Wavefield in action

• 256 frames of the time series

• Takes about 8 hours compute time for 64 patches.

Page 17: Artificial ‘Physics-light’ Ring Data Rachel Howe, Irene Gonzalez-Hernandez, and Frank Hill

Flows from time series (narrow)

Page 18: Artificial ‘Physics-light’ Ring Data Rachel Howe, Irene Gonzalez-Hernandez, and Frank Hill

Modes with consistently ‘sensible’ widths in 8 patches

Page 19: Artificial ‘Physics-light’ Ring Data Rachel Howe, Irene Gonzalez-Hernandez, and Frank Hill

Conclusions

• Power spectra work reasonably well.

• Widths need fine-tuning

• Something isn’t right with the time series – precision problems with FFTs?

• Need more computers!

Page 20: Artificial ‘Physics-light’ Ring Data Rachel Howe, Irene Gonzalez-Hernandez, and Frank Hill

Time Distance from Artificial Data

Shukur Kholikov and Rachel Howe

Page 21: Artificial ‘Physics-light’ Ring Data Rachel Howe, Irene Gonzalez-Hernandez, and Frank Hill

TD-test

• 128 128 2048 artificial time series

• Narrow-ring version, no flows

• Set does not contain lower-l information

• S. Kholikov’s time distance code

• Fit for ‘phase’ and ‘envelope’ travel times.

Page 22: Artificial ‘Physics-light’ Ring Data Rachel Howe, Irene Gonzalez-Hernandez, and Frank Hill

TD—more details

• Cross-correlation function of artificial data computed for the angular distance [1.1, 3.5].

• Then Gabor-fitting parameters obtained to compare travel times with GONG data. Only one realization of artificial data used (2048 min) from 15x15 region. So, using bigger region and more realizations could smooth envelope travel time curve too.

• Also, I found that correlation amplitude in case of artificial data is little different from real observations which can come from power distribution used to simulate artificial power spectrum.

Page 23: Artificial ‘Physics-light’ Ring Data Rachel Howe, Irene Gonzalez-Hernandez, and Frank Hill

Time-distance curve

Phase

Envelope