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On the Temporal Changes of Helioseismic Properties Derived with - - PowerPoint PPT Presentation

On the Temporal Changes of Helioseismic Properties Derived with Different Mode Fitting Techniques SPD 2016 Meeting Boulder, CO S.G. Korzennik Harvard-Smithsonian Center for Astrophysics, USA. May 2016 S.G. Korzennik (CfA) Temporal


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SLIDE 1

On the Temporal Changes of Helioseismic Properties Derived with Different Mode Fitting Techniques

SPD 2016 Meeting — Boulder, CO S.G. Korzennik

Harvard-Smithsonian Center for Astrophysics, USA.

May 2016

S.G. Korzennik (CfA) Temporal Changes, Different Techniques May 2016 1 / 18

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Introduction

Introduction

◮ 3 methodologies, 2 data sets, 20 years of observations:

NSO SU CfA sym. asym. sym. asym. sym. asym. GONG √ ⋆ × × √ √ MDI+HMI × × √ √ √ √ ⋆: preliminary results, tables not available.

◮ Raw mode comparisons

◮ Frequency ◮ Scaling ◮ Attrition ◮ Singlets to multiplets reduction ◮ Change of mean weighted frequency ◮ Line-width, Asymmetry

◮ Rotation inversion comparison ◮ Conclusions

S.G. Korzennik (CfA) Temporal Changes, Different Techniques May 2016 2 / 18

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SLIDE 3

Raw Comparisons: Frequency

Frequency

◮ δν: change wrt to time, hence activity; ◮ Raw <δν> sensitive to mode set, i.e.: {n, ℓ} ◮ Weighted mean frequency shift:

◮ relative mode mass (Qn,ℓ): mass of volume sampled; ◮ by uncertainty (“tradition”), why? ◮ More physical scaling: line-width (Γ) or power (P = AΓ)

◮ Weighting does not remove dependency on either ν, ℓ or log(ν/L). ◮ Mode attrition complicates comparisons (need common mode set).

S.G. Korzennik (CfA) Temporal Changes, Different Techniques May 2016 3 / 18

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SLIDE 4

Raw Comparisons: Frequency

Frequency Scaling

◮ Scaled frequency changes for 3 epochs and 3 weightings: Q, Q/Γ & Q/P

S.G. Korzennik (CfA) Temporal Changes, Different Techniques May 2016 4 / 18

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SLIDE 5

Raw Comparisons: Frequency

Frequency Comparison

◮ Scaled frequency changes, (δνQ/P), as measured by 7 different fitting method.

S.G. Korzennik (CfA) Temporal Changes, Different Techniques May 2016 5 / 18

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SLIDE 6

Raw Comparisons: Frequency

Attrition

◮ Mode attrition for different fitting methodologies

S.G. Korzennik (CfA) Temporal Changes, Different Techniques May 2016 6 / 18

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SLIDE 7

Raw Comparisons: Frequency

Singlets to multiplets reduction

νn,ℓ,m = Σiciβ

m(i) →

   νn,ℓ = c0β

0(0)

  • r

νn,ℓ,0 = Σiciβ

0(i) ◮ The quantity ∆0 ν = νn,ℓ − νn,ℓ,0 is a strong function of ν and solar activity. ◮ Explains past discrepancy between <δνn,ℓ,0> (CfA) and <δνn,ℓ> (NSO & SU). ◮ Adopted <δνn,ℓ> (which quantity means what?).

S.G. Korzennik (CfA) Temporal Changes, Different Techniques May 2016 7 / 18

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SLIDE 8

Raw Comparisons: Frequency

Change of frequency, δνn,ℓ,0

S.G. Korzennik (CfA) Temporal Changes, Different Techniques May 2016 8 / 18

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SLIDE 9

Raw Comparisons: Frequency

Change of frequency, δνn,ℓ, symmetric profiles

S.G. Korzennik (CfA) Temporal Changes, Different Techniques May 2016 9 / 18

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SLIDE 10

Raw Comparisons: Frequency

Change of frequency, δνn,ℓ, asymmetric profiles

S.G. Korzennik (CfA) Temporal Changes, Different Techniques May 2016 10 / 18

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SLIDE 11

Raw values: line-width, asymmetry

Line-width

◮ Top: GONG data (NSO & CfA), bottom: MDI+HMI data (SU & CfA)

S.G. Korzennik (CfA) Temporal Changes, Different Techniques May 2016 11 / 18

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SLIDE 12

Raw values: line-width, asymmetry

Asymmetry

◮ Mean change of weighted asymmetry, δα Q

S.G. Korzennik (CfA) Temporal Changes, Different Techniques May 2016 12 / 18

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Rotation Inversions Comparison

Propagation Diagrams: my fitting to MDI+HMI

S.G. Korzennik (CfA) Temporal Changes, Different Techniques May 2016 13 / 18

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Rotation Inversions Comparison

Collage: my fitting to MDI+HMI

S.G. Korzennik (CfA) Temporal Changes, Different Techniques May 2016 14 / 18

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Rotation Inversions Comparison

Collage: SU’s fitting to MDI+HMI

S.G. Korzennik (CfA) Temporal Changes, Different Techniques May 2016 15 / 18

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Rotation Inversions Comparison

Collage: NSO’s fitting to GONG

S.G. Korzennik (CfA) Temporal Changes, Different Techniques May 2016 16 / 18

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Conclusions

Conclusions

◮ Raw Frequencies, Line-width Asymmetry, Amplitudes & Background

◮ Very different dependence of δν on ν between symmetric and asymmetric fits. ◮ Very different attrition patterns. ◮ Much better agreement when using consistently <δνn,ℓ>; ◮ my symmetric fit matches NSO’s and SU’s magnitude; ◮ my asymmetric fit leads to a small decrease in the magnitude of change. ◮ Line-width: Inconsistent results between data and methods. ◮ Asymmetry: inconsistent results between methods, consistent results between data (CfA) ◮ A & B: inconsistent results.

◮ Rotation Inversions

◮ Cycle 24 is different from Cycle 23; ◮ un-physical twist at high latitudes when inverting SU’s or NSO’s results. S.G. Korzennik (CfA) Temporal Changes, Different Techniques May 2016 17 / 18

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The End

The End

S.G. Korzennik (CfA) Temporal Changes, Different Techniques May 2016 18 / 18