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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


  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

  2. 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

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

  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

  5. Raw Comparisons: Frequency Frequency Comparison ◮ Scaled frequency changes, ( δν Q / P ), as measured by 7 different fitting method. S.G. Korzennik (CfA) Temporal Changes, Different Techniques May 2016 5 / 18

  6. Raw Comparisons: Frequency Attrition ◮ Mode attrition for different fitting methodologies S.G. Korzennik (CfA) Temporal Changes, Different Techniques May 2016 6 / 18

  7. Raw Comparisons: Frequency Singlets to multiplets reduction ℓ  ν n ,ℓ = c 0 β 0 ( 0 )  ℓ ν n ,ℓ, m = Σ i c i β m ( i ) → or ℓ  ν n ,ℓ, 0 = Σ i c i β 0 ( i ) ◮ The quantity ∆ 0 ν = ν n ,ℓ − ν n ,ℓ, 0 is a strong function of ν and solar activity. ◮ Explains past discrepancy between <δν n ,ℓ, 0 > (CfA) and <δν n ,ℓ > (NSO & SU). ◮ Adopted <δν n ,ℓ > (which quantity means what?). S.G. Korzennik (CfA) Temporal Changes, Different Techniques May 2016 7 / 18

  8. Raw Comparisons: Frequency Change of frequency, δν n ,ℓ, 0 S.G. Korzennik (CfA) Temporal Changes, Different Techniques May 2016 8 / 18

  9. Raw Comparisons: Frequency Change of frequency, δν n ,ℓ , symmetric profiles S.G. Korzennik (CfA) Temporal Changes, Different Techniques May 2016 9 / 18

  10. Raw Comparisons: Frequency Change of frequency, δν n ,ℓ , asymmetric profiles S.G. Korzennik (CfA) Temporal Changes, Different Techniques May 2016 10 / 18

  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

  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

  13. Rotation Inversions Comparison Propagation Diagrams: my fitting to MDI+HMI S.G. Korzennik (CfA) Temporal Changes, Different Techniques May 2016 13 / 18

  14. Rotation Inversions Comparison Collage: my fitting to MDI+HMI S.G. Korzennik (CfA) Temporal Changes, Different Techniques May 2016 14 / 18

  15. Rotation Inversions Comparison Collage: SU’s fitting to MDI+HMI S.G. Korzennik (CfA) Temporal Changes, Different Techniques May 2016 15 / 18

  16. Rotation Inversions Comparison Collage: NSO’s fitting to GONG S.G. Korzennik (CfA) Temporal Changes, Different Techniques May 2016 16 / 18

  17. 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 <δν n ,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

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

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