Updates on Measurements of the Wavefunctions of Solar Acoustic Waves Scattered by Sunspot

20
Updates on Measurements of the Wavefunctions of Solar Acoustic Waves Scattered by Sunspot Hui Zhao 1 Collaborators: Dean-Yi Chou 2 Ming-Hsu Yang 2 Zhi-Chao Liang 2 1 National Astronomical Observatory, Chinese Academy of Scienc NAOC, 25 August 2012 2 National Tsing Hua University, Taiwan

description

Updates on Measurements of the Wavefunctions of Solar Acoustic Waves Scattered by Sunspot. Hui Zhao 1 Collaborators: Dean-Yi Chou 2 Ming-Hsu Yang 2 Zhi-Chao Liang 2. 1 National Astronomical Observatory, Chinese Academy of Sciences. 2 National Tsing Hua University, Taiwan. - PowerPoint PPT Presentation

Transcript of Updates on Measurements of the Wavefunctions of Solar Acoustic Waves Scattered by Sunspot

Page 1: Updates on Measurements of the Wavefunctions of Solar Acoustic Waves Scattered by Sunspot

Updates on Measurements of the Wavefunctions of Solar Acoustic Waves Scattered by

Sunspot

Hui Zhao1

Collaborators:Dean-Yi Chou2

Ming-Hsu Yang2

Zhi-Chao Liang2

1National Astronomical Observatory, Chinese Academy of Sciences

NAOC, 25 August 2012

2National Tsing Hua University, Taiwan

Page 2: Updates on Measurements of the Wavefunctions of Solar Acoustic Waves Scattered by Sunspot

The interaction of the acoustic waves with the magnetic region : Two views

a. The incident wave is modified as it enters the magnetic region. This modification in the wave inside the magnetic region yields a change in the wave around the magnetic region.

b. The magnetic region generates a scattered wave as the incident wave perturbs the magnetic region. This scattered wave is added to the incident wave to yield the total wave in and around the magnetic region.

Page 3: Updates on Measurements of the Wavefunctions of Solar Acoustic Waves Scattered by Sunspot

Equations for Interaction of Waves with Magnetic Regions Equations for Interaction of Waves with Magnetic Regions

quiet Sun

magnetic region

Page 4: Updates on Measurements of the Wavefunctions of Solar Acoustic Waves Scattered by Sunspot

where S is the source describing the interaction.

Solve the inhomogeneous equation:

Need an incident wave propagating toward of the sunspot.

The conceptually simplest incident wave is the one propagating horizontally in a certain direction.

Page 5: Updates on Measurements of the Wavefunctions of Solar Acoustic Waves Scattered by Sunspot

Cameron, Gizon & Duvall (2008)Cameron, Gizon & Duvall (2008)

2. The incident wave is the line-averaged 2. The incident wave is the line-averaged signal, which is a plane wave packet. signal, which is a plane wave packet.

3. Cross-correlation between the 3. Cross-correlation between the reference line and each pointreference line and each point

1. Signals on a ridge (fixed n) are 1. Signals on a ridge (fixed n) are isolated to obtain horizontal waves. isolated to obtain horizontal waves.

Page 6: Updates on Measurements of the Wavefunctions of Solar Acoustic Waves Scattered by Sunspot

The cross-correlation function relates to the wave function, but is not the wave function!!!

denominator

Page 7: Updates on Measurements of the Wavefunctions of Solar Acoustic Waves Scattered by Sunspot

NOAA 11084: 29 June – 5 July 2010 (12,402 frames)NOAA 11092: 30 July – 7 August 2010 (13,616 frames)

DATADATA : : NOAAs NOAAs 11084 11092 11084 11092 (HMI) (HMI)

Stable

axisymmetric

Clean around

Page 8: Updates on Measurements of the Wavefunctions of Solar Acoustic Waves Scattered by Sunspot

CCF vs. Wave Function

AR11092

p2 modes

Different :

Amplitude

Phase

Width

Dispersion

Page 9: Updates on Measurements of the Wavefunctions of Solar Acoustic Waves Scattered by Sunspot

Incident Waves, Total Wave, Scattered WaveIncident Waves, Total Wave, Scattered Wave

Page 10: Updates on Measurements of the Wavefunctions of Solar Acoustic Waves Scattered by Sunspot

Scattered wave : p2 modes

The curvature of AR11084 is greater than that of AR11092

Page 11: Updates on Measurements of the Wavefunctions of Solar Acoustic Waves Scattered by Sunspot

Scattered wave : f modes

Have No obviously curvature

Page 12: Updates on Measurements of the Wavefunctions of Solar Acoustic Waves Scattered by Sunspot

Scattered wave : p5 modes

The curvature of p5 modes is greater than that of p2 modes

Page 13: Updates on Measurements of the Wavefunctions of Solar Acoustic Waves Scattered by Sunspot

Updated results• Phase speed filter

Page 14: Updates on Measurements of the Wavefunctions of Solar Acoustic Waves Scattered by Sunspot

Phase speed filter : l=300

Page 15: Updates on Measurements of the Wavefunctions of Solar Acoustic Waves Scattered by Sunspot

Phase speed filter : l=200

Page 16: Updates on Measurements of the Wavefunctions of Solar Acoustic Waves Scattered by Sunspot

Updated resultsScattering from n to n’

f

p1p2

p3p4p5

Page 17: Updates on Measurements of the Wavefunctions of Solar Acoustic Waves Scattered by Sunspot

Scatter wave : p2 to p1 and p3

Page 18: Updates on Measurements of the Wavefunctions of Solar Acoustic Waves Scattered by Sunspot

Mode Conversion

• Scattering : n n (n, kx, ky) (n, kx’, ky’)

ω does not change. (kx2+ky2=kx’2+ky’2) k changes direction.• Scattering : n n’ (n, kx, ky) (n’, kx’, ky’) ω does not change. |k| changes.

Page 19: Updates on Measurements of the Wavefunctions of Solar Acoustic Waves Scattered by Sunspot

The End

Page 20: Updates on Measurements of the Wavefunctions of Solar Acoustic Waves Scattered by Sunspot

Direction filter

AR11084, p2 modes, time=0 / plot : reference line