Local helioseismology at small scales - PowerPoint PPT Presentation

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Local helioseismology at small scales

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(Horizontally) high-resolution view of the solar interior. For more details, ask Katsukawa-san ... High-resolution local helioseismology (3/4) ... – PowerPoint PPT presentation

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Title: Local helioseismology at small scales


1
Local helioseismologyat small scales
Takashi Sekii (NAOJ)
2
I am talking about
  • How SDO and Solar-B can work together for
    high-resolution local helioseismology, for
    subphotospheric dynamics
  • What kind of challenges are ahead

3
Solar-B
  • A J/US/UK/European collaboration
  • To be launched in September 2006

4
Solar Optical Telescope
  • 50-cm Solar Optical Telescope (SOT) produces
    high-resolution Dopplergrams that can be used for
    local helioseismology
  • FOV narrow but high spatial resolution
  • Not suited for probing deep layers
  • (Horizontally) high-resolution view of the solar
    interior
  • For more details, ask Katsukawa-san

5
HMI and SOT
  • Spatial resolution and FOV
  • HMI/SDO 1 arcsec, the entire disc
  • SOT/Solar-B 0.2 arcsec, 328x164()
  • size of individual flux tubes 100-300km (0.2
    arcsec150km)
  • HMI/SOT Simultaneous observation will be very
    useful as it combines broader coverage (HMI) and
    higher resolution (SOT)

6
High-resolution local helioseismology (1/4)
  • Is it worth doing?
  • Is there any wavefield power at such a small
    scale?

7
High-resolution local helioseismology (2/4)
  • MDI high-resolution power spectrum
  • No resonant p modes above l2000
  • The f-mode frequency ? sqrt(l)

8
High-resolution local helioseismology (3/4)
  • Sekii et al 2001 MDII(left) versus La Palma
    SVST G-band (right, Berger et al 1998)

9
High-resolution local helioseismology (4/4)
  • La Palma result shows improvement in (mainly
    p-mode) time-distance S/N in lt10,000 km range,
    down to lt1,000km
  • Local helioseismology with high-degree f modes is
    an obvious thing to do, but p-mode seismology
    will also benefits from higher-resolution

10
Challenges (1/2)
  • Propagation of waves in magnetized fluid when
    wavelength is similar to the size of individual
    flux tubes
  • And use them for diagnostic purpose
  • Can we observe kernels? (Duvall, Gizon Birch)

11
Challenges (2/2)
  • What is the smartest way to merge f-mode data and
    p-mode data (or do we just merge them)
  • Similarly, how do we merge HMI data and SOT data?
  • T-d analysis in magnetic regions
  • Comparing magnetic-line data (HMI SOT) and
    non-magnetic-line data (SOT) should be useful
    (not just for HR stuff!)
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