SENSITIVITY KERNELS for FLOWS in TIME-DISTANCE HELIOSEISMOLOGY

EXTENSION to SPHERICAL GEOMETRY

Vincent G.A. B�ning, Markus Roth, Wolfgang Zima, Aaron C. Birch, Laurent Gizon

    Research output: Contribution to journalArticle

    Abstract

    We extend an existing Born approximation method for calculating the linear sensitivity of helioseismic travel times to flows from Cartesian to spherical geometry. This development is necessary for using the Born approximation for inferring large-scale flows in the deep solar interior. As first sanity check, we compare two f-mode kernels from our spherical method and from an existing Cartesian method. The horizontal and total integrals agree to within 0.3%. As a second consistency test, we consider a uniformly rotating Sun and a travel distance of 42�. The analytical travel-time difference agrees with the forward-modeled travel-time difference to within 2%. In addition, we evaluate the impact of different choices of filter functions on the kernels for a meridional travel distance of 42�. For all filters, the sensitivity is found to be distributed over a large fraction of the convection zone. We show that the kernels depend on the filter function employed in the data analysis process. If modes of higher harmonic degree (90 ≲ l ≲ 170) are permitted, a noisy pattern of a spatial scale corresponding to l ≈ 260 appears near the surface. When mainly low-degree modes are used (l ≲ 70), the sensitivity is concentrated in the deepest regions and it visually resembles a ray-path-like structure. Among the different low-degree filters used, we find the kernel for phase-speed-filtered measurements to be best localized in depth.

    Original languageEnglish (US)
    Article number49
    JournalAstrophysical Journal
    Volume824
    Issue number1
    DOIs
    StatePublished - Jun 10 2016

    Fingerprint

    helioseismology
    travel
    travel time
    filter
    Born approximation
    filters
    sensitivity
    solar interior
    convection
    rays
    sun
    geometry
    harmonics
    method
    approximation

    Keywords

    • scattering
    • Sun: helioseismology
    • Sun: interior
    • Sun: oscillations
    • waves

    ASJC Scopus subject areas

    • Astronomy and Astrophysics
    • Space and Planetary Science

    Cite this

    SENSITIVITY KERNELS for FLOWS in TIME-DISTANCE HELIOSEISMOLOGY : EXTENSION to SPHERICAL GEOMETRY. / B�ning, Vincent G.A.; Roth, Markus; Zima, Wolfgang; Birch, Aaron C.; Gizon, Laurent.

    In: Astrophysical Journal, Vol. 824, No. 1, 49, 10.06.2016.

    Research output: Contribution to journalArticle

    B�ning, Vincent G.A. ; Roth, Markus ; Zima, Wolfgang ; Birch, Aaron C. ; Gizon, Laurent. / SENSITIVITY KERNELS for FLOWS in TIME-DISTANCE HELIOSEISMOLOGY : EXTENSION to SPHERICAL GEOMETRY. In: Astrophysical Journal. 2016 ; Vol. 824, No. 1.
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