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INVERSIONS FOR AVERAGE SUPERGRANULAR FLOWS USING FINITE-FREQUENCY KERNELS

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F12%3A10128769" target="_blank" >RIV/00216208:11320/12:10128769 - isvavai.cz</a>

  • Alternative codes found

    RIV/67985815:_____/12:00388115

  • Result on the web

    <a href="http://dx.doi.org/10.1088/2041-8205/759/2/L29" target="_blank" >http://dx.doi.org/10.1088/2041-8205/759/2/L29</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1088/2041-8205/759/2/L29" target="_blank" >10.1088/2041-8205/759/2/L29</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    INVERSIONS FOR AVERAGE SUPERGRANULAR FLOWS USING FINITE-FREQUENCY KERNELS

  • Original language description

    I analyze the maps recording the travel-time shifts caused by averaged plasma anomalies under an "average supergranule," constructed by means of statistical averaging over 5582 individual supergranules with large divergence signals detected in two monthsof Helioseismic and Magnetic Imager Dopplergrams. By utilizing a three-dimensional validated time-distance inversion code, I measure a peak vertical velocity of 117 +/- 2 m s(-1) at depths around 1.2 Mm in the center of the supergranule and a root-mean-square vertical velocity of 21 m s(-1) over the area of the supergranule. A discrepancy between this measurement and the measured surface vertical velocity ( a few m s(-1)) can be explained by the existence of the large-amplitude vertical flow under thesurface of supergranules with large divergence signals, recently suggested by Duvall & Hanasoge.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

  • CEP classification

    BN - Astronomy and celestial mechanics, astrophysics

  • OECD FORD branch

Result continuities

  • Project

    Result was created during the realization of more than one project. More information in the Projects tab.

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2012

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Astrophysical Journal Letters

  • ISSN

    2041-8205

  • e-ISSN

  • Volume of the periodical

    759

  • Issue of the periodical within the volume

    2

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    5

  • Pages from-to

  • UT code for WoS article

    000310581600003

  • EID of the result in the Scopus database