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Comparison of solar horizontal velocity fields from SDO/HMI and Hinode data

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F13%3A10174146" target="_blank" >RIV/00216208:11320/13:10174146 - isvavai.cz</a>

  • Alternative codes found

    RIV/67985815:_____/13:00421332

  • Result on the web

    <a href="http://dx.doi.org/10.1051/0004-6361/201220867" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201220867</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1051/0004-6361/201220867" target="_blank" >10.1051/0004-6361/201220867</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Comparison of solar horizontal velocity fields from SDO/HMI and Hinode data

  • Original language description

    Context. The measurement of the Sun's surface motions with a high spatial and temporal resolution is still a challenge. Aims. We wish to validate horizontal velocity measurements all over the visible disk of the Sun from Solar Dynamics Observatory/Helioseismic and Magnetic Imager (SDO/HMI) data. Methods. Horizontal velocity fields are measured by following the proper motions of solar granules using a newly developed version of the coherent structure tracking (CST) code. The comparison of the surface flows measured at high spatial resolution (Hinode, 0.1 arcsec) and low resolution (SDO/HMI, 0.5 arcsec) allows us to determine corrections to be applied to the horizontal velocity measured from HMI white light data. Results. We derive horizontal velocity maps with spatial and temporal resolutions of respectively 2.5 Mm and 30 min. From the two components of the horizontal velocity v(x) and v(y) measured in the sky plane and the simultaneous line of sight component from SDO/HMI dopplergrams

  • 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

    <a href="/en/project/GPP209%2F12%2FP568" target="_blank" >GPP209/12/P568: Convection and plasma motions in the near-surface layers of the solar convection zone</a><br>

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2013

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Astronomy and Astrophysics

  • ISSN

    0004-6361

  • e-ISSN

  • Volume of the periodical

    552

  • Issue of the periodical within the volume

    duben

  • Country of publishing house

    FR - FRANCE

  • Number of pages

    7

  • Pages from-to

  • UT code for WoS article

    000317912000112

  • EID of the result in the Scopus database