All

What are you looking for?

All
Projects
Results
Organizations

Quick search

  • Projects supported by TA ČR
  • Excellent projects
  • Projects with the highest public support
  • Current projects

Smart search

  • That is how I find a specific +word
  • That is how I leave the -word out of the results
  • “That is how I can find the whole phrase”

Quasi full-disk maps of solar horizontal velocities using SDO/HMI data

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F12%3A10128767" target="_blank" >RIV/00216208:11320/12:10128767 - isvavai.cz</a>

  • Alternative codes found

    RIV/67985815:_____/12:00388116

  • Result on the web

    <a href="http://dx.doi.org/10.1051/0004-6361/201118678" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201118678</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1051/0004-6361/201118678" target="_blank" >10.1051/0004-6361/201118678</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Quasi full-disk maps of solar horizontal velocities using SDO/HMI data

  • Original language description

    Aims. For the first time, the motion of granules (solar plasma on the surface on scales larger than 2.5 Mm) has been followed over the entire visible surface of the Sun, using SDO/HMI white-light data. Methods. Horizontal velocity fields are derived fromimage correlation tracking using a new version of the coherent structure tracking algorithm. The spatial and temporal resolutions of the horizontal velocity map are 2.5 Mm and 30 min, respectively. Results. From this reconstruction, using the multi-resolution analysis, one can obtain to the velocity field at different scales with its derivatives such as the horizontal divergence or the vertical component of the vorticity. The intrinsic error on the velocity is similar to 0.25 km s(-1) for a time sequence of 30 min and a mesh size of 2.5 Mm. This is acceptable compared to the granule velocities, which range between 0.3 km s(-1) and 1.8 km s(-1). A high correlation between velocities computed from Hinode and SDO/HMI has been found (85%).

  • 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

  • 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

    Astronomy and Astrophysics

  • ISSN

    0004-6361

  • e-ISSN

  • Volume of the periodical

    540

  • Issue of the periodical within the volume

    duben

  • Country of publishing house

    DE - GERMANY

  • Number of pages

    8

  • Pages from-to

  • UT code for WoS article

    000303315400102

  • EID of the result in the Scopus database