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Dynamics of the solar atmosphere above a pore with a light bridge

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F13%3A10193076" target="_blank" >RIV/00216208:11320/13:10193076 - isvavai.cz</a>

  • Alternative codes found

    RIV/67985815:_____/13:00423843

  • Result on the web

    <a href="http://dx.doi.org/10.1051/0004-6361/201322148" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201322148</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1051/0004-6361/201322148" target="_blank" >10.1051/0004-6361/201322148</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Dynamics of the solar atmosphere above a pore with a light bridge

  • Original language description

    Context. Solar pores are small sunspots lacking a penumbra that have a prevailing vertical magnetic-field component. They can include light bridges at places with locally reduced magnetic field. Like sunspots, they exhibit a wide range of oscillatory phenomena. Aims. A large isolated pore with a light bridge (NOAA 11005) is studied to obtain characteristics of a chromospheric filamentary structure around the pore, to analyse oscillations and waves in and around the pore, and to understand the structureand brightness of the light bridge. Methods. Spectral imaging observations in the line Ca II 854.2 nm and complementary spectropolarimetry in Fe I lines, obtained with the DST/IBIS spectrometer and HINODE/SOT spectropolarimeter, were used to measure photospheric and chromospheric velocity fields, oscillations, waves, the magnetic field in the photosphere, and acoustic energy flux and radiative losses in the chromosphere. Results. The chromospheric filamentary structure around the pore ha

  • 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

    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

    560

  • Issue of the periodical within the volume

    prosinec

  • Country of publishing house

    FR - FRANCE

  • Number of pages

    14

  • Pages from-to

  • UT code for WoS article

    000328754500084

  • EID of the result in the Scopus database