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The Hanle and Zeeman Polarization Signals of the Solar Ca II 8542 angstromLine

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F16%3A00463132" target="_blank" >RIV/67985815:_____/16:00463132 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.3847/2041-8205/826/1/L10" target="_blank" >http://dx.doi.org/10.3847/2041-8205/826/1/L10</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.3847/2041-8205/826/1/L10" target="_blank" >10.3847/2041-8205/826/1/L10</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    The Hanle and Zeeman Polarization Signals of the Solar Ca II 8542 angstromLine

  • Original language description

    We highlight the main results of a three-dimensional (3D) multilevel radiative transfer investigation about the solar disk-center polarization of the Ca-II 8542 angstrom line. First, through the use of a 3D model of the solar atmosphere, we investigate the linear polarization that occurs due to the atomic level polarization produced by the absorption and scattering of anisotropic radiation, taking into account the symmetry-breaking effects caused by its thermal, dynamic, and magnetic structure. Second, we study the contribution of the Zeeman effect to the linear and circular polarization. Finally, we show examples of the Stokes profiles produced by the joint action of the atomic level polarization and the Hanle and Zeeman effects. We find that the Zeeman effect tends to dominate the linear polarization signals only in the localized patches of opposite magnetic polarity, where the magnetic field is relatively strong and slightly inclined; outside such very localized patches, the linear polarization is often dominated by the contribution of atomic level polarization.

  • 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/GA16-16861S" target="_blank" >GA16-16861S: Multidimensional modeling of polarized spectra of the outer solar atmosphere</a><br>

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2016

  • 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

    826

  • Issue of the periodical within the volume

    1

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    6

  • Pages from-to

    "L10/1"-"L10/6"

  • UT code for WoS article

    000380739300010

  • EID of the result in the Scopus database

    2-s2.0-84979255183