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Signatures of the non-Maxwellian ?-distributions in optically thin line spectra I. Theory and synthetic Fe IX?XIII spectra

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F14%3A00435318" target="_blank" >RIV/67985815:_____/14:00435318 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1051/0004-6361/201424124" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201424124</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1051/0004-6361/201424124" target="_blank" >10.1051/0004-6361/201424124</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Signatures of the non-Maxwellian ?-distributions in optically thin line spectra I. Theory and synthetic Fe IX?XIII spectra

  • Original language description

    We investigate the possibility of diagnosing the degree of departure from the Maxwellian distribution using single-ion spectra originating in astrophysical plasmas in collisional ionization equilibrium. We find that it is possible to perform density diagnostics independently of kappa, with many Fe xi, Fe xii, and Fe xiii line ratios showing strong density-sensitivity and negligible sensitivity to kappa and temperature. We also tested different averaging of the collision strengths. It is found that averaging over 0.01 interval in log(E [ Ryd ]) is sufficient to produce accurate distribution-averaged collision strengths Upsilon(T,kappa) at temperatures of the ion formation in ionization equilibrium.

  • 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/GAP209%2F12%2F1652" target="_blank" >GAP209/12/1652: Analysis of the non-thermal electron distribution in the solar corona and transition region</a><br>

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2014

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Astronomy & Astrophysics

  • ISSN

    0004-6361

  • e-ISSN

  • Volume of the periodical

    570

  • Issue of the periodical within the volume

    October

  • Country of publishing house

    FR - FRANCE

  • Number of pages

    23

  • Pages from-to

    "A124/1"-"A124/23"

  • UT code for WoS article

    000344158500074

  • EID of the result in the Scopus database