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Understanding the HMI Pseudocontinuum in White-light Solar Flares

  1. 1.
    SYSNO ASEP0495487
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleUnderstanding the HMI Pseudocontinuum in White-light Solar Flares
    Author(s) Švanda, Michal (ASU-R) RID, ORCID
    Jurčák, Jan (ASU-R) RID, ORCID
    Kašparová, Jana (ASU-R) RID, ORCID
    Kleint, L. (CH)
    Article number144
    Source TitleAstrophysical Journal - ISSN 0004-637X
    Roč. 860, č. 2 (2018)
    Number of pages9 s.
    Publication formOnline - E
    Languageeng - English
    CountryUS - United States
    KeywordsSun ; activity ; flares
    Subject RIVBN - Astronomy, Celestial Mechanics, Astrophysics
    OECD categoryAstronomy (including astrophysics,space science)
    R&D ProjectsGA16-18495S GA ČR - Czech Science Foundation (CSF)
    GA18-06319S GA ČR - Czech Science Foundation (CSF)
    Institutional supportASU-R - RVO:67985815
    UT WOS000436072400006
    EID SCOPUS85049225362
    DOI10.3847/1538-4357/aac3e4
    AnnotationWe analyze observations of the X9.3 solar flare (SOL2017-09-06T11:53) observed by SDO/HMI and Hinode/Solar Optical Telescope. Our aim is to learn about the nature of the HMI pseudocontinuum I-c used as a proxy for the white-light continuum. From model atmospheres retrieved by an inversion code applied to the Stokes profiles observed by the Hinode satellite, we synthesize profiles of the FeI 617.3 nm line and compare them to HMI observations. Based on a pixel-by-pixel comparison, we show that the value of I-c represents the continuum level well in quiet-Sun regions only. In magnetized regions, it suffers from a simplistic algorithm that is applied to a complex line shape. During this flare, both instruments also registered emission profiles in the flare ribbons. Such emission profiles are poorly represented by the six spectral points of HMI and the MDI-like algorithm does not account for emission profiles in general, thus, the derived pseudocontinuum intensity does not approximate the continuum value properly.
    WorkplaceAstronomical Institute
    ContactRadka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
    Year of Publishing2019
Number of the records: 1  

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