Počet záznamů: 1  

Heating of the solar photosphere during a white-light flare

  1. 1.
    SYSNO ASEP0499738
    Druh ASEPJ - Článek v odborném periodiku
    Zařazení RIVJ - Článek v odborném periodiku
    Poddruh JČlánek ve WOS
    NázevHeating of the solar photosphere during a white-light flare
    Tvůrce(i) Jurčák, Jan (ASU-R) RID, ORCID
    Kašparová, Jana (ASU-R) RID, ORCID
    Švanda, Michal (ASU-R) RID, ORCID
    Kleint, L. (CH)
    Číslo článkuA183
    Zdroj.dok.Astronomy & Astrophysics. - : EDP Sciences - ISSN 0004-6361
    Roč. 620, December (2018)
    Poč.str.9 s.
    Forma vydáníOnline - E
    Jazyk dok.eng - angličtina
    Země vyd.FR - Francie
    Klíč. slovaSun ; photosphere ; flares
    Vědní obor RIVBN - Astronomie a nebeská mechanika, astrofyzika
    Obor OECDAstronomy (including astrophysics,space science)
    CEPGA18-06319S GA ČR - Grantová agentura ČR
    GA16-18495S GA ČR - Grantová agentura ČR
    Institucionální podporaASU-R - RVO:67985815
    UT WOS000453301200014
    EID SCOPUS85058854870
    DOI10.1051/0004-6361/201833946
    AnotaceWe analyse the temperature stratification in the solar photosphere during a white-light flare and compare it with the post-white-light flare state. We used two scans of the Hinode/SOT spectropolarimeter to infer, by means of the LTE inversion code Stokes Inversion based on Response function (SIR), the physical properties in the solar photosphere during and after a white-light flare. The resulting model atmospheres are compared and the changes are related to the white-light flare. We show that the analysed white-light flare continuum brightening is probably not caused by the temperature increase at the formation height of the photospheric continuum. However, the photosphere is heated by the flare approximately down to log tau = -0.5 and this results in emission profiles of the observed Fe I lines. From the comparison with the post-white-light flare state of the atmosphere, we estimate that the major contribution to the increase in the continuum intensity originates in the heated chromosphere.
    PracovištěAstronomický ústav
    KontaktRadka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
    Rok sběru2019
Počet záznamů: 1  

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