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dc.contributor.authorHeinzel, P.
dc.contributor.authorGunár, S.
dc.contributor.authorAnzer, U.
dc.identifier.citationHeinzel , P , Gunár , S & Anzer , U 2015 , ' Fast approximate radiative transfer method for visualizing the fine structure of prominences in the hydrogen Hα line ' , Astronomy & Astrophysics , vol. 579 , A16 .
dc.identifier.otherPURE: 204805887
dc.identifier.otherPURE UUID: 04bafc19-2155-4ff5-bfc9-1bfed0099392
dc.identifier.otherScopus: 84934905661
dc.identifier.otherWOS: 000358877100028
dc.descriptionP.H. acknowledges the support from grant 209/12/0906 of the Grant Agency of the Czech Republic. S.G. acknowledges support from the European Commission via the Marie Curie Actions – Intra-European Fellowships Project No. 328138. P.H. and S.G. acknowledge support from project RVO:67985815 of the Astronomical Institute of the Czech Academy of Sciences and from the MPA Garching. U.A. thanks for the support from the Astronomical Institute of the Czech Academy of Sciences.en
dc.description.abstractAims. We present a novel approximate radiative transfer method developed to visualize 3D whole-prominence models with multiple fine structures using the hydrogen Hα spectral line. Methods. This method employs a fast line-of-sight synthesis of the Hα line profiles through the whole 3D prominence volume and realistically reflects the basic properties of the Hα line formation in the cool and low-density prominence medium. The method can be applied both to prominences seen above the limb and filaments seen against the disk. Results. We provide recipes for the use of this method for visualizing the prominence or filament models that have multiple fine structures. We also perform tests of the method that demonstrate its accuracy under prominence conditions. Conclusions. We demonstrate that this fast approximate radiative transfer method provides realistic synthetic Hα intensities useful for a reliable visualization of prominences and filaments. Such synthetic high-resolution images of modeled prominences/filaments can be used for a direct comparison with high-resolution observations.
dc.relation.ispartofAstronomy & Astrophysicsen
dc.rightsReproduced with permission from Astronomy & Astrophysics, © 2015 ESOen
dc.subjectRadiative transferen
dc.subjectSun: filaments, prominencesen
dc.subjectSun: magnetic fieldsen
dc.subjectQC Physicsen
dc.titleFast approximate radiative transfer method for visualizing the fine structure of prominences in the hydrogen Hα lineen
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews. Applied Mathematicsen
dc.description.statusPeer revieweden

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