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Numerical RHD simulations of flaring chromosphere with Flarix
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SYSNO ASEP 0470182 Document Type C - Proceedings Paper (int. conf.) R&D Document Type Conference Paper Title Numerical RHD simulations of flaring chromosphere with Flarix Author(s) Heinzel, Petr (ASU-R) RID, ORCID
Kašparová, Jana (ASU-R) RID, ORCID
Varady, Michal (ASU-R) RID, ORCID
Karlický, Marian (ASU-R) RID, ORCID
Moravec, Z. (CZ)Source Title Solar and Stellar Flares and their Effects on Planets. - Cambridge : Cambridge University Press, 2016 - ISBN 9781107137578 Pages s. 233-238 Number of pages 6 s. Publication form Print - P Action Symposium of the International Astronomical Union /320./ Event date 11.08.2015 - 14.08.2015 VEvent location Honolulu Country US - United States Event type WRD Language eng - English Country GB - United Kingdom Keywords Sun ; flares ; hydrodynamics Subject RIV BN - Astronomy, Celestial Mechanics, Astrophysics OECD category Astronomy (including astrophysics,space science) R&D Projects GAP209/12/0103 GA ČR - Czech Science Foundation (CSF) Institutional support ASU-R - RVO:67985815 UT WOS 000452774600039 EID SCOPUS 85054282773 DOI 10.1017/S1743921316000363 Annotation Flarix is a radiation–hydrodynamical (RHD) code for modeling of the response of the chromosphere to a beam bombardment during solar flares. It solves the set of hydrodynamic conservation equations coupled with NLTE equations of radiative transfer. The simulations are driven by high energy electron beams. We present results of the Flarix simulations of a flaring loop relevant to the problem of continuum radiation during flares. In particular we focus on properties of the hydrogen Balmer continuum which was recently detected by IRIS.
Workplace Astronomical Institute Contact Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326 Year of Publishing 2017
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