Modelling of Flare Processes: A Comparison of the Two RHD Codes FLARIX and RADYN

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F19%3A00520216" target="_blank" >RIV/67985815:_____/19:00520216 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Result language
angličtina
Original language name
Modelling of Flare Processes: A Comparison of the Two RHD Codes FLARIX and RADYN
Original language description
We present a comparison of two autonomous, methodologically different radiation hydrodynamic codes, FLARIX and RADYN, and their use to model the solar flare processes. Both codes can model the time evolution of a 1D atmosphere heated by a specified process, e.g. by electron beams propagating from the injection site in the corona down to the lower atmosphere. In such a scenario time scales can be rather short and lead to fast heating on even sub-second time scales.n
Czech name
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Czech description
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Project
<a href="/en/project/GA16-18495S" target="_blank" >GA16-18495S: Advanced solar science with IRIS</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2019
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Article name in the collection
Radiative Signatures from the Cosmos: A Conference in Honor of Ivan Hubený
ISBN
9781583819265
ISSN
1050-3390
e-ISSN
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Number of pages
6
Pages from-to
141-146
Publisher name
Astronomical Society of the Pacific
Place of publication
San Francisco
Event location
Paris
Event date
Oct 23, 2018
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
000494866300022

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