Continuum enhancements in the ultraviolet, the visible and the infrared during the X1 flare on 2014 March 29

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F16%3A00461300" target="_blank" >RIV/67985815:_____/16:00461300 - isvavai.cz</a>
Result on the web
<a href="http://hdl.handle.net/11104/0260923" target="_blank" >http://hdl.handle.net/11104/0260923</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.3847/0004-637X/816/2/88" target="_blank" >10.3847/0004-637X/816/2/88</a>

Result language
angličtina
Original language name
Continuum enhancements in the ultraviolet, the visible and the infrared during the X1 flare on 2014 March 29
Original language description
Enhanced continuum brightness is observed in many flares ("white light flares"), yet it is still unclear which processes contribute to the emission. To understand the transport of energy needed to account for this emission, we must first identify both the emission processes and the emission source regions. Possibilities include heating in the chromosphere causing optically thin or thick emission from free-bound transitions of Hydrogen, and heating of the photosphere causing enhanced H-continuum brightness. To investigate these possibilities, we combine observations from Interface Region Imaging Spectrograph (IRIS),
Czech name
—
Czech description
—

Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
—
OECD FORD branch
10308 - Astronomy (including astrophysics,space science)

Project
<a href="/en/project/GAP209%2F12%2F1652" target="_blank" >GAP209/12/1652: Analysis of the non-thermal electron distribution in the solar corona and transition region</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2016
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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