First Detection of Solar Flare Emission in Mid-ultraviolet Balmer Continuum
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F18%3A00497530" target="_blank" >RIV/67985815:_____/18:00497530 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.3847/2041-8213/aaeace" target="_blank" >http://dx.doi.org/10.3847/2041-8213/aaeace</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.3847/2041-8213/aaeace" target="_blank" >10.3847/2041-8213/aaeace</a>
Alternative languages
Result language
angličtina
Original language name
First Detection of Solar Flare Emission in Mid-ultraviolet Balmer Continuum
Original language description
We present the first detection of solar flare emission at mid-ultraviolet wavelengths around 2000 angstrom by the channel 2 of the Large-Yield RAdiometer (LYRA) on board the PRoject for OnBoard Autonomy 2 mission. The flare (SOL20170906) was also observed in the channel 1 of LYRA centered at the H I Ly alpha line at 1216 angstrom, showing a clear non-thermal profile in both channels. The flare radiation in channel 2 is consistent with the hydrogen Balmer continuum emission produced by an optically thin chromospheric slab heated up to 10,000 K. Simultaneous observations in channels 1 and 2 allow the separation of the line emission (primarily from the Lya line) from the Balmer continuum emission. Together with the recent detection of the Balmer continuum emission in the near-ultraviolet by the Interface Region Imaging Spectrometer, the LYRA observations strengthen the interpretation of broadband flare emission as the hydrogen recombination continua originating in the chromosphere.
Czech name
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Czech description
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Classification
Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
<a href="/en/project/GA16-18495S" target="_blank" >GA16-18495S: Advanced solar science with IRIS</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)
Others
Publication year
2018
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Astrophysical Journal Letters
ISSN
2041-8213
e-ISSN
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Volume of the periodical
867
Issue of the periodical within the volume
2
Country of publishing house
US - UNITED STATES
Number of pages
5
Pages from-to
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UT code for WoS article
000449400000003
EID of the result in the Scopus database
2-s2.0-85056727649