Radio, EUV, and X-Ray Observations during a Filament Rise in the 2011 June 7 Solar Flare

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F20%3A00534153" target="_blank" >RIV/67985815:_____/20:00534153 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.3847/1538-4357/ab5801" target="_blank" >https://doi.org/10.3847/1538-4357/ab5801</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.3847/1538-4357/ab5801" target="_blank" >10.3847/1538-4357/ab5801</a>

Result language
angličtina
Original language name
Radio, EUV, and X-Ray Observations during a Filament Rise in the 2011 June 7 Solar Flare
Original language description
We interpret the unusual radio continuum and transient X-ray sources, which are located outside the two parallel flare ribbons, as those generated during an interaction of the rising filament with the above-lying magnetic loops. The EUV brightening at the filament footpoint could be a signature of the magnetic reconnection inside the magnetic rope carrying the filament. Possible scenarios of the similar to 30 s period oscillations in radio, X-ray, and EUV are discussed.
Czech name
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Czech description
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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
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2020
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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