Fragmented Reconnection and Narrowband Decimetric Spikes
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F13%3A00398910" target="_blank" >RIV/67985815:_____/13:00398910 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
Fragmented Reconnection and Narrowband Decimetric Spikes
Original language description
Using numerical simulations, the fragmented reconnection process is described. It is shown that during this reconnection process plasmoids in a broad range of spatial scales are generated and form a cascade of interacting plasmoids. These interactions then produce electromagnetic waves. It is proposed that the observed narrowband dm-spikes are radio signatures of these processes. Some properties of these cascades of plasmoids are derived. Finally, it is discussed how these processes can generate the above-the-loop-top hard X-ray sources as well as the hard X-ray emission at footpoints of flare magnetic ropes.
Czech name
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Czech description
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Classification
Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Result continuities
Project
<a href="/en/project/GAP209%2F12%2F0103" target="_blank" >GAP209/12/0103: Radio and X-ray diagnostics of primary-energy-release processes in solar flares and their numerical simulations</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2013
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Central European Astrophysical Bulletin
ISSN
1845-8319
e-ISSN
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Volume of the periodical
37
Issue of the periodical within the volume
2
Country of publishing house
HR - CROATIA
Number of pages
14
Pages from-to
521-534
UT code for WoS article
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EID of the result in the Scopus database
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