Simulations of HXR Foot-point Source Sizes for Modified Thick-target Models
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F13%3A00398911" target="_blank" >RIV/67985815:_____/13:00398911 - 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
Simulations of HXR Foot-point Source Sizes for Modified Thick-target Models
Original language description
We study vertical sizes of foot-point hard X-ray (HXR) sources using a relativistic test particle approach in a flare loop with a converging magnetic field. We compare results for the Collisional Thick Target Model (CTTM) with recently proposed modifications of the CTTM comprising a secondary acceleration of beam electrons. Our preliminary results indicate that none of the proposed modifications of the CTTM can explain the observed sizes of the HXR sources in a single loop flare scenario.
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
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
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
6
Pages from-to
535-540
UT code for WoS article
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EID of the result in the Scopus database
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