Observational consequences of the local re-acceleration thick-target model

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F13%3A00399190" target="_blank" >RIV/67985815:_____/13:00399190 - isvavai.cz</a>
Alternative codes found
RIV/44555601:13440/13:43885026
Result on the web
<a href="http://dx.doi.org/10.1088/1742-6596/440/1/012013" target="_blank" >http://dx.doi.org/10.1088/1742-6596/440/1/012013</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1088/1742-6596/440/1/012013" target="_blank" >10.1088/1742-6596/440/1/012013</a>

Result language
angličtina
Original language name
Observational consequences of the local re-acceleration thick-target model
Original language description
The authors compare the e ciency of the hard X-ray production and the vertical sizes and positions of the hard X-ray sources for the classical collisional thick-target model and for its recently proposed modication, the local re-acceleration thick-targetmodel. The latter model has been proposed in order to ease some of the severe theoretical problems of the collisional thick-target model related to interpretation of the observational properties of the foot-point HXR sources in solar ares. The results are obtained using a relativistic test-particle approach for a fully ionised atmosphere with a converging magnetic eld and a single (compact) are loop.
Czech name
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Czech description
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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
2013
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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