On the Possibility to Diagnose the Non-Maxwellian kappa-Distributions from the Hinode/EIS EUV Spectra

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F13%3A00399488" target="_blank" >RIV/67985815:_____/13:00399488 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1007/s11207-012-0136-0" target="_blank" >http://dx.doi.org/10.1007/s11207-012-0136-0</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1007/s11207-012-0136-0" target="_blank" >10.1007/s11207-012-0136-0</a>

Result language
angličtina
Original language name
On the Possibility to Diagnose the Non-Maxwellian kappa-Distributions from the Hinode/EIS EUV Spectra
Original language description
Density diagnostics using lines of the non-Fe elements is discussed and the influence of kappa on the diagnostics of electron density is presented. The density diagnostics using these non-Fe EIS lines are strongly affected by both known and unknown blends. Therefore, we performed the density diagnostics using the Fe xii -aEuro parts per thousand xiv lines. Subsequently, these proposed diagnostic methods for kappa-distributions are tested using the spectral atlas obtained by Brown et al. (Astrophys. J. Suppl. 176, 511, 2008). These data do not provide conclusive evidence for the presence of kappa-distributions due to possible plasma multitermality, a low observed signal-to-noise ratio, and unremovable or unknown blends.
Czech name
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Czech description
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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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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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