Statistical analysis of UV spectra of a quiescent prominence observed by IRIS

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F18%3A00498319" target="_blank" >RIV/67985815:_____/18:00498319 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1051/0004-6361/201833466" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201833466</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/201833466" target="_blank" >10.1051/0004-6361/201833466</a>

Result language
angličtina
Original language name
Statistical analysis of UV spectra of a quiescent prominence observed by IRIS
Original language description
The paper analyzes the structure and dynamics of a quiescent prominence that occurred on October 22, 2013 and was observed by several instruments including the Interface Region Imaging Spectrograph (IRIS). We aim to determine the physical characteristics of the observed prominence using Mg II k and h (2796 and 2803 angstrom), C II (1334 and 1336 angstrom), and Si IV (1394 angstrom) lines observed by IRIS. In addition we study the dynamical behavior of the prominence. n
Czech name
—
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
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Publication year
2018
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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