Density diagnostics derived from the O iv and S iv intercombination lines observed by IRIS

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F16%3A00470337" target="_blank" >RIV/67985815:_____/16:00470337 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1051/0004-6361/201628965" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201628965</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/201628965" target="_blank" >10.1051/0004-6361/201628965</a>

Result language
angličtina
Original language name
Density diagnostics derived from the O iv and S iv intercombination lines observed by IRIS
Original language description
In this work we have investigated the use of the O IV and S IV emission lines observed by IRIS as electronndensity diagnostics in the plasma from which they are emitted. These ions are formed at similar temperatures and therefore arenexpected to provide similar density diagnostics (within a factor of around two).n
Czech name
—
Czech description
—

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
<a href="/en/project/GAP209%2F12%2F1652" target="_blank" >GAP209/12/1652: Analysis of the non-thermal electron distribution in the solar corona and transition region</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2016
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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