Ionisation Equilibrium for the Non-Maxwellian Electron -Distributions in Solar Flares: Updated Calculations

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F15%3A00456020" target="_blank" >RIV/67985815:_____/15:00456020 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1007/s11207-015-0734-8" target="_blank" >http://dx.doi.org/10.1007/s11207-015-0734-8</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1007/s11207-015-0734-8" target="_blank" >10.1007/s11207-015-0734-8</a>

Result language
angličtina
Original language name
Ionisation Equilibrium for the Non-Maxwellian Electron -Distributions in Solar Flares: Updated Calculations
Original language description
We use the latest available atomic data to calculate the ionisation and recombination rates for the non-Maxwellian -distributions, which were shown previously to provide a good fit to the enhanced intensities of dielectronic satellite lines during solar flares. The ionisation and recombination coefficients are subsequently used to derive the ionisation equilibrium. To do so, we consider odd values of ranging from 1 to 19, i.e., from Maxwellian to strongly non-Maxwellian cases.
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
<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
2015
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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