2D non-LTE modelling of a filament observed in the H alpha line with the DST/IBIS spectropolarimeter
Identifikátory výsledku
Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F19%3A00520568" target="_blank" >RIV/67985815:_____/19:00520568 - isvavai.cz</a>
Výsledek na webu
<a href="https://doi.org/10.1051/0004-6361/201935358" target="_blank" >https://doi.org/10.1051/0004-6361/201935358</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/201935358" target="_blank" >10.1051/0004-6361/201935358</a>
Alternativní jazyky
Jazyk výsledku
angličtina
Název v původním jazyce
2D non-LTE modelling of a filament observed in the H alpha line with the DST/IBIS spectropolarimeter
Popis výsledku v původním jazyce
We analyse the spectral observations obtained in the H alpha line to derive the thermodynamic properties of the plasma of the observed fragment of the filament. Methods. We used a 2D filament model employing radiative transfer computations under conditions that depart from the local thermodynamic equilibrium. We employed a forward modelling technique in which we used the 2D model to produce synthetic H alpha line profiles that we compared with the observations. We then found the set of model input parameters, which produces synthetic spectra with the best agreement with observations. Our analysis shows that one part of the observed fragment of the filament is cooler, denser, and more dynamic than its other part that is hotter, less dense, and more quiescent. The derived temperatures in the first part range from 6000 K to 10 000 K and in the latter part from 11 000 K to 14 000 K. The gas pressure is 0.2-0.4 dyn cm(-2) in the first part and around 0.15 dyn cm(-2) in the latter part. The more dynamic nature of the first part is characterised by the line-of-sight velocities with absolute values of 6-7 km s(-1) and microturbulent velocities of 8-9 km s(-1). On the other hand, the latter part exhibits line-of-sight velocities with absolute values 0-2.5 km s(-1) and microturbulent velocities of 4-6 km s(-1).
Název v anglickém jazyce
2D non-LTE modelling of a filament observed in the H alpha line with the DST/IBIS spectropolarimeter
Popis výsledku anglicky
We analyse the spectral observations obtained in the H alpha line to derive the thermodynamic properties of the plasma of the observed fragment of the filament. Methods. We used a 2D filament model employing radiative transfer computations under conditions that depart from the local thermodynamic equilibrium. We employed a forward modelling technique in which we used the 2D model to produce synthetic H alpha line profiles that we compared with the observations. We then found the set of model input parameters, which produces synthetic spectra with the best agreement with observations. Our analysis shows that one part of the observed fragment of the filament is cooler, denser, and more dynamic than its other part that is hotter, less dense, and more quiescent. The derived temperatures in the first part range from 6000 K to 10 000 K and in the latter part from 11 000 K to 14 000 K. The gas pressure is 0.2-0.4 dyn cm(-2) in the first part and around 0.15 dyn cm(-2) in the latter part. The more dynamic nature of the first part is characterised by the line-of-sight velocities with absolute values of 6-7 km s(-1) and microturbulent velocities of 8-9 km s(-1). On the other hand, the latter part exhibits line-of-sight velocities with absolute values 0-2.5 km s(-1) and microturbulent velocities of 4-6 km s(-1).
Klasifikace
Druh
J<sub>imp</sub> - Článek v periodiku v databázi Web of Science
CEP obor
—
OECD FORD obor
10308 - Astronomy (including astrophysics,space science)
Návaznosti výsledku
Projekt
Výsledek vznikl pri realizaci vícero projektů. Více informací v záložce Projekty.
Návaznosti
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Ostatní
Rok uplatnění
2019
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Údaje specifické pro druh výsledku
Název periodika
Astronomy & Astrophysics
ISSN
1432-0746
e-ISSN
—
Svazek periodika
631
Číslo periodika v rámci svazku
November
Stát vydavatele periodika
FR - Francouzská republika
Počet stran výsledku
12
Strana od-do
A146
Kód UT WoS článku
000499478000001
EID výsledku v databázi Scopus
2-s2.0-85076636587