Podrobno

Theoretical relations between model parameters and Metis observables for eruptive prominences and coronal mass ejections
ID Jejčič, Sonja (Avtor), ID Schwartz, Pavol (Avtor), ID Heinzel, Petr (Avtor), ID Gunár, Stanislav (Avtor)

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Izvleček
Context. We investigate the behavior of the plasma in eruptive prominences and coronal mass ejections in characteristic physical conditions. Aims. We aim to demonstrate various relations between the plasma parameters and radiation properties relevant to Solar Orbiter and Metis observations. Methods. Our method is based on 2D non-local thermodynamic equilibrium (non-LTE) modeling of moving structures that are externally illuminated from the solar disk. We have focused on temperatures below 105 K and a range of gas pressures to investigate the opacity effects in the Lα line. Overall, we applied a large grid of isothermal and isobaric models. Results. Our results are presented in the form of various correlation plots showing relationships between the plasma parameters and radiation properties relevant to Metis observations. We also demonstrate the relative importance of radiative and collisional ionization of hydrogen and the ratio between radiative and collisional excitation of the Lα line. Our results point to the need to carry out optically thick non-LTE modeling for specific plasma conditions. The visible light (VL) emission was also obtained for the purposes of a comparison with the Metis data.

Jezik:Angleški jezik
Ključne besede:solar atmosphere, solar prominences, solar filaments, coronal mass ejections
Vrsta gradiva:Članek v reviji
Tipologija:1.01 - Izvirni znanstveni članek
Organizacija:FMF - Fakulteta za matematiko in fiziko
Status publikacije:Objavljeno
Različica publikacije:Objavljena publikacija
Datum objave:01.04.2025
Leto izida:2025
Št. strani:9 str.
Številčenje:Vol. 696, art. no. ǂA14
PID:20.500.12556/RUL-169926 Povezava se odpre v novem oknu
UDK:523.9
ISSN pri članku:1432-0746
DOI:10.1051/0004-6361/202453116 Povezava se odpre v novem oknu
COBISS.SI-ID:239668483 Povezava se odpre v novem oknu
Datum objave v RUL:17.06.2025
Število ogledov:275
Število prenosov:55
Metapodatki:XML DC-XML DC-RDF
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Gradivo je del revije

Naslov:Astronomy & astrophysics
Skrajšan naslov:Astron. astrophys.
Založnik:EDP Sciences
ISSN:1432-0746
COBISS.SI-ID:392577 Povezava se odpre v novem oknu

Licence

Licenca:CC BY 4.0, Creative Commons Priznanje avtorstva 4.0 Mednarodna
Povezava:http://creativecommons.org/licenses/by/4.0/deed.sl
Opis:To je standardna licenca Creative Commons, ki daje uporabnikom največ možnosti za nadaljnjo uporabo dela, pri čemer morajo navesti avtorja.

Sekundarni jezik

Jezik:Slovenski jezik
Ključne besede:Sončeva atmosfera, Sončeva protuberance, Sončevi filamenti, koronarni izbruhi snovi

Projekti

Financer:ARIS - Javna agencija za znanstvenoraziskovalno in inovacijsko dejavnost Republike Slovenije
Številka projekta:P1-0188-2022
Naslov:Astrofizika in fizika atmosfere

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