Academic Journal

Validation of a Wave Heated 3D MHD Coronal-wind Model using Polarized Brightness and EUV Observations

التفاصيل البيبلوغرافية
العنوان: Validation of a Wave Heated 3D MHD Coronal-wind Model using Polarized Brightness and EUV Observations
المؤلفون: Parenti, Susanna, Réville, Victor, Brun, Allan Sacha, Pinto, Rui F., Auchère, Frédéric, Buchlin, Eric, Perri, Barbara, Strugarek, Antoine
المساهمون: Astrophysique Interprétation Modélisation (AIM (UMR_7158 / UMR_E_9005 / UM_112)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Institut d'astrophysique spatiale (IAS), Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales Paris (CNES), Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Centre National de la Recherche Scientifique (CNRS)
المصدر: ISSN: 0004-637X.
بيانات النشر: HAL CCSD
American Astronomical Society
سنة النشر: 2022
المجموعة: Université Toulouse III - Paul Sabatier: HAL-UPS
مصطلحات موضوعية: Magnetohydrodynamical simulations, Solar physics, Solar coronal heating, Solar coronal streamers, Solar corona, Solar extreme ultraviolet emission, Solar radiation, Solar atmosphere, [SDU]Sciences of the Universe [physics], [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]
الوصف: International audience ; The physical properties responsible for the formation and evolution of the corona and heliosphere are still not completely understood. 3D MHD global modeling is a powerful tool to investigate all the possible candidate processes. To fully understand the role of each of them, we need a validation process where the output from the simulations is quantitatively compared to the observational data. In this work, we present the results from our validation process applied to the wave turbulence driven 3D MHD corona-wind model WindPredict-AW. At this stage of the model development, we focus the work to the coronal regime in quiescent condition. We analyze three simulation results, which differ by the boundary values. We use the 3D distributions of density and temperature, output from the simulations at the time of around the first Parker Solar Probe perihelion (during minimum of the solar activity), to synthesize both extreme ultraviolet (EUV) and white-light-polarized (WL pB) images to reproduce the observed solar corona. For these tests, we selected AIA 193 Å, 211 Å, and 171 Å EUV emissions, MLSO K-Cor, and LASCO C2 pB images obtained on 2018 November 6 and 7. We then make quantitative comparisons of the disk and off limb corona. We show that our model is able to produce synthetic images comparable to those of the observed corona.
نوع الوثيقة: article in journal/newspaper
اللغة: English
Relation: info:eu-repo/semantics/altIdentifier/arxiv/2203.10876; ARXIV: 2203.10876; BIBCODE: 2022ApJ.929.75P
DOI: 10.3847/1538-4357/ac56da
الاتاحة: https://insu.hal.science/insu-03672026
https://insu.hal.science/insu-03672026v1/document
https://insu.hal.science/insu-03672026v1/file/Parenti_2022_ApJ_929_75.pdf
https://doi.org/10.3847/1538-4357/ac56da
Rights: http://creativecommons.org/licenses/by/ ; info:eu-repo/semantics/OpenAccess
رقم الانضمام: edsbas.DFD88597
قاعدة البيانات: BASE
الوصف
DOI:10.3847/1538-4357/ac56da