Quantitative Evaluation of Coronal Magnetic Field Models Using Tomographic Reconstructions of Electron Density

التفاصيل البيبلوغرافية
العنوان: Quantitative Evaluation of Coronal Magnetic Field Models Using Tomographic Reconstructions of Electron Density
المؤلفون: Shaela I. Jones, T. J. Wang, C. N. Arge, C. J. Henney, V. M. Uritsky, C. Rura
المصدر: The Astrophysical Journal. 928:131
بيانات النشر: American Astronomical Society, 2022.
سنة النشر: 2022
مصطلحات موضوعية: Space and Planetary Science, Physics::Space Physics, Astrophysics::Solar and Stellar Astrophysics, Astronomy and Astrophysics
الوصف: We introduce a new quantitative approach for assessing the quality of coronal magnetic field models. The method compares the location of the magnetic neutral line at a specified height in the magnetic field model with the locations of localized density peaks in the coronal electron density, as measured using coronal rotational tomography. This approach is flexible to the presence of pseudostreamers in the coronal magnetic field, as well as folds in the streamer belt. We present an example application during mid-2010 when the white-light streamer-belt structure is complex and the emergence of a large active region on the far side of the Sun presents a challenge for modeling the coronal magnetic structure.
تدمد: 1538-4357
0004-637X
URL الوصول: https://explore.openaire.eu/search/publication?articleId=doi_________::f5a303ddb7ac13984401b2b6ea196e5e
https://doi.org/10.3847/1538-4357/ac5751
حقوق: OPEN
رقم الأكسشن: edsair.doi...........f5a303ddb7ac13984401b2b6ea196e5e
قاعدة البيانات: OpenAIRE