Academic Journal

Propagation of Type II spicules into the solar corona III. MHD simulation

التفاصيل البيبلوغرافية
العنوان: Propagation of Type II spicules into the solar corona III. MHD simulation
المؤلفون: Díaz-Figueroa, E. E., González-Avilés, J. J., de Parga, G. Ares
المصدر: Journal of Physics: Conference Series ; volume 2307, issue 1, page 012065 ; ISSN 1742-6588 1742-6596
بيانات النشر: IOP Publishing
سنة النشر: 2022
الوصف: We study the possible influence of a magnetic narrow region on the propagation of jets with some characteristics of Type II spicules into the solar corona using MHD approximation numerical simulations. We found that an increase of temperature occurs mainly at the top of the jet, which supports the idea of sectioning the spicule in the TM approximation of the previous works. Also, we show that the magnetic bottle does not directly affect the propagation of the jet; since the physical conditions of the ideal MHD equations imply that the magnetic field lines are frozen-in with the plasma.
نوع الوثيقة: article in journal/newspaper
اللغة: unknown
DOI: 10.1088/1742-6596/2307/1/012065
DOI: 10.1088/1742-6596/2307/1/012065/pdf
الاتاحة: http://dx.doi.org/10.1088/1742-6596/2307/1/012065
https://iopscience.iop.org/article/10.1088/1742-6596/2307/1/012065
https://iopscience.iop.org/article/10.1088/1742-6596/2307/1/012065/pdf
Rights: http://creativecommons.org/licenses/by/3.0/ ; https://iopscience.iop.org/info/page/text-and-data-mining
رقم الانضمام: edsbas.41B9183D
قاعدة البيانات: BASE
الوصف
DOI:10.1088/1742-6596/2307/1/012065