Spicule jets in the solar atmosphere modeled with resistive MHD and thermal conduction

التفاصيل البيبلوغرافية
العنوان: Spicule jets in the solar atmosphere modeled with resistive MHD and thermal conduction
المؤلفون: González-Avilés, J. J., Guzmán, F. S., Fedun, V., Verth, G.
المصدر: The Astrophysical Journal, 897:153 (19 pp), 2020 July 14
سنة النشر: 2020
المجموعة: Astrophysics
مصطلحات موضوعية: Astrophysics - Solar and Stellar Astrophysics
الوصف: Using numerical simulations, we study the effects of magnetic resistivity and thermal conductivity in the dynamics and properties of solar jets with characteristics of Type II spicules and cool coronal jets. The dynamic evolution of the jets is governed by the resistive MHD equations with thermal conduction along the magnetic field lines on a 2.5D slice. The magnetic field configuration consists of two symmetric neighboring loops with opposite polarity, used to support reconnection and followed by the plasma jet formation. In total 10 simulations were carried out with different values of resistivity and thermal conductivity, that produce jets with different morphological and thermal properties we quantify. We find that an increase in magnetic resistivity does not produce significant effects on the morphology, velocity and temperature of the jets. However, thermal conductivity affects both temperature and morphology of the jets. In particular, thermal conductivity causes jets to reach greater heights and increases the temperature of the jet-apex. Also, heat flux maps indicate the jet-apex and corona interchange energy more efficiently than the body of the jet. These results could potentially open a new avenue for plasma diagnostics in the Sun's atmosphere.
Comment: 11 pages, 4 figures. Accepted for publication in the Astrophysical Journal
نوع الوثيقة: Working Paper
DOI: 10.3847/1538-4357/ab97b8
URL الوصول: http://arxiv.org/abs/2005.13647
رقم الأكسشن: edsarx.2005.13647
قاعدة البيانات: arXiv
الوصف
DOI:10.3847/1538-4357/ab97b8