Magnetic Flux Rope Identification and Characterization from Observationally Driven Solar Coronal Models
(2017)
Journal Article
Lowder, C., & Yeates, A. (2017). Magnetic Flux Rope Identification and Characterization from Observationally Driven Solar Coronal Models. Astrophysical Journal, 846(2), Article 106. https://doi.org/10.3847/1538-4357/aa86b1
Formed through magnetic field shearing and reconnection in the solar corona, magnetic flux ropes are structures of twisted magnetic field, threaded along an axis. Their evolution and potential eruption are of great importance for space weather. Here... Read More about Magnetic Flux Rope Identification and Characterization from Observationally Driven Solar Coronal Models.