作者:陳鵬飛,許敖敖,丁明德
摘要:Solar filaments are an intriguing phenomenon,like cool clouds suspended in the hot corona.Similar structures exist in the intergalactic medium as well.Despite being a long-studied topic,solar filaments have continually attracted intensive attention because of their link to coronal heating,coronal seismology,solar flares and coronal mass ejections(CMEs).In this review paper,by combing through the solar filament-related work done in the past decade,we discuss several controversial topics,such as the fine structures,dynamics,magnetic configurations and helicity of filaments.With high-resolution and highsensitivity observations,combined with numerical simulations,it is expected that resolving these disputes will definitely lead to a huge leap in understanding the physics related to solar filaments,and even shed light on galactic filaments.
發文機構:School of Astronomy and Space Science Key Laboratory of Modern Astronomy&Astrophysics State Key Laboratory of Lunar and Planetary Sciences
關鍵詞:MAGNETOHYDRODYNAMICSSun:prominencesSun:filaments
分類號: P182[天文地球—天文學]