Successive X-class flares and coronal mass ejections driven by shearing motion and sunspot rotation in active region NOAA 12673

XL Yan, JC Wang, GM Pan, DF Kong… - The Astrophysical …, 2018 - iopscience.iop.org
We present a clear case study on the occurrence of two successive X-class flares, including
a decade-class flare (X9. 3) and two coronal mass ejections (CMEs) triggered by shearing …

A magnetic reconnection event in the solar atmosphere driven by relaxation of a twisted arch filament system

Z Huang, C Mou, H Fu, L Deng, B Li… - The Astrophysical …, 2018 - iopscience.iop.org
We present high-resolution observations of a magnetic reconnection event in the solar
atmosphere taken with the New Vacuum Solar Telescope, Atmospheric Imaging Assembly …

The surge-like eruption of a miniature filament associated with circular flare ribbon

H Li, J Yang, Y Jiang, Y Bi, Z Qu, H Chen - Astrophysics and Space …, 2018 - Springer
We present a study of a mini-filament erupting in association with a circular ribbon flare
observed by NVST and SDO/AIA on 2014 March 17. The filament was located at one …

Occurrence and persistence of magnetic elements in the quiet Sun

F Giannattasio, F Berrilli, G Consolini… - Astronomy & …, 2018 - aanda.org
Context. Turbulent convection efficiently transports energy up to the solar photosphere, but
its multi-scale nature and dynamic properties are still not fully understood. Several works in …

Automated detection methods for solar activities and an application for statistic analysis of solar filament

Q Hao, PF Chen, C Fang - Proceedings of the International …, 2018 - cambridge.org
With the rapid development of telescopes, both temporal cadence and the spatial resolution
of observations are increasing. This in turn generates vast amount of data, which can be …