Haisheng Ji

TL;DR: An overview of solar flares and associated phenomena, drawing upon a wide range of observational data primarily from the RHESSI era, is presented in this paper, where the focus is on different areas of flare phenomena (footpoints and ribbons, coronal sources, relationship to coronal mass ejections) and their interconnections.

TL;DR: An overview of solar flares and associated phenomena, drawing upon a wide range of observational data primarily from the RHESSI era, is presented in this article, with the emphasis on the observations from multiple points of view, while bearing in mind the models that link them to each other and to theory.

TL;DR: In this article, the fine temporal and spatial structure of a filament eruption on 2002 May 27 following an M2-class flare was observed at the Big Bear Solar Observatory, with a cadence of 40 ms. The event appears to be a failed eruption, as the filament material, seen in absorption by TRACE, first accelerated then decelerated as it approached its peak height of similar to 8 x 10(4) km while the filament threads drained back to the Sun.

TL;DR: In this paper, the authors studied six X-class flares and found significant changes in the photospheric magnetic fields associated with all of the events, and the observed changes are permanent.

TL;DR: In this article, the authors presented the results from a high-cadence Ha blue-wing observation of an M1.1-class solar flare, which occurred in NOAA AR 10687 on 2004 November 1.