Guillermo Stenborg

TL;DR: The SOHO/LASCO CME catalog as mentioned in this paper is a data base for the analysis of coronal mass ejections (CMEs) in the solar corona.

TL;DR: In this article, the authors report direct observations of the magnetic reconnection site during an eruptive process that occurred on 2003 November 18, which started with a rapid expansion of a few magnetic arcades located over the east limb of the Sun and developed an energetic partial-halo coronal mass ejection (CME), a long current sheet and a group of bright flare loops in the wake of the CME.

TL;DR: In this article, the authors studied the coronal mass ejections (CMEs) and flares associated with large solar energetic particle (SEP) events of solar cycle 23 (1996-2002) to determine what property of the solar eruptions might order the SEP intensity.

TL;DR: In this article, a detailed analysis of Extreme Ultraviolet observations of the formation of a flux rope during a confined flare followed about seven hours later by the ejection of the flux rope and an eruptive flare.

TL;DR: In this article, the authors compared the heliospheric images with in situ plasma and magnetic field measurements obtained by near-Earth spacecraft, and found a near perfect association between the occurrence of these waves and the arrival of density enhancements at the leading edges of high-speed solar wind streams.