G. M. Simnett

TL;DR: The heliosphere instrument for spectrum, composition, and anisotropy (HISCALE) recorded the fluxes of low-energy ions and electrons when Ulysses crossed the southern solar polar region and revealed that the large-scale structure of the heliospace to at least approximately -75 degrees was significantly influenced by the near-equatorial heliospheric current sheet.

TL;DR: In this article, a review of theoretical models on origin, injection, and acceleration of CIR particles reported by Scholer, Mann et al. is presented, along with a more complete observational picture.

TL;DR: In this article, the authors analyzed the development of a coronal mass ejection on 9 July 1996 by comparing the observations of the LASCO/SOHO coronagraphs with those of the Nancay radioheliograph.

TL;DR: In this article, the authors discuss in detail the energetic particles seen at the two spacecraft during 7 and 11 May, with the objective of understanding the origin of the intense electron event seen on 10 May and the manner in which particles escaping from the shock populate the inner heliosphere.

TL;DR: The corotating particle events give us a unique opportunity to probe the three-dimensional structures of the heliosphere This is especially true if we have observations over a period of extreme stability of the CIRs, such as existed over the recent solar minimum as discussed by the authors.