“…Rather, we present complementary aspects of the data, emphasizing the composition and energy range of the energetic particles. We argue, based in part on the conclusion that it was unlikely that there was a well-positioned shock associated with this event, (see Rouillard et al (2019), this issue), that the event may be a good candidate for being produced by current-driven processes [as also suggested for downward accelerated electrons by Cairns et al (2003), andHaerendel (2017)], possibly associated with the reconnection that must take place during and after the release of a CME, or simply driven by the relaxation of the region to a less stressed configuration of the corona after the release of the stressed fields and large mass carried away by the CME [e.g., Chen (2011)]. In Figure 1 we present an overview of the event, with measurements by the aforementioned instruments both for context, and to provide clues to the energetic particle acceleration process.…”