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Analysis of Small-scale Magnetic Flux Ropes Covering the Whole Ulysses Mission

• Authors: Yu Chen, Qiang Hu, and Jakobus A. le Roux

2019 The Astrophysical Journal 881 58.

• Provider: AAS Journals

Caption: Figure 3.

Distribution of average solar wind speed for all small-scale flux ropes in Category I. The bin size is 10 km s−1. The blue dots denote flux ropes detected at higher latitudes, whereas the dark orange dots are those at lower latitudes. The entire event set is marked by the golden dots. Various statistical quantities are also denoted.