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. 2016 Sep 7;13(1):3. doi: 10.1007/s41116-016-0002-5

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© The Author(s) 2016

Open AccessThis article is distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution, and reproduction in any medium, provided you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made.

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Fig. 14 — a Average heavy ion abundances at $\sim 0.32$ – $0.45 MeV / nucleon$ in 64 large SEP events events relative to those measured in the fast and slow solar wind, normalized to oxygen and plotted versus M/Q (adapted from Desai et al. 2006a). b Average abundances measured in the slow solar wind divided by those measured in 40 large CME-related SEP events above $\sim 5 MeV / nucleon$ , plotted versus the FIP of each element (adapted from Mewaldt et al. 2002)