Figure 4 from Heliosphere Responds to a Large Solar Wind Intensification: Decisive Observations from IBEX

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Heliosphere Responds to a Large Solar Wind Intensification: Decisive Observations from IBEX

Authors: D. J. McComas, M. A. Dayeh, H. O. Funsten, J. Heerikhuisen, P. H. Janzen, D. B. Reisenfeld, N. A. Schwadron, J. R. Szalay, and E. J. Zirnstein

2018 The Astrophysical Journal Letters 856 L10.

Provider: AAS Journals

Caption: Figure 4.

Comparison of ENA fluxes from early 2016 to early 2017 from CG corrected ram data. The IBEX Ribbon is visible in the lowest energies, 0.7 and 1.1 keV. At higher energies, the ENAs are progressively enhanced with increasing energy from the 1.7 to 2.7 to 4.3 keV energy bands, consistent with the greater generation and faster return of higher energy ENAs calculated by the numerical model (Figure 1).

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