Solar wind charge exchange in cometary atmospheres - III. Results from the Rosetta mission to comet 67P/Churyumov-Gerasimenko (Corrigendum)

Cyril Simon Wedlund; Etienne Behar; Hans Nilsson; Markku Alho; Esa Kallio; Herbert Gunell; Dennis Bodewits; Kevin Heritier; Marina Galand; Arnaud Beth; Martin Rubin; Kathrin Altwegg; Martin Volwerk; Guillaume Gronoff; Ronnie Hoekstra

doi:10.1051/0004-6361/201834881e

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Volume 640 (August 2020)

A&A, 640 (2020) C3

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Rosetta mission full comet phase results

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Erratum

This article is an erratum for:
[https://doi.org/10.1051/0004-6361/201834881]

Fig. 10

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Solarwind ion and ENA fluxes during the Rosetta mission 2014–2016. The fluxes are measured when available by RPC-ICA, and when unavailable, are predicted by the analytical model using ROSINA-COPS and RPC-ICA data. All fluxes are averaged over 24 h. (A) Helium species. (B) Hydrogen species. ENA fluxes are drawn in blue for clarity. The solar wind ion cavity is indicated as a gray-shaded region. Safe mode and excursions where ROSINA data were excluded from the analysis are indicated.

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