Energy spectra of energetic neutral hydrogen backscattered and sputtered from the lunar regolith by the solar wind

Open Access

Fig. 5

Fitted models of energetic neutral hydrogen flux, with components separated for solar wind speeds <400 km s⁻¹ (top) and >400 km s⁻¹ (bottom). The solid vertical line indicates the median solar wind proton energy within the data set. The other lines have the same meaning as in Fig. 4b.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.