Self-consistent simulation of photoelectrons in exoplanet winds: Faster ionisation and weaker mass-loss rates

Open Access

Fig. 9

Ionisation yields for the case M0.05. Top panel: number of total (primary plus secondary) ions created per primary photoelectron as a function of wavelength and altitude for the M0.05 planet. The grey regions indicate where . Bottom panel: total (primary plus secondary) ions created per primary photoelectron averaged over wavelength and as a function of altitude.

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.