Fig. 13
Number flow of the ISD particles over a full solar cycle (2018–2040). Left panel: small particles (ad < 0.2 μm). Right panel: large particles (ad > 0.3 μm). Fluxes are given in particles day-1 m-2 assuming the detection area is always orthogonal to the ISD flow. The smooth line shows the moving average of the flux over a period of 1 yr. The number flux can reach values close to zero when the Earth and ISD velocity vectors become similar.
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.