Free Access

Fig. 6

image

Distribution of geocentric radiants of modeled particles, which approach the Earth’s orbit within 0.05 au at the present in the ecliptical coordinate frame with the modified ecliptic longitude to place the Earth’s apex into the coordinate origin. This distribution was derived from the model for tev = 500 Po and the strength of the P-R drag characterized with value of parameter β = 0. The radiant positions are shown in the Hammer projection of celestial sphere. The mean radiants of filaments F1 and F4 as well as F2 and F3 are connected (light blue dashed lines) to show the symmetry of the radiant areas.

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.