Fig. 3.

Download original image
Influence of heat conduction on quasi-discontinuous solar wind solutions. Upper panel shows heating function QH, T (black, Eq. (3)); heat conduction source term Qcon (red, Eq. (14)) for an exemplary slow solar wind solution (ϵ = 1 R⊙) is shown in the range from 1 R⊙ to 1 AU. Bottom panel shows ratio of absolute powers ϕ as a function of the heating function width ϵ for the slow (black) and fast (red) solar wind solutions.
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.