Fig. 2
Qabs (solid lines) and Qsca (dashed lines) for CMM grains with cores of amorphous carbon (left) and cores of amorphous silicate of olivine type (middle) and pyroxene type (right) for different grain radii in μm. The inner mantle is aromatic-rich and the outer mantle aliphatic-rich amorphous carbon. At long wavelengths Qabs and Qsca increase with increasing grain size.
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.