After we move to storing means/ dispersions in the CCSLCs, we need to convert them into single rasters for the current PS input format. The mean will use something like
To minimize changes to the SAS, we can run a function on each CCSLC burst stack and produce one amplitude_mean.tif and one amplitude_dispersion.tif per burst.
After we move to storing means/ dispersions in the CCSLCs, we need to convert them into single rasters for the current PS input format. The mean will use something like
$$ \mu{total} = (\sum{i=1}^k \mu_i Ni) / (\sum{i=1}^k N_i) $$
with similar idea for $\sigma^2_{total}$.
To minimize changes to the SAS, we can run a function on each CCSLC burst stack and produce one
amplitude_mean.tifand oneamplitude_dispersion.tifper burst.