ism3d.arts.utils.clouds_split

ism3d.arts.utils.clouds_split(obj, w)

Divivd the cloudlet model by channel in advance to avoid doing it during channel looping

Note:

returned v has a flip sign from V_los vrange[0] first channel velocity and vrange[1] last channel velocity

The returned list should have a element number of N(objs)

for ccloudlet model: fluxscale is the flux per cloud for continuum model: fluxscale is the flux of the object within a plane