  Precise localisation and characterization of active regions and coronal holes
as observed by EUV imagers are crucial for a wide range of solar and
helio-physics studies. We describe a segmentation procedure, the SPOCA-suite,
that produces catalogs of Active Regions (AR) and Coronal Holes (CH) on SDO-AIA
images. The method builds upon our previous work on 'Spatial Possibilistic
Clustering Algorithm' (SPOCA) and substantially improve it in several ways. The
SPOCA-suite is applied in near real time on AIA archive and produces entries
into the AR and CH catalogs of the Heliophysics Event Knowledgebase (HEK) every
four hours. We give an illustration of the use of SPOCA for determination of
the CH filling factors. This reports is intended as a reference guide for the
users of SPoCA output.
