Speaker
Matteo Di Carlo
(Istituto Nazionale di Astrofisica (INAF))
Description
The PRISMA network is composed of many camera devices distributed in different parts of Italy
detecting fireballs everyday. Each camera produces images that must be synchronized in a server
and calibrated daily and monthly. In case of multiple detections (event), another process must be
run in order to perform other kinds of analysis. The entire network must be monitored in order to
detect faulty devices. This contribution analyses the decision taken for monitoring and controlling
the PRISMA network in the server available in Turin.
Primary author
Matteo Di Carlo
(Istituto Nazionale di Astrofisica (INAF))
