LIGHT POLLUTION

Every Light Has Its Shadow

GROUND BASED NETWORK

PRISMA

First Italian Network for the Systematic Surveillance of Meteors and the Atmosphere (PRISMA) involves the creation of an Italian network of all-sky cameras for observing bright meteors (fireballs and bolides), with the aim of determining the orbits of the objects that cause them and accurately defining the areas where fragments may fall, in order to recover the meteorites.

TYPE OF INSTRUMENT
All-sky cameras
N° OF STATIONS
42 in CE, > 80 in Italy
LOCATION
Italy
COORDINATES
See the map
MEASUREMENT POINT
Diverse
STATUS
Operational
DATA AVAILABILITY
Soon to be published
TIME RANGE
Since 2018
FREQUENCY OF MEASUREMENT
Each 10 minutes
DATA PUBLISHING FREQUENCY
n/a
DATA PUBLISHING DELAY
n/a
OWNER
INAF (Istituto Nazionale
di Astrofisica)

MORE INFORMATION

CALIBRATED DATA
Yes
MEASUREMENT UNIT
mag/arcsec²
WAVELENGTH RANGE
300 – 1000 nm
FIELD-OF-VIEW
All-sky
POINTING DIRECTION
Zenith
DATA VISUALISATION
No
DATA DOWNLOAD
No
DATA FORMAT
n/a
DATA POLICY
n/a

FURTHER REFERENCES

– News From the Italian PRISMA Fareball Network (read the article)
– Improving Astrometry and Photometry Reduction for PRISMA All-Sky Cameras (read the article)

This repository is managed by INAF as part of the Interreg Central Europe project DARKERSKY4CE, co-funded by the European Union. The views and opinions expressed herein are those of the authors and do not necessarily reflect those of the European Commission. Whilst INAF takes every precaution to ensure that the content is accurate, INAF cannot guarantee that all information or data on the website is correct. Therefore, INAF accepts no responsibility or liability whatsoever with regard to the information or data on the website or for any use which may be made of it.