The Thermal Infrared Laboratory (TIRLab) of INGV-Osservatorio Vesuviano manages the thermal infrared permanent volcanic surveillance network (TIRNet) of the volcanic areas of Campi Flegrei and Vesuvio (Italy). TIRNet network is composed of 7 stations which acquire IR frames of volcanic sites characterized by thermal anomalies due to diffuse degassing.
Fabio Sansivero (responsible)
Giuseppe Vilardo
Solfatara1 station (SF1) acquires IR frames of diffuse degassing area in the SE sector of Solfatara crater including Bocca Grande and Bocca Nuova fumaroles.
Solfatara2 station (SF1) acquires IR frames of diffuse degassing area at the base of NW inner slope of Solfatara crater.
Pisciarelli station (PS1) acquires IR frames of the diffuse degassing area of Pisciarelli at the base of the eastern outer slope of Solfatara volcanic edifice.
Olibano station (OLIB) acquires IR frames of the diffuse degassing area on the southern slope of Monte Olibano lava dome.
SOB station (SOB) acquires IR frames of the diffuse degassing area on the eastern rim of Solfatara volcanic edifice.
Antiniana station (ANTN) acquires IR frames of the diffuse degassing area of Agnano - via Antiniana, at East of Solfatara volcanic edifice.
Vesuvio station (VES) acquires IR frames of the diffuse degassing area of inner western rim of Vesuvio crater.
Acquisition technology of TIRNet surveillance network.
Description of data processing
The first station of TIRNet network was installed on June 2004 at Vesuvius crater and after this date several technological improvements were applied to the network stations. All station are equipped with FLIR SC645/655 infrared cameras at present time. These cameras acquire IR frames at 640x480 resolution in the 7.5-13 μm thermal infrared bandwidth. Sensor accuracy is ± 2°C and thermal sensibility is 30 mK (at 50/60 Hz).
The thermal infrared Remote Monitoring Station (RMS) performs daily automated acquisition of IR images and their upload to a server of the INGV-Osservatorio Vesuviano Surveillance Center in Naples (Italy). IR RMS was designed and developed by the Thermal Infrared Laboratory of the Osservatorio Vesuviano and both its hardware and software are constantly technologically upgraded.
In the figure on the right side are illustrated the main components of the IR RMS:
A FLIR IR camera, protected by a stainless steel case with Germanium window, and an air Temperature and Humidity probe are connected to the IR RMS. The probe is necessary to real-time correct the IR frames acquired by the FLIR camera. Whole system is handled by dedicated software developed in Python programming language.
IR RMS main components
The acquired IR frames are uploaded to the acquisition server in the Osservatorio Vesuviano data center and processed by the automated software A.S.I.R.A. (Automated System for IR Analysis; Sansivero et al., 2019) developed by the OV Thermal Infrared Laboratory. This software extracts surface temperature time-series and heat-flux estimations of the monitored volcanic areas by processing IR data. These time-series values are plotted in the Monitoring Room of Osservatorio Vesuviano to improve volcanic surveillance.
Main data processing phases implemented in ASIRA are illustrated in the following flowchart.
Sansivero, F.; Scarpato, G.; Vilardo, G. The automated infrared thermal imaging system for the continuous long-term monitoring of the surface temperature of the Vesuvius crater. Ann. Geophys. 2013, 56, S0454.
Vilardo, G.; Sansivero, F.; Chiodini, G. Long-term TIR imagery processing for spatiotemporal monitoring of surface thermal features in volcanic environment: A case study in the Campi Flegrei (Southern Italy). J. Geophys. Res. Solid Earth 2015, 120, 812–826.
Sansivero, F.; Vilardo, G. Processing Thermal Infrared Imagery Time-Series from Volcano Permanent Ground-Based Monitoring Network. Latest Methodological Improvements to Characterize Surface Temperatures Behavior of Thermal Anomaly Areas. Remote Sens. 2019, 11, 553. https://doi.org/10.3390/rs11050553
