Crustal Deformation of the Alban Hills Volcanic Complex (Central Italy) by Permanent Scatterers Analysis

Details Crustal Deformation of the Alban Hills Volcanic Complex (Central Italy) by Permanent Scatterers Analysis Crustal Deformation of the Alban Hills Volcanic Complex (Central Italy) by Permanent Scatterers Analysis

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004esasp.550e..36t&link_type=abstract

Proceedings of the FRINGE 2003 Workshop (ESA SP-550). 1-5 December 2003, ESA/ESRIN, Frascati, Italy. Editor: H. Lacoste. Publish

Astronomy and Astrophysics

Astrophysics

Scientific paper

The Alban Hills volcanic complex, 15 km SE of Rome, Italy, is considered a quiescent volcano, whose last erupted products have been radiometrically dated at 20 ka [1]. The area of most recent activity (maar lakes of Albano and Nemi, last magmatic products younger than 23 ka, Funiciello et al., in press) experienced periodical unrest episodes documented since the Roman age. They consist of intermittent swarms of moderate intensity earthquakes (Fig. 1; [2]; [3]; [4]), of occasional episodes of magmatic CO2 release ([5]), of lahar events due to catastrophic lake overspills ([6]), and of considerable surface deformation ([7]; [3]).

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