Fabrizio Marra

Dr. Fabrizio Marra


Research Focus & Metrics

Academic Career Length

15Years (2012-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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1 September 2016 in Earth and Planetary Science Letters
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Journal Article
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FMFabrizio Marra
Fabrizio Marra
ERE.J. Rohling
E.J. Rohling
fabio florindofabio florindo
fabio florindo
BJB. Jicha
B. Jicha
SNS. Nomade
S. Nomade
PRP.R. Renne
P.R. Renne



20 January 2015 in Archaeometry
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Journal Article
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FMFabrizio Marra
Fabrizio Marra
EDE. D'AMbrosio
E. D'AMbrosio
MGM. Gaeta
M. Gaeta
MMM. Mattei
M. Mattei

15 June 2016 in Geophysical Research Letters
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Journal Article
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FMFabrizio Marra
Fabrizio Marra
MGM. Gaeta
M. Gaeta
BGBiagio Giaccio
Biagio Giaccio
BJB. R. Jicha
B. R. Jicha
DPD. M. Palladino
D. M. Palladino
Salvatore StramondoSalvatore Stramondo
Salvatore Stramondo
We present new 40Ar/39Ar data which allow us to refine the recurrence time for the most recent eruptive activity occurred at Colli Albani Volcanic District (CAVD) and constrain its geographic area. Time elapsed since the last eruption (36 kyr) overruns the recurrence time (31 kyr) in the last 100 kyr. New interferometric synthetic aperture radar data, covering the years 1993–2010, reveal ongoing inflation with maximum uplift rates (>2 mm/yr) in the area hosting the most recent (<200 ka) vents, suggesting that the observed uplift might be caused by magma injection within the youngest plumbing system. Finally, we frame the present deformation within the structural pattern of the area of Rome, characterized by 50 m of regional uplift since 200 ka and by geologic evidence for a recent (<2000 years) switch of the local stress‐field, highlighting that the precursors of a new phase of volcanic activity are likely occurring at the CAVD.

26 May 2020 in Scientific Reports
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FMFabrizio Marra
Fabrizio Marra
CCC. Castellano
C. Castellano
Cucci LuigiCucci Luigi
Cucci Luigi
FFF. Florindo
F. Florindo
MGM. Gaeta
M. Gaeta
CTC. Tolomei
C. Tolomei
This multi-disciplinary work provides an updated assessment of possible future eruptive scenarios for the city of Rome. Seven new 40Ar/39Ar ages from selected products of the Monti Sabatini and Vulsini volcanic districts, along with a compilation of all the literature ages on the Colli Albani and Vico products, are used to reconstruct and compare the eruptive histories of the Monti Sabatini and Colli Albani over the last 900 ka, in order to define their present state of activity. Petrographic analyses of the dated units characterize the crystal cargo, and Advanced-InSAR analysis highlights active deformation in the MS. We also review the historical and instrumental seismicity affecting this region. Based on the chronology of the most recent phases and the time elapsed between the last eruptions, we conclude that the waning/extinguishment of eruptive activity shifted progressively from NW to SE, from northern Latium toward the Neapolitan area, crossing the city of Rome. Although Monti Sabatini is unaffected by the unrest indicators presently occurring at the Colli Albani, it should be regarded as a dormant volcanic district, as the time of 70 kyr elapsed since the last eruption is of the same order of the longest dormancies occurred in the past.