Repository logo
  • English
  • Italiano
Log In
New user? Click here to register.Have you forgotten your password?
  1. Home
  2. Affiliation
  3. INGV
  4. Article published / in press
  5. Feasibility study for the microseismic monitoring of the natural gas reservoir of "SANT'ALBERTO" (Po Plain, Italy)
 
  • Details

Feasibility study for the microseismic monitoring of the natural gas reservoir of "SANT'ALBERTO" (Po Plain, Italy)

Author(s)
Carannante, Simona  
Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Milano, Milano, Italia  
D'Alema, Ezio  
Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Milano, Milano, Italia  
Lovati, Sara  
Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Milano, Milano, Italia  
Massa, Marco  
Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Milano, Milano, Italia  
Augliera, Paolo  
Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Milano, Milano, Italia  
Franceschina, Gianlorenzo  
Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Milano, Milano, Italia  
Language
English
Obiettivo Specifico
1SR. TERREMOTI - Servizi e ricerca per la Società
Status
Published
JCR Journal
JCR Journal
Peer review journal
Yes
Journal
Annals of Geophysics  
Issue/vol(year)
/60(2017)
Pages (printed)
S0217
Date Issued
2017
DOI
10.4401/ag-7111
URI
https://www.earth-prints.org/handle/2122/11215
Subjects
Induced seismicity, Microseismic monitoring, Seismic network, Ambient noise.
Abstract
In this paper we present a feasibility study for the surface seismic monitoring of the “Sant’Alberto” gas reservoir (Po Plain, Northern Italy). The project was commissioned to INGV in the framework of the activities planned by the oil & gas E&P company PoValley Energy (PVE), aiming to exploit the underground deposit. After estimating the ambient seismic noise of the area, we hypothesized a microseismic network composed of five stations installed in a 8.0 x 8.0 km 2 area centered on the surface projection of the reservoir. Moreover, due to the high noise levels observed, we also considered the possible installation of a borehole station at 200 m depth. Detection and localization
thresholds were estimated by comparing the simulated power spectral density of hypothetical seismic sources located in the crustal volume surrounding the reservoir, with the mean power spectra of the ambient seismic noise observed (or hypothesized) at each station-site. Two crustal volumes for the earthquakes detection were considered: the inner domain of detection, DI (8.6 x 8.6 x 4.0 km 3 ), within which we should ensure the highest network performance, and the extended domain of detection, DE (18.6 x 18.6 x 9.0 km 3 ). After estimating the background level of ambient seismic noise, simulations show that: 1) five surface stations installed within the surface projection of DI ensure
localization thresholds ranging between M L 0.7 and 0.8 within DI; 2) the installation of the borehole station allows to improve the detection threshold everywhere within DI, and down to M L = -0.4 nearby the reservoir; and 3) localization thresholds obtained in the crustal volume included in DE, but not in DI, show values around M L = 1.0.
Type
article
File(s)
Loading...
Thumbnail Image
Name

CarannanteEtAl_2017_Annals.pdf

Size

5.17 MB

Format

Adobe PDF

Checksum (MD5)

0b302cc679cbfae6c7fd06b13461bf51

rome library|catania library|milano library|napoli library|pisa library|palermo library
Explore By
  • Research Outputs
  • Researchers
  • Organizations
Info
  • Earth-Prints Open Archive Brochure
  • Earth-Prints Archive Policy
  • Why should you use Earth-prints?
Earth-prints working group
⚬Anna Grazia Chiodetti (Project Leader)
⚬Gabriele Ferrara (Technical and Editorial Assistant)
⚬Massimiliano Cascone
⚬Francesca Leone
⚬Salvatore Barba
⚬Emmanuel Baroux
⚬Roberto Basili
⚬Paolo Marco De Martini

Built with DSpace-CRIS software - Extension maintained and optimized by 4Science

  • Privacy policy
  • End User Agreement
  • Send Feedback