Istituto Nazionale di Geofisica e Vulcanologia, Italy

Slides:



Advertisements
Similar presentations
Technical Solutions for NEMO PROJECT R. Papaleo Villa OLMO, October 2001.
Advertisements

P. Sapienza, Laboratori Nazionali del Sud (INFN)NOW2004, sept A km 3 detector in the Mediterranean: status of NEMO Motivation for a km 3 detector.
N THE CRUSTAL STRUCTURE OF SOUTHERN TYRRHENIAN SEA SUBDUCTION ZONE G. Gaudiosi (1),D. Lo Bascio (1),M. Maistrello (2),G.Musacchio (2) and I. Guerra (3)
Side 1 Mat.-nat. Fak. søndag, 20. juli 2014 Norwegian participation in EMSO - European Multidisciplinary Seafloor Observation UoT J. Mienert Det matematisk–
Jan 2009 U. Katz: Astroparticle Physics 1 What is KM3NeT – the Vision  Future cubic-kilometre sized neutrino telescope in the Mediterranean Sea  Exceeds.
A.Margiotta, SNOW 2006, Stockholm, 6 May 2006 Status Report of the NEMO Project (NEutrino Mediterranean Observatory) Towards a km 3 Neutrino Telescope.
ESONET LIDO - Demo Mission: the East Sicily node The Laboratori Nazionali del Sud–INFN (Italian Institute for Nuclear Physics) has set up two cabled deep.
SUPERSITES COORDINATION WORKSHOP Monday 10 June 2013
ITU-UNESCO IOC-WMO Workshop Submarine Cables for Ocean/Climate Monitoring and Disaster Warning-Roma European Multidisciplinary Seafloor Observatory.
Introduction to future synergy options Uli Katz ECAP, Univ. Erlangen Deep Ocean Cabled Observatories Amsterdam, May 2012.
EPOS Kick-off Meeting – INGV November 2010, Roma EMSO European Multidisciplinary Seafloor Observatory Paolo Favali Istituto Nazionale di Geofisica.
All Regions Workshop #2, 5-7 Oct , Paris, France G. Riccobene – LNS / INFN The East Sicily Node Facilities Giorgio Riccobene INFN-LNS, Catania
KM3Net and EMSO: joint approach for the Earth and Sea Sciences Giuditta Marinaro on behalf of EMSO Consortium KM3Net Collaboration Meeting – Catania –
Work on GEOSTAR included ESONET LIDO - Demo Mission: the Cadiz node INGV activities D. Embriaco, G. Marinaro, G. Giovanetti, S. Monna, G. Cianchini, M.
NEAREST kick-off Meeting 9-11 October, Bologna NEARESTWP4 INGV: Leader PI: Paolo Favali.
4 th International Workshop on Very Large Volume Neutrino Telescopes for the Mediterranean Sea October 2009, Athens, Greece NEMO-SN1 observatory.
Hanoi, Aug. 6-12, 2006 Pascal Vernin 1 Antares Status report P.Vernin CEA Saclay, Dapnia On behalf of the Antares collaboration P.Vernin
TFH Berlin Deployment technologies of seafloor observatories Hans W. Gerber Dept. Mechanical Engineering TFH Berlin, University of Applied Sciences, Germany.
Listening to the Deep-Ocean Environment ESONET (European Sea-Floor Observatories Network) 5-7 Oct. 2009All Regions Workshop #2.
C.DistefanoCRIS 2008 – Salina, September The KM3Net Consortium Istituto Nazionale di Fisica Nucleare Laboratori Nazionali del Sud Towards a km3-scale.
All Regions Workshop #2, Paris 5-7th Oct V. Lykousis 1 and A. Tselepides 2 1 Hellenic Centre for Marine Research 2 University of Pireous
Mr.Santosh Kumar Scientist Web:
The role of gliders in sustained observations of the ocean Deliverable 4.1 or WP 4.
A new concept of observatories for long term seabed monitoring lfremer Paris, mars 2004Atelier Expérimentation Instrumentation ASSEM : A new.
Labeled Test-site of the European projects ESONET & EMSO Dr. Juanjo Dañobeitia UTM – CSIC & SARTI (UPC) SPAIN.
Final General Assembly – Paris, France – September 19, 2014 FP7-Infra : Design studies for European Research Infrastrutures 1st October 2011.
INFN Bari, Bologna, Catania, Genova, LNF, LNS, Napoli, Pisa, Roma Università Bari, Bologna, Catania, Genova, Napoli, Pisa, Roma “La Sapienza” CNR Istituto.
Strategy for building the infrastructure of EMSO - Norwegian node - Bénédicte Ferré & Jürgen Mienert Institute of Geology University of Tromsø All Regions.
Laura Beranzoli Istituto Nazionale di Geofisica e Vulcanologia October 5-7, 2009ESONET NoE - 2nd All Region Workshop WP4 – Demonstration Missions.
Session 4A - In situ Sustained Eulerian Observatories Richard Lampitt (1) & Paolo Favali (2) (1) National Oceanography Centre Southampton, UK (2) Istituto.
The NEMO Project: Toward a km 3 Neutrino Telescope in the Mediterranean Sea M. Circella, INFN Bari NUPPAC-05, Nov The NEMO Project (NEutrino Mediterranean.
 NEMO The NEMO Status Report M.Taiuti on behalf of the NEMO Collaboration Merida, Yucatan, Mexico 30th International Cosmic Ray Conference.
IES Integration of research activities on a long-term perspective Co-operation between universities, research institutes, enterprises and technology organisations.
Isabella Amore Laboratori Nazionali del Sud - INFN, Catania International School of Cosmic Ray Astrophysics 15th Course: "Astrophysics at Ultra-high Energies"
EuroGOOS Annual Meeting 2009/10/ /10/08 ESONET All Regions Workshop 2009, October 5-7 th, Paris Integrating and Enhancing the European capacity for.
The KM3NeT consortium ( - supported through the European Union's 6th framework programme in a 3-year Design Study - aims at the construction.
Universitat Politècnica de Catalunya Michel André MEUST: Real-time Monitoring of Noise and Acoustic Events in Cetacean Acoustic Niches.
NEMO-O DE NEMO First results from the NEMO Test Site G. Riccobene, for the NEMO Collaboration The NEMO Collaboration is performing the Phase 1 of the project,
G. Riccobene, INFN-LNS Nikhef, May 24-25, 2012 Giorgio Riccobene INFN-Laboratori Nazionali del Sud Abyssal undular vortices in the Eastern Mediterranean.
EGI Technical Forum 18 September Authors: P. Favali (INGV), G. Riccobene (INFN), L. Badiali (INGV), D. Cesini (INFN), G. Giovanetti, (INGV), E.
BY K.MOUNIKA CSE 4 TH YEAR. What is a Tsunami? A tsunami is a wave in the ocean or in a lake that is created by a geologic event characterized by a series.
NEAREST Meeting 8-9 May, Barcelona NEARESTWP4 Leader: INGV INGV Team: Laura Beranzoli, Davide Embriaco, Paolo Favali, Francesco Frugoni, Marco Lagalante,
International Workshop on a Very Large Volume Neutrino Telescope for the Mediterranean Sea VLVnT08 - Toulon Paolo Favali Istituto Nazionale di Geofisica.
EGI Community Forum 27 March Giuditta Marinaro 1.
ARENA08 Roma June 2008 Francesco Simeone (Francesco Simeone INFN Roma) Beam-forming and matched filter techniques.
Isabella Amore VLV T08, Toulon, France April 2008 International Workshop on a Very Large Volume Neutrino Telescope for the Mediterranean Sea Results.
EMSO European Multidisciplinary Seafloor and Water-Column Observatory Lucio Badiali on behalf of the EMSO Consortium.
LIDO Demonstration Mission (LIDO-DM) “LIstening to the Deep Ocean” The DM objectives are: geo-hazard and bio-acoustics LIDO-DM will operate a first nucleus.
Status of the LIDO East Sicily Station F.Bruni.
SEA operations – June 2012 Short summary report R. Papaleo 22 june 2012.
Earth-Sea Science Junction Boxes
Deep sea infrastructure: ROV M. Musumeci KM3NET meeting Paris October 2008.
European Multidisciplinary Seafloor and Water Column Observatory - Portugal (EMSO-PT) Nuno Lourenço – (on behalf of Miguel Miranda)
Begoña Pérez Gómez, Puertos del Estado, Spain
University of Bologna Bologna (Italy)
Correlation between underwater noise level and AIS data in the Gulf of Catania (Sicily) Sara Pulvirenti Erice International School.
Interdisciplinary Activity ANTARES
Robert Lahmann VLVnT – Toulon – 24-April-2008
M.Taiuti on behalf of the NEMO Collaboration
LNS in numbers INFN Laboratori Nazionali del Sud are located in the Catania University campus area Total area: m2 Total volume: m3 Staff members:
Laura Beranzoli Istituto Nazionale di Geofisica e Vulcanologia
(NEutrino Mediterranean Observatory): Toward a km3 Neutrino Telescope
Massimiliano Drudi (INGV) Ugo Di Giammatteo (ACS)
I EMSO European Multidisciplinary Seafloor and water-column Observatory Paolo Favali on behalf of EMSO Consortium
Junction Boxes for KM3NeT
KM3NeT: where are we and where do we go
INGV-MOIST Case Study and INDIGO solution for:
EMSO European Multidisciplinary Seafloor Observation Paolo Favali
KM3Net… past, present, and future oppurtunities for Oceanography and Geophysics TRANSFERT OF HEAT BY DIFFUSION AND MIXING.
a Marine Environment Tests and Research Infrastructure
Presentation transcript:

Istituto Nazionale di Geofisica e Vulcanologia, Italy East Sicily Paolo Favali Istituto Nazionale di Geofisica e Vulcanologia, Italy

Western Ionian Scientific Relevance Geo-hazards Oceanography Marine Biology

Earthquakes and Tsunamis Geo-hazard Earthquakes and Tsunamis 1454-XVI XVI - 1713 1714-1814 1815-1859 1860-1917 1918-1990

INGV Seismological Instrumental Catalogue 1169 1693 1908 1990 1818 M= 7.0 M= 5.0 M= 3.0 Magnitude Geo-hazard INGV Seismological Instrumental Catalogue 1975 - 2001 Strong earthquakes 1000 – 1992

Earthquake max intensity map Geo-hazard Earthquake max intensity map

22 events (33% of the total italian tsunamis) 8 Aeolian Islands 2 Sicily Channel 4 Northern Sicily 1908 2 Messina Strait 6 Eastern Sicily 1169 - 1693 Tsunamis in Sicily 22 events (33% of the total italian tsunamis)

Geo-hazards Sharp topographic gradient: The Malta Escarpment landslides Sharp topographic gradient: The Malta Escarpment ETNA volcano

Oceanography Western Ionian involved in water mass exchange with Tyrrhenian basin Relevant site for the exchange of water masses between Eastern and Western Mediterranean

Marine Biology Key area for studying the seasonal movements of whales and sperm whales within the Mediterranean basin. (along with the Sicily channel and the Strait of Gibraltar) It can be considered a "whale gate" where to count animals moving among the western and eastern Mediterranean Sea. The area is characterized by deep waters with a steep continental shelf, potential habitat for Cuvier's beaked whales, deep divers very sensitive to anthropogenic noise.

SN-1: a GEOSTAR-class observatory Pilot experiment: October ’02 - May ‘03 (>130 days; >12 Gbyte data) Coordinates: 37° 26,533’ N, 15° 23,587’ E Depth: 2105 m

SN-1 Background seismic noise During and after Etna eruption Infra-gravity waves noise notch Micro- seismic band Short period Pressure Waves (wind) SN-1 Background seismic noise Z SN1 (black) VAE (grey) Before Etna eruption During and after Etna eruption Monna et al., GRL, 2005 Noise in high and low sea current velocity (N-S component)

Contribution to the seismicity knowledge earthquakes recorded only by SN-1 Tyrrhenian Sea Deep Ionian Basin Etna Calabria Malta Escarpement Ionian Sea SN-1 Sgroi et al., Geophys. J. Int. 2007

NEMO-SN1 Observatory layout Agreement between INFN (owner of the underwater cable) and INGV - 2001

Deployment of OƲDE and SN1 25 January 2005 Deployment of OƲDE and SN1 2060 m w.d. Hydrophones Electronics Cable-ship Pertinacia, Elettra Tlc.

Ocean noise Detection Experiment ODE Ocean noise Detection Experiment OnDE was deployed on Jan 23, 2005 Cable Layer Vessel Pertinacia

NEMO-SN1 sensors Sensor Sampling rate Three-component broad-band seismometer 100Hz Hydrophone (geophysics) 100 Hz Hydrophones (bio-acoustics) 96 KHz Gravity meter 1 Hz Scalar magnetometer 1 sample every 10 min. Three-axes single-point current meter 2Hz CTD 1 sample every 12 min.

SN1 geophysical and oceanographic station Seismological data 2005-2006 Map of epicentres of regional and local earthquakes localised by the land seismological network and SN1 data jointly. blue circles ≤ M 2, 2 < green circles ≤ M 3, 3 < yellow circles ≤ M 4, 4< red circles

Java 08.08.2007 M = 7.4 Greece, 28.08.2007 M = 4.3

The OnDE station (2005-2006) (INFN-Univ. Pavia) Study of the underwater acoustic environment to develop the strategies required for the detection of acoustic pulses generated by high energy neutrinos interacting with nuclei in seawater. % of slots with sperm whale sounds per day Daily acoustic contacts with sperm whales in the period September-December 2005. NEMO Project shows a unexpected high passage of sperm whales.

European Seafloor Observatory NETwork Artic GOALS: Geohazards Global change Biodiversity Norwegian Margin Nordic Sea ESONET EC Concerted Action (2002-2004) EC Network of Excellence (2007-2011) Porcupine Ligurian Sea Black Sea Azorre Hellenic Eastern Sicily Hyberian Margin 10 Key-sites

NEMO-SN1 Observatory layout Dec. 2006

Funded by “REGIONE SICILIANA” (2006 -2008) PROSPECTIVES PEGASO Project INGV and INFN partners Funded by “REGIONE SICILIANA” (2006 -2008) OBJECTIVES: To develop seafloor modules for environmental and geo-hazard monitoring B) To build an hybrid underwater system for the deployment, recovery and connection of complex mechanical deep-sea structures

PEGASO Project ORION-4 GMM Develop a set of small-size seafloor ‘portable’ modules for specific environmental and geo-hazard monitoring equipped with various communication systems

Deep-sea Shuttle operations PEGASO Project Deep-sea Shuttle main characteristics Cable length: 4000 m Max. operating depth: 3500 m Max. payload: 30 kN Deep-sea Shuttle operations Deployment and recovery of underwater modules (e.g., SN-1 type, junction boxes, NEMO towers) Tender on-going

PEGASO Project ROV main characteristics Umbilical Cable length (> 150 m) Max. operating depth: 4000 m ROV operations Inspection, carrying payload and connection/disconnection of underwater connectors Tender assigned

Thanks to the PEGASO system development, the NEMO-SN1 site will increase its capabilities to be an “open laboratory”, cabled node of ESONET-EMSO INFN has undertaken the preparatory phase for the realisation of an infrastructure at the Capo Passero site dedicated to the installation of the km-cube-telescope: 100 km cable down to 3500 m w.d., (deployed July 2007) a shore station