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Advanced PRocedures for volcanIc and Seismic Monitoring

Advanced PRocedures for volcanIc and Seismic Monitoring

Objective

APHORISM project proposes the development and testing of two new methods to combine Earth Observation satellite data from different sensors, and ground data. The aim is to demonstrate that this two types of data, appropriately managed and integrated, can provide new improved Copernicus products useful for seismic and volcanic crisis management.

The first method, APE – A Priori information for Earthquake damage mapping, concerns the generation of maps to address the detection and estimate of damage caused by a seism. The use of satellite data to investigate earthquake damages is not an innovative issue. We can find a wide literature and projects concerning such issue, but usually the approach are only based on change detection techniques and classifications algorithms. The novelty of APE relies on the exploitation of a priori information derived by InSAR time series to measure surface movements, shakemaps obtained from seismological data, and vulnerability information. This a priori information is then integrated with change detection map to improve accuracy and to limit false alarms.

The second method deals with volcanic crisis management. The method, MACE - Multi-platform volcanic Ash Cloud Estimation, concerns the exploitation of GEO (Geosynchronous Earth Orbit) sensor platform, LEO (Low Earth Orbit) satellite sensors and ground measures to improve the ash detection and retrieval and to characterise the volcanic ash clouds. The basic idea of MACE consists of an improvement of volcanic ash retrievals at the space–time scale by using both the LEO and GEO estimations and in-situ data. Indeed the standard ash thermal infrared retrieval is integrated with data coming from a wider spectral range from visible to microwave. The ash detection is also extended in case of cloudy atmosphere or steam plumes.

APE and MACE methods have been defined in order to provide products oriented toward the next ESA Sentinels satellite missions.

Coordinator

ISTITUTO NAZIONALE DI GEOFISICA E VULCANOLOGIA

Address

Via Di Vigna Murata 605
00143 Roma

Italy

Activity type

Higher or Secondary Education Establishments

EU Contribution

€ 567 824

Administrative Contact

Sofia Mariano (Ms)

Participants (6)

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CENTRE TECNOLOGIC DE TELECOMUNICACIONS DE CATALUNYA

Spain

EU Contribution

€ 290 873

BUREAU DE RECHERCHES GEOLOGIQUES ET MINIERES

France

EU Contribution

€ 260 048

UNIVERSITA DEGLI STUDI DI ROMA LA SAPIENZA

Italy

EU Contribution

€ 336 800

GAMMA REMOTE SENSING RESEARCH AND CONSULTING AG

Switzerland

EU Contribution

€ 188 000

THE CHANCELLOR, MASTERS AND SCHOLARS OF THE UNIVERSITY OF OXFORD

United Kingdom

EU Contribution

€ 157 996

ALMA SISTEMI SRL

Italy

EU Contribution

€ 113 911

Project information

Grant agreement ID: 606738

Status

Closed project

  • Start date

    11 November 2013

  • End date

    1 January 2017

Funded under:

FP7-SPACE

  • Overall budget:

    € 2 477 694,40

  • EU contribution

    € 1 915 452

Coordinated by:

ISTITUTO NAZIONALE DI GEOFISICA E VULCANOLOGIA

Italy

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