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EurOCEAN 2000 - Vlaams Instituut voor de Zee

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GEOPHYSICAL AND OCEANOGRAPHIC STATION FOR ABYSSAL<br />

RESEARCH: GEOSTAR 2 – ENHANCEMENTS OF THE SYSTEM<br />

FOR THE DEEP SEA SCIENTIFIC MISSION<br />

INTRODUCTION<br />

660<br />

Paolo Favali 1 , Giuseppe Smriglio 1 , Caterina Montuori 1<br />

1 Istituto Nazionale di Geofisica, Roma<br />

GEOSTAR 2 (GEophysical and Oceanographic STation for Abyssal Research) is a scientific<br />

and technological project fun<strong>de</strong>d by the European Commission in the framework of Marine<br />

Science and Technology Programme (MAST-III CT98-0183). The ongoing 2 nd phase continues<br />

the first GEOSTAR phase (CT95-0007) en<strong>de</strong>d in the 1998. The main objectives of both<br />

GEOSTAR projects are to realise and test an autonomous benthic observatory able to collect<br />

geophysical, geochemical and oceanographic data for long-term (up to1 year) in <strong>de</strong>ep-sea<br />

(4000 m). GEOSTAR realised also a <strong>de</strong>dicated <strong>de</strong>ployment/recovery system, based on a<br />

mobile docker concept, linked with the ship by an electromechanical cable (Beranzoli et al.,<br />

1998). The <strong>de</strong>ployment/recovery procedure has been <strong>de</strong>rived from the so called “two-module”<br />

concept successfully applied by NASA in many space missions (Apollo, Space Shuttles) where<br />

the Mobile Docker is both the carrier and a 2 way communication Surface-Bottom Station<br />

during all phases (e.g. for instruments check). The station is conceived to have a broad range of<br />

sensors. The simultaneous acquisition of a set of various measurements with a unique time<br />

reference can make GEOSTAR to be the first element of a future multiparametric ocean<br />

network. The presence of such a network is important consi<strong>de</strong>ring, for example, that the<br />

present distribution of land-based geophysical observatories is ina<strong>de</strong>quate for addressing<br />

important scientific issues related to many features of our planet both at global and regional<br />

scale.<br />

The first phase (1995-1998), named GEOSTAR 1, was aimed at <strong>de</strong>signing and realising the<br />

system and at verifying its performances and reliability (Favali et al., 1998, Jourdain, 1999).<br />

GEOSTAR 1 was <strong>de</strong>ployed in Adriatic Sea from August 13 th to September 2 nd , 1998 at about<br />

40 km East of Ravenna and at a <strong>de</strong>pth of 42 m. During the 3 weeks mission the acquisition<br />

system recor<strong>de</strong>d continuously for 440 hours (97.8% of the total time). A magnetic observatory<br />

and three broad band seismic stations were installed on land to integrate the geophysical<br />

measurements. The mission <strong>de</strong>monstrated reliability of the <strong>de</strong>ployment/recovery vehicle, of the<br />

sensors and efficiency of the communication system Bottom Station-surface.<br />

The second phase - started in 1999 - has the purpose to perform the first long-term scientific<br />

mission at abyssal <strong>de</strong>pth for a period of at least 6-8 months. After geological and geotechnical<br />

surveys, done during the first phase, the <strong>de</strong>ployment site was located in the Southern<br />

Tyrrhenian Sea at 25-30 km NNE of USTICA Island, at a <strong>de</strong>pth of 3400 m. From the<br />

geological and environmental point of view this site represents an optimal observation point in<br />

or<strong>de</strong>r to obtain relevant information about geodynamics and oceanography of the whole<br />

Mediterranean basin. GEOSTAR 2 will carry new equipment for geophysical and chemicalphysical<br />

analyses not available in the first phase.

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