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Abstract

The deep-water developments of Greater Plutonio in Block 18 and PSVM (Plutao, Saturno, Venus and Marte) in Block 31 have each shown 4D seismic monitoring to be a very valuable surveillance tool in support of reservoir management. This paper describes the observations made from the 4D data across the two areas. Both areas have a mixture of channelised and sheet-like turbidite reservoirs: Greater Plutonio has a higher proportion of sheet-like reservoirs, with simple 4D anomalies. PSVM has a higher proportion of channelised reservoirs with more complex anomalies.

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/content/papers/10.3997/2214-4609.201702348
2017-10-02
2024-03-28
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http://instance.metastore.ingenta.com/content/papers/10.3997/2214-4609.201702348
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