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Abstract

It is commonly considered that reservoir properties of Peritethyan carbonates mostly originated<br>from intense dissolution (vugs, molds, enlarged fractures, caverns) in a variety meteoric<br>diagenetic environments. This dissolution took place prior to the burial by non-reservoir or seal<br>units, under unconformities of different orders of magnitude or in shallow, near-surface aquifers.<br>Primary depositional porosities are seen as extensively obliterated by cementation and<br>compaction.

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/content/papers/10.3997/2214-4609.201405769
2002-05-27
2024-04-26
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http://instance.metastore.ingenta.com/content/papers/10.3997/2214-4609.201405769
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