The aim of this paper is to summarize the present knowledge reached by the authors on the carbonate ramp which developed in the iberian basin during Kimmeridgian times. Our results were obtained from a combined field analysis and computer modelling carried out in the north Iberian Chain (NE Spain). Extensive field analysis in the Ricla area (Zaragoza, NE Spain), resulted in a detailed mapping of the transition from inner to outer-ramp facies on this carbonate ramp. Three facies belts may be distinguished in this ramp. The outer ramp facies consists of marls and mudstones rhythmic facies. The inner ramp facies, located above fair-weather wave base, are dominated by coral patch reef growing. The middie ramp facies are represented by marls and micrites bearing skeletal and oolitic tempestite levels which sharply grade into high-amplitude dolitic sandwave. Factors such as resedimentation by storms, carbonato production and relative variation of sea level acting in the Kimmeridgian ramp are also quantiphied and discussed. Most of the mud accumulated in outer-ramp areas was produced in the coral "carbonate factory" located in inner areas. Off-shore resedimentation by storm was the main agent of basinward transport of this mud. The deduced accommodation curve consists of three elements: a linear rise which satisfactorily matches the normal subsidence figures observed in intracratonic basins; a third-order cycle, that may have a regional cause and higher order cycles in the Milanckovich band, that may be eustatic in origin
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