Comportamiento geoquimico de las formaciones salinas bajo el efecto de la temperatura y la irradiacion

La generación de defectos cristalinos y la migración de las fases fluidas (salmueras y gases), son los efectos más relevantes de la irradiación y la temperatura sobre una formación salina, susceptible de albergar un almacenamiento de residuos radiactivos. Para determinar dichos efectos se ha puesto a punto la metodología necesaria y se ha verificado sobre muestras salinas de la mina de Sallent (Barcelona). El contenido en agua oscila entre 0,04 y 1 %. Sin embargo, la cantidad de salmuera susceptible de migrar será inferior a la total, debido a que parte de esta se encuentra en inclusiones fluidas inferiores a 100 mm. La composición química de la salmuera, factor clave para el estudio de corrosión de contenedores, es de carácter magnésico (1,15 moles/litro) y potásico (0,31 moles/litro) en el caso de las inclusiones. El análisis de los gases presentes indica la ausencia de gases tóxicos y concentraciones muy bajas de hidrógeno y metano. Finalmente, se ha observado que la generación de defectos por irradiación, está en relación directa con la presencia de impurezas en la roca, siendo concordantes los resultados experimentales con las predicciones del modelo de JainLidiard.

Diagenetic processes in a partially dolomitized carbonate reservoir: Casablanca oil field, Valencia Trough, offshore Spain.

Mesozoic and Neogene carbonates located in the Valencia Trough (offshore Spain, western Mediterranean Sea)are oil reservoirs. This paper investigates the diagenetic evolution of the Upper Jurassic limestones, currently dolomitized, that constitute the main reservoir of the Casablanca oil field. Core samples from Casablanca-1A well have been studied to determine the diagenetic products and their relation with porosity evolution, and to reconstruct the fluid flow history prior to and during oil emplacement. On the basis of petrological observations and geochemical analyses (major, minor and trace element composition and oxygen, carbon and strontium isotope composition), a major dolomitization event is recognized postdating subaerial exposure, erosion and karstification. The dolomitization event originated two replacive dolomites (RD1 and RD2) and two dolomite cements (saddle dolomite cement, SDC, and milky-white dolomite cement, MDC)which are partially cogenetic. RD1, RD2 and SDC precipitated at increasing temperatures (over 60ºC and below 110ºC), probably from meteoric water mixed with marine water. The last dolomite type milky-white dolomite cement) precipitated with increasing burial conditions and by arrival of hydrothermal fluids during the Miocene. The post-dolomitization sequence comprises precipitation of calcite cement and partial calcitization of all previous dolomites. The oxygen, carbon and strontium isotope compositions suggest that this calcite cementation occurred from meteoric waters mixed with Burdigalian - Langhian marine waters trapped in the sediments and expelled by compaction in the moderate to deep burial realm. Normal faults were the conduits for upward migration of these fluids as well as for later oil expulsion from the Burdigalian - Langhian source rocks. Late corrosion associated with organic acid-enriched fluids took place prior or simultaneously to oil migration during the Pliocene, enhancing porosity and increasing eservoir quality.