The role of cooling horizons in genesis of hydrocarbon deposits

Resumo

The penetration of fluid flow through cooling horizons resulted in the condensation of the gaseous phase in the course of chemical reactions of natural hydrocarbon synthesis (HS) owing to the occurrence of simple postmagmatic fluid compounds (H₂, CO₂, H₂S). In practice it is possible to use aerospace infrared remote sensing to search for hydrocarbon deposits genetically associated with cooling horizons.