Sidewall coring, cast thin sections and scanning electron microscopy (SEM) reveal significant differences in reservoir space types among different lithologies. The main reservoir spaces in tectonic breccia are secondary pores and fractures, including matrix dissolution pores, intergranular dissolution pores, weathering fractures, tectonic fractures and dissolution-enlarged fractures (
Figs. 3a-3c and
9a-9e). Matrix dissolution pores and intergranular dissolution pores (
Fig. 9a-9b) are relatively developed within the breccia clasts, mainly as sieve-like pores. Weathering fractures (
Fig. 3b) are irregular fractures formed by weathering of volcanic rocks exposed at the surface, most developed near the weathering crust on the top of volcanic rocks, commonly presenting horsetail-like, en echelon-like, and leaf vein-like patterns. Weathering fractures intersect with tectonic fractures, dividing the rocks into blocks of varying sizes, which facilitates dissolution. Zeolites, argillaceous materials and carbonate minerals are commonly found to fill weathering fractures. Tectonic fractures (
Figs. 3a-3c,
9g) are the main fracture type in the LK7-A structure, characterized by large scale, straight fracture surfaces and long extension distances, serving as important seepage channels in volcanic reservoirs. Multiple phases of tectonic fractures and their intersections can be observed in sidewall cores, mostly filled with siliceous or carbonate minerals. Dissolution-enlarged fractures (
Fig. 9c) are formed by the secondary dissolution of feldspar, calcite, and ankerite filling in early tectonic fractures, resulting in widened fractures. The widths of the dissolution fractures vary, and they are most developed near the top weathering and dissolution zone. The main reservoir spaces in trachyte and rhyolite include primary pores, secondary pores and fractures, such as primary gas pores (
Fig. 9d), intra-crystalline dissolution pores (
Fig. 9e), condensed contraction fractures (
Fig. 9f) and tectonic fractures. Due to the low volatile content in magma, primary pores account for a small proportion, mainly as elongated primary gas pores. Condensed contraction fractures are formed during the ascent of magma to the surface and effusion, when magma contacts with relatively low-temperature surrounding rocks, air, or water and cools rapidly. During solidification, the cooling magma undergoes quenching and rapid contraction, generating tensile stress that forms fractures. The condensed contraction fractures are abundant in lava with large extension scale but small aperture and they are formed early with high overall filling degree, commonly filled or semi-filled by chlorite, calcite, or quartz. Tuff generally has poorly developed reservoir spaces, dominated by secondary pores and fractures, such as intra-crystalline dissolution pores, devitrification pores (
Fig. 9h) and microfractures. Devitrification pores are micro-pores formed by the transformation of volcanic glass from an amorphous to crystalline state, distributed in patches.