QUANTITATIVE 3D PETROGRAPHY USING X-RAY TOMOGRAPHY: APPLICATION TO BISHOP TUFF PUMICE CLASTS
X-ray tomography yields a 3D map of the linear x-ray attenuation coefficient, which is a function of the atomic number and density of the material, and the x-ray energy used. Based on the compositional contrasts between different phases, various phases can be identified in a rock.
Pumice clasts, characterized by isolated crystals surrounded by a low-density matrix, are ideal for the application of this technique. We present our first results obtained using x-ray tomography for pumice clasts from the Bishop Tuff. Samples studied are from units F7, F8 and Ig2Ea and are representative of the variability in density and crystal contents observed in the early erupted Bishop.
Data were collected on the GeoSoilEnvironCARS beamline at the Advanced Photon Source, Argonne National Laboratory, using a 22 keV monochromatic x-ray beam. Image analysis was performed using the software Blob3D.
Intensity contrasts in the resulting images allow the separation of magnetite, sanidine, quartz (including minor plagioclase), glass and vesicles. Crystals smaller than 5 voxels in diameter cannot be quantified properly, mostly due to noise in the images. This constrains the spatial resolution of the resulting images; there is a trade-off between sample size and spatial resolution. We employed multiple runs with samples of varying sizes (5-10 mm) to obtain adequate resolution (voxel sizes, 7-17 μm).
We have previously studied quartz size distributions in Bishop pumice clasts using a crushing, sieving, and winnowing procedure. The agreement between our new and previous results is very good; in particular, we confirm the scarcity of quartz crystals smaller than 100 μm. We also obtained magnetite and sanidine size distributions, which are similar to those for quartz, emphasizing the significance of this depletion in small crystals.
We have just obtained our first vesicle size distributions. Integrated analysis of the crystal and vesicle size data will provide a critical test for our hypothesis of bubble rising in the Bishop magma.