BETTER UNDERSTANDING THE EARLY ERUPTIVE HISTORY OF MT. ST. HELENS THROUGH IMPROVED MICROANALYSIS OF TEPHRA GLASSES
Mt. St. Helens has a long history with many major eruptions and is a key source of volcanic ash. Because eruptions that were closely-spaced in time have very similar volcanic glass compositions, distinguishing ash from different eruptions can be challenging. Careful analytical work and relatively high precision data are needed.
At Concord, we have developed analytical routines that are up to the task. We have applied them to some of the earliest tephras from Mt. St. Helens. Analyses of glass shards from the "Set C" layers using the electron microprobe show small but reproducible differences in the abundances of several major and minor element oxides. In addition, the Cs and Cy layers, once thought to be possibly from the same eruption, are clearly different. For example, the Cs, Cy, and Cw layers, contain 0.9, 1.0, and 1.2 wt% FeO and 4.1, 4.5, and 4.3 wt% Na2O, respectively. Additionally, Cs differs from both Cy and Cw by higher TiO2 and MgO (0.05 and 0.15 wt%, respectively) while Cw contains 0.15 wt% lower K2O than Cs and Cy. This electron microprobe approach can now be applied to other Mt. St. Helens ash samples from around the region. With further analyses we also hope to better understand the history of the volcano.
This research was conducted in Concord University’s Electron Microprobe Laboratory, a regional teaching and research facility supported by the WV Research Trust Fund and WV EPSCoR.