Abstract
The lower crust has long been recognized as a place where significant chemical evolution of magma occurs. Understanding the conditions that lead to long-term storage in or rapid transport through these lower crustal systems has remained a challenge. In this study, active-source seismic data are processed to image prominent reflectors in the lower crust and upper mantle near Mount St. Helens. Results show strong and weak near-Moho reflectivity located near previously inferred regions of magma storage and high-density bodies underlying volcanic centers, respectively. To explain these observations, we hypothesize that magmas intersecting the high-density lower crustal bodies experience enhanced vertical buoyancy forces/transport due to the increased density contrast between melt and host rock. The reduced reflectivity near high-density bodies is therefore a result of both decreased impedance contrasts between crust and mantle host rocks and diminished lower crust magma accumulation, which ultimately causes focusing of volcanism above these features.
| Original language | English |
|---|---|
| Article number | e2020GL090612 |
| Pages (from-to) | 1-8 |
| Number of pages | 8 |
| Journal | Geophysical Research Letters |
| Volume | 48 |
| Issue number | 5 |
| DOIs | |
| Publication status | Published - 16 Mar 2021 |
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