Storage, ascent and emplacement of rhyolite lavas

textThe physical properties and dynamic processes that control effusions of rhyolitic lavas are poorly constrained because of a paucity of direct observations. To assess the pre-eruptive storage conditions, eruptive ascent, and subaerial emplacement for a suite of volumetrically diverse rhyolitic lavas, I studied 10 obsidian lavas from Yellowstone Caldera, Wyoming and Mono Craters, California. Storage, ascent, and emplacement of those lavas were quantitatively constrained using phenocryst compositions, high temperature experiments, microlite textures, and compositional gradients surrounding spherulites. Compositions of phenocrysts and quartz-hosted glass inclusions indicate the magmas at Yellowstone were stored at 750±25 °C in the shallow crust (<7 km), in agreement with phase equilibria experiments. Following the initiation of an eruption, magma leaves the chamber and ascends in a conduit. Microlite number density can be used to quantify eruptive ascent rates. To generate the observed microlite number densities (10⁸·¹¹±⁰·⁰³) to 10⁹·⁴⁵±⁰·¹⁵ cm⁻³), the magmas decompressed at ~1 MPa hour⁻¹, equivalent to ascent rates of ~10 mm s⁻¹. Upon subaerial emplacement, microlites act as rigid particles in a deforming fluid (lava), and hence their 3D orientations could indicate flow direction and how strain accumulates in the fluid during flow. Microlites are strongly aligned in samples from all flows, but variations in alignment were found to be independent of flow volume or distance travelled. Together, those observations suggest that strains accumulated during subaerial transport must be small (