Abstract

Constraining the eruption rates of flood basalt lava flows remains a significant challenge despite decades of work. One potential observable proxy for eruption rates is flood basalt lava-flow lobe thicknesses, a topic that we tackle here quantitatively. In this study, we provide the first global compilation of pāhoehoe lava-lobe thicknesses from various continental flood basalt provinces (∼ 3,800 measurements) to compare characteristic thicknesses within and between provinces. We refer to thin lobes (∼ ≤5 m), characteristic of “compound” lavas, as hummocky pāhoehoe lava flows or flow-fields. Conversely, we term thicker lobes, characteristic of “simple” flows, as coming from sheet-lobe-dominated flows. Data from the Deccan Traps and Columbia River flood-basalt provinces are archetypal since they have the most consistent datasets as well as established chemo- and litho-stratigraphies. Examining Deccan lobe thicknesses, we find that previously suggested (and disputed) distinct temporal and regional distributions of hummocky pāhoehoe and sheet-lobe-dominated flow fields are not strongly supported by the data and that each geochemically defined formation displays both lobe types in varying amounts. Thin flow-lobes do not appear to indicate proximity to source. The modal lobe thickness of Deccan formations with abundant “thin” lava-lobes is 8 m, while the mode for sheet-lobe-dominated formations is only 17 m. Sheet-lobes up to 75–80 m are rare in the Deccan and Columbia River Provinces, and ones >100 m are exceptional globally. For other flood basalt provinces, modal thickness plots show a prevalence toward similar lobe thicknesses to Deccan, with many provinces having some or most lobes in the 5–8 m modal range. However, median values are generally thicker, in the 8–12 m range, suggesting that sheet-lobes dominate. By contrast, lobes from non-flood basalt flow-fields (e.g., Hawai’i, Snake River Plain) show distinctly thinner modes, sub-5 m. Our results provide a quantitative basis to ascertain variations in gross lava morphology and, perhaps, this will in future be related to emplacement dynamics of different flood basalt provinces, or parts thereof. We can also systematically distinguish outlier lobes (or regions) from typical lobes in a province, e.g., North American Central Atlantic Magmatic Province lava-lobes are anomalously thick and are closely related to feeder-intrusions, thus enabling a better understanding of conditions required to produce large-volume, thick, flood basalt lava-lobes and flows.

Highlights

  • Continental flood basalt (CFB) province emplacement represents some of the largest volcanic events in Earth history, associated with the biggest and longest (∼ 1,000 km; Self et al, 2008) recognized lava flow-fields on Earth

  • We address these challenges by comparing lava flow morphology across multiple CFB provinces and modern analogs with a specific focus on the Deccan Traps ( Deccan)

  • We present lava lobe thickness data based on logs made through flood-basalt lava sequences from which we can estimate the value and range of lobe thicknesses for each formation and whole CFB provinces

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Summary

INTRODUCTION

Continental flood basalt (CFB) province emplacement represents some of the largest volcanic events in Earth history, associated with the biggest (up to or perhaps > than 5,000 km3; Self et al, 2014) and longest (∼ 1,000 km; Self et al, 2008) recognized lava flow-fields on Earth. The whole range and modes of lobe thickness in each Deccan formation (Figure 5A) and sub-group (Figure 5B) are shown as univariate kernel density estimators to calculate the probability density function (PDF) of lava flow thicknesses in a data set. Whole sub-groups of the Deccan have indicative thickness PDFs (Figures 5B, 6B) that support some of the conclusions of previous studies (Bondre et al, 2004), in that the lower, older subgroup (Kalsubai) formations together have the most peaked and thinnest mode, and the upper sub-group (Wai) has the broadest mode with a mean thickness similar to that for the middle subgroup (Lonavala) formations This reflects that the Kalsubai subgroup may overall be composed of more HP-type lava flow fields than the upper two sub-groups but testing the reality and details of this suggestion require further work. It is unclear whether the typical thickness implies a typical flow rate for all CFBs or a rheological/physical constraint on the thickness to which sheet lobes can inflate

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