5 Magma Ascent to Magma Mingling, Volatility, and Volcanism: A Session in Honor of Sheila J. Seaman
Sunday, 14 March 2021
1:30 PM - 5:30 PM
Monson
MORPHOLOGY, ORIENTATION, AND DISTRIBUTION OF EXPLOSIVE CRATERS IN THE NYAMBENI HILLS VOLCANIC FIELD
Paper number: 5-12
Program: Symposia Sessions
Time: 4:40 PM – 4:50 PM
Authors
-
Cora Van HazingaSalem State University, Salem, MA
-
James MuirheadUniversity of Auckland, Auckland
-
Sara ManaSalem State University, Salem, MA
Abstract
Here we present our findings on the analysis of these explosive volcanic features found in NHVF. Google Earth Pro is utilized to map outlines of craters and cones. The morphometry of each cone is analyzed for erosional marks and slope angle to determine the area and shape of the original feature before erosion. The degree of confidence for each feature is reported to allow for a more informed data analysis. ArcGIS is used to find minimum bounding geometry data. Trends of the long axes of high confidence features with a short axis/long axis ratio greater than 1.2 provide an estimate of the orientation of that feature and are graphically expressed in a rose diagram.
Data has been collected on >100 cones within the northeastern slopes of the NHVF. Here both the long axis of the most reliable basaltic scoria cones and the linear distribution of the various features, represented by the near angle relationships of all cones, indicate a general NE-SW trend. This bearing diverges from the overall N-S trend of the rift but is similar to the observed orientation of other volcanic features in the Kenya Rift (e.g. Mega Volcanic Field, South Natron and Marsabit). A NE-SW trend could suggest a NW-SE orientation of σ3 or could be explained by the presence of pre-existing lithospheric weaknesses in the host rock influencing the direction of dikes.
Geological Society of America Abstracts with Programs. Vol. 53, No. 1
doi: 10.1130/abs/2021NE-361666
© Copyright 2021 The Geological Society of America (GSA), all rights reserved. Permission is hereby granted to the author(s) of this abstract to reproduce and distribute it freely, for noncommercial purposes. Permission is hereby granted to any individual scientist to download a single copy of this electronic file and reproduce up to 20 paper copies for noncommercial purposes advancing science and education, including classroom use, providing all reproductions include the complete content shown here, including the author information. All other forms of reproduction and/or transmittal are prohibited without written permission from GSA Copyright Permissions.