The vast majority of theses in this collection are open access and freely available. There are a small number of theses that have access restricted to the WWU campus. For off-campus access to a thesis labeled "Campus Only Access," please log in here with your WWU universal ID, or talk to your librarian about requesting the restricted thesis through interlibrary loan.
Date Permissions Signed
8-4-2022
Date of Award
Summer 2022
Document Type
Masters Thesis
Department or Program Affiliation
Geology
Degree Name
Master of Science (MS)
Department
Geology
First Advisor
Caplan-Auerbach, Jacqueline
Second Advisor
Roland, Emily Carlson
Third Advisor
Chadwick, William W.
Fourth Advisor
Dziak, Robert P.
Abstract
West Mata Volcano located in the NE Lau Basin is the site of the deepest observed submarine volcanic eruption, 1,200 meters below sea level. In May 2009, a research cruise collected video data of two eruptive vents showcasing different eruption styles. During the same research cruise, a BprobeTM portable hydrophone was deployed at the summit of West Mata and collected data that coincides with video recorded at the vents during ROV dives. These data sets were correlated to better understand the spectral signatures associated with the two eruptive vents. Both vents were near the summit, about 50 meters apart, and exhibit different eruptive styles. Hades vent exhibited bubble bursting described as Strombolian-style, while Prometheus vent exhibited active degassing, and slight lava fountaining referred to as Hawaiian-style. In December 2009, a moored hydrophone array consisting of four stations to the north, east, south, and west of West Mata collected data for up to two years. Short-term changes in eruptive behavior provide evidence of transitioning flow regimes. As Hades exhibited periods of singular bursting, while other times there were successive bursting events, it exhibited transitions from bubbly (successive bursts) to slug (singular bursts) flow. This switch in flow regime may have been caused by a slower magma rise rate that allowed bubble coalescence. Prometheus vent generated Hawaiian-style eruptions which also produced bubbly to slug flow regimes. Due to an eruptive vent filled with volcanic debris, bubbles were broken up as they moved through the rubble, thus producing the active degassing. Based on these observations, a time sequence of events is presented here to characterize the eruptive sequences at the West Mata vents, supported by the observed long-term trends in the hydrophone data and changes in bathymetry. These data are used to infer an evolution of the magmatic plumbing system during the 2009-2011 eruptive activity at West Mata.
Type
Text
Keywords
Submarine volcanism, hydroacoustics, West Mata, NE Lau Basin
Publisher
Western Washington University
OCLC Number
1340137982
Subject – LCSH
Submarine volcanoes--Polynesia; Volcanic eruptions--Polynesia; Underwater acoustics--Polynesia
Geographic Coverage
Polynesia
Format
application/pdf
Genre/Form
masters theses
Language
English
Rights
Copying of this document in whole or in part is allowable only for scholarly purposes. It is understood, however, that any copying or publication of this document for commercial purposes, or for financial gain, shall not be allowed without the author’s written permission.
Rights Statement
http://rightsstatements.org/vocab/NoC-US/1.0/
Recommended Citation
Louis, Mikkel Shanice, "Eruption Evolution of West Mata Volcano, NE Lau Basin Using Hydroacoustic and Video Data" (2022). WWU Graduate School Collection. 1124.
https://cedar.wwu.edu/wwuet/1124
Color bar script for spectrograms
date2jul.m (1 kB)
Date script for spectrograms
hydrophone_corr.m (3 kB)
hydrophone script 1
hydrophone_mata.m (3 kB)
hydrophone data West Mata
hydrophone_sdat.m (1 kB)
South hydrophone data
jfft.m (3 kB)
spectrogram filter 1
jfiltfilt.m (1 kB)
spectrogram filter 2
jspecgram.m (2 kB)
spectrogram script 1
jspecgram2.m (3 kB)
spectrogram script 2
jul2day.m (1 kB)
hydrophone data script 2
mata_all_stations.m (1 kB)
west mata data
mata_video.m (1 kB)
west mata video data
mmread.m (25 kB)
video read script
processFrame.m (3 kB)
video script
spec_color.map (1 kB)
spectrogram color scheme
0506First70sec.mp4 (6254 kB)
Eruption video 1
0506Video.mp4 (1422 kB)
Eruption video
0506Video2.mp4 (6094 kB)
Eruption video 2
0506Video3.mp4 (4998 kB)
Eruption video 3
0506Video4.mp4 (2982 kB)
Eruption Video 4
0507Video1.mp4 (6622 kB)
Eruption Day 2 Video 1
0507Video2.mp4 (7965 kB)
Eruption Day 2 Video 2
0507Video3.mp4 (7499 kB)
Eruption Day 2 Video 3
0507Video4.mp4 (4513 kB)
Eruption Day 2 Video 4
mata2.mp4 (1936 kB)