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Cluster Analysis of Thermal Icequakes Using the Seismometer to Investigate Ice and Ocean Structure (SIIOS): Implications for Ocean World SeismologyOcean Worlds are of high interest to the planetary community due to the potential habitability of their subsurface oceans. Over the next few decades several missions will be sent to ocean worlds including the Europa Clipper, Dragonfly, and possibly a Europa lander. The Dragonfly and Europa lander missions will carry seismic payloads tasked with detecting and locating seismic sources. The Seismometer to Investigate Ice and Ocean Structure (SIIOS) is a NASA PSTAR funded project that investigates ocean world seismology using terrestrial analogs. The goals of the SIIOS experiment include quantitatively comparing flight-candidate seismometers to traditional instruments, comparing single-station approaches to a small-aperture array, and characterizing the local seismic environment of our field sites. Here we present an analysis of detected local events at our field sites at Gulkana Glacier in Alaska and in Northwest Greenland approximately 80 km North of Qaanaaq, Greenland. Both field sites passively recorded data for about two weeks. We deployed our experiment on Gulkana Glacier in September 2017 and in Greenland in June 2018. At Gulkana there was a nearby USGS weather station which recorded wind data. Temperature data was collected using the MERRA satellite. In Greenland we deployed our own weather station to collect temperature and wind data. Gulkana represents a noisier and more active environment. Temperatures fluctuated around 0°C, allowing for surface runoff to occur during the day. The glacier had several moulins, and during deployment we heard several rockfalls from nearby mountains. In addition to the local environment, Gulkana is located close to an active plate boundary (relative to Greenland). This meant that there were more regional events recorded over two weeks, than in Greenland. Greenland’s local environment was also quieter, and less active. Temperatures remained below freezing. The Greenland ice was much thicker than Gulkana (~850 m versus ~100 m) and our stations were above a subglacial lake. Both conditions can reduce event detections from basal motion. Lastly, we encased our Greenland array in an aluminum vault and buried it beneath the surface unlike our array in Gulkana where the instruments were at the surface and covered with plastic bins. The vault further insulated the array from thermal and atmospheric events.

Document ID
20200001816
Acquisition Source
Marshall Space Flight Center
Document Type
Conference Paper
Authors
Marusiak, A. G.
(Maryland Univ. College Park, MD, United States)
Schmerr, N. C.
(Maryland Univ. College Park, MD, United States)
Avenson, B.
(Silicon Audio, Inc. Austin, TX, United States)
Bailey, S. H.
(University of Arizona Tucson, AZ, United States)
Bray, V. J.
(University of Arizona Tucson, AZ, United States)
Dahl, P.
(Washington Univ. Seattle, WA, United States)
DellaGiustina, D. N.
(University of Arizona Tucson, AZ, United States)
Pettit, E.C.
(Oregon State Univ. Corvallis, OR, United States)
Wagner, N.
(Alaska Univ. Fairbanks, AK, United States)
Weber, R. C.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Date Acquired
March 19, 2020
Publication Date
March 16, 2020
Subject Category
Space Sciences (General)
Report/Patent Number
MSFC-E-DAA-TN76954
Report Number: MSFC-E-DAA-TN76954
Meeting Information
Meeting: Lunar and Planetary Science Conference
Location: The Woodlands, TX
Country: United States
Start Date: March 16, 2020
End Date: March 20, 2020
Sponsors: Lunar and Planetary Institute (LPI)
Funding Number(s)
CONTRACT_GRANT: 80NSSC17K0229
CONTRACT_GRANT: 80NSSC18K1260
Distribution Limits
Public
Copyright
Public Use Permitted.
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