Researchers published a paper titled: “Seafloor Direct Current Techniques for Deep Marine, Near-bottom Gas Hydrate Investigation” in The Leading Edge.
The resistivity profiles show significant changes in the distribution of high resistivity anomalies, associated with hydrate concentration, occurred from one week to the next.
Two time-lapse DCR profiles were recovered from the instruments showing images of the near subseafloor.
The research team successfully recovered the Integrated Portable Seafloor Observatory (IPSO) lander and DCR array from the seafloor at MC118 after a 5-month deployment.
The research team successfully deployed the IPSO lander and DCR array on the seafloor at MC118.
The DCR pressure housing successfully passed high-pressure testing conducted at the Southwest Research Institute in San Antonio, Texas. The tests were conducted to determine if the pressure housing could survive the pressures that exist on the seafloor at MC118, which is located at a water depth of approximately 900 meters.
Researchers identified and ranked potential sites for the deployment of the DCR array. The primary site is supported by the recovery of hydrate during the 2011 Jumbo Piston coring effort, by the identification of a significant resistivity anomaly during the 2009 DCR survey of the mound at MC118, and by anomalously high heat flow values measured across the nearby surface trace of the fault identified in the subsurface chirp data collected in 2005.
The team constructed the IPSO lander, including installing and testing the oceanographic instruments to be deployed on the lander.
Renovations to the DCR device have been made prior to its scheduled deployment at Woolsley Mound in September 2013. Four electronic cards, damaged when the instrument housing flooded last year, were replaced. O-ring groove dimensions in the instrument housing were also verified to ensure proper seating of the rings under the pressures anticipated at the seafloor at MC118.