Network


Latest external collaboration on country level. Dive into details by clicking on the dots.

Hotspot


Dive into the research topics where William Shedd is active.

Publication


Featured researches published by William Shedd.


Proceedings of the National Academy of Sciences of the United States of America | 2012

Impact of the Deepwater Horizon oil spill on a deep-water coral community in the Gulf of Mexico

Helen K. White; Pen-Yuan Hsing; Walter Cho; Timothy M. Shank; Erik E. Cordes; Andrea M. Quattrini; Robert K. Nelson; Amanda W.J. Demopoulos; Christopher R. German; James M. Brooks; Harry H. Roberts; William Shedd; Christopher M. Reddy; Charles R. Fisher

To assess the potential impact of the Deepwater Horizon oil spill on offshore ecosystems, 11 sites hosting deep-water coral communities were examined 3 to 4 mo after the well was capped. Healthy coral communities were observed at all sites >20 km from the Macondo well, including seven sites previously visited in September 2009, where the corals and communities appeared unchanged. However, at one site 11 km southwest of the Macondo well, coral colonies presented widespread signs of stress, including varying degrees of tissue loss, sclerite enlargement, excess mucous production, bleached commensal ophiuroids, and covering by brown flocculent material (floc). On the basis of these criteria the level of impact to individual colonies was ranked from 0 (least impact) to 4 (greatest impact). Of the 43 corals imaged at that site, 46% exhibited evidence of impact on more than half of the colony, whereas nearly a quarter of all of the corals showed impact to >90% of the colony. Additionally, 53% of these corals’ ophiuroid associates displayed abnormal color and/or attachment posture. Analysis of hopanoid petroleum biomarkers isolated from the floc provides strong evidence that this material contained oil from the Macondo well. The presence of recently damaged and deceased corals beneath the path of a previously documented plume emanating from the Macondo well provides compelling evidence that the oil impacted deep-water ecosystems. Our findings underscore the unprecedented nature of the spill in terms of its magnitude, release at depth, and impact to deep-water ecosystems.


Proceedings of the National Academy of Sciences of the United States of America | 2014

Footprint of Deepwater Horizon blowout impact to deep-water coral communities.

Charles R. Fisher; Pen-Yuan Hsing; Carl L. Kaiser; Dana R. Yoerger; Harry H. Roberts; William Shedd; Erik E. Cordes; Timothy M. Shank; Samantha P. Berlet; Miles Saunders; Elizabeth A. Larcom; James M. Brooks

Significance The Deepwater Horizon blowout released more oil and gas into the deep sea than any previous spill. Soon after the well was capped, a deep-sea community 13 km southwest of the wellhead was discovered with corals that had been damaged by the spill. Here we show this was not an isolated incident; at least two other coral communities were also impacted by the spill. One was almost twice as far from the wellhead and in 50% deeper water, considerably expanding the known area of impact. In addition, two of four other newly discovered coral communities in the region were fouled with commercial fishing line, indicating a large cumulative effect of anthropogenic activities on the corals of the deep Gulf of Mexico. On April 20, 2010, the Deepwater Horizon (DWH) blowout occurred, releasing more oil than any accidental spill in history. Oil release continued for 87 d and much of the oil and gas remained in, or returned to, the deep sea. A coral community significantly impacted by the spill was discovered in late 2010 at 1,370 m depth. Here we describe the discovery of five previously unknown coral communities near the Macondo wellhead and show that at least two additional coral communities were impacted by the spill. Although the oil-containing flocullent material that was present on corals when the first impacted community was discovered was largely gone, a characteristic patchy covering of hydrozoans on dead portions of the skeleton allowed recognition of impacted colonies at the more recently discovered sites. One of these communities was 6 km south of the Macondo wellhead and over 90% of the corals present showed the characteristic signs of recent impact. The other community, 22 km southeast of the wellhead between 1,850 and 1,950 m depth, was more lightly impacted. However, the discovery of this site considerably extends the distance from Macondo and depth range of significant impact to benthic macrofaunal communities. We also show that most known deep-water coral communities in the Gulf of Mexico do not appear to have been acutely impacted by the spill, although two of the newly discovered communities near the wellhead apparently not impacted by the spill have been impacted by deep-sea fishing operations.


Geophysics | 2006

Seafloor reflectivity : An important seismic property for interpreting fluid/gas expulsion geology and the presence of gas hydrate

Harry H. Roberts; Bob A. Hardage; William Shedd; Jesse Hunt

A bottom-simulating reflection (BSR) is a seismic reflectivity phenomenon that is widely accepted as indicating the base of the gas-hydrate stability zone. The acoustic impedance difference between sediments invaded with gas hydrate above the BSR and sediments without gas hydrate, but commonly with free gas below, are accepted as the conditions that create this reflection. The relationship between BSRs and marine gas hydrate has become so well known since the 1970s that investigators, when asked to define the most important seismic attribute of marine gas-hydrate systems, usually reply, “a BSR event.” Research conducted over the last decade has focused on calibrating seafloor seismic reflectivity across the geology of the northern Gulf of Mexico (GoM) continental slope surface to the seafloor. This research indicates that the presence and character of seafloor bright spots (SBS) can be indicators of gas hydrates in surface and near-surface sediments (Figure 1). It has become apparent that SBSs on the cont...


Eos, Transactions American Geophysical Union | 2007

Alvin Explores the Deep Northern Gulf of Mexico Slope

Harry H. Roberts; Robert S. Carney; Mathew Kupchik; Charles R. Fisher; Kim Nelson; Erin L. Becker; Liz Goehring; Stephanie Lessard-Pilon; Guy Telesnicki; Bernie B. Bernard; James M. Brooks; Monika Bright; Erik E. Cordes; Stéphane Hourdez; Jesse Hunt; William Shedd; Gregory S. Boland; Samantha B. Joye; Vladimir A. Samarkin; Meaghan Bernier; Marshall W. Bowles; Ian R. MacDonald; Helge Niemann; Cindy Petersen; Cheryl L. Morrison; Jeremy Potter

Many of the worlds productive deepwater hydrocarbon basins experience significant and ongoing vertical migration of fluids and gases to the modern seafloor. These products, which are composed of hydrocarbon gases, crude oil, formation fluids, and fluidized sediment, dramatically change the geologic character of the ocean floor, and they create sites where chemosynthetic communities supported by sulfide and hydrocarbons flourish. Unique fauna inhabit these sites, and the chemosynthetic primary production results in communities with biomass much greater than that of the surrounding seafloor.


6th International Conference on Gas Hydrates (ICGH 2008), Vancouver, BC, Canada, July 6-10, 2008 | 2008

SITE SELECTION FOR DOE/JIP GAS HYDRATE DRILLING IN THE NORTHERN GULF OF MEXICO

Deborah R. Hutchinson; Dianna Shelander; Jianchun Dai; Dan McConnell; William Shedd; Matthew Frye; Carolyn D. Ruppel; Ray Boswell; Emrys Jones; Timothy S. Collett; Kelly Rose; Brandon Dugan; Warren T. Wood; Tom Latham

Studies of geologic and geophysical data from the offshore of India have revealed two geologically distinct areas with inferred gas hydrate occurrences: the passive continental margins of the Indian Peninsula and along the Andaman convergent margin. The Indian National Gas Hydrate Program (NGHP) Expedition 01 was designed to study the occurrence of gas hydrate off the Indian Peninsula and along the Andaman convergent margin with special emphasis on understanding the geologic and geochemical controls on the occurrence of gas hydrate in these two diverse settings. NGHP Expedition 01 established the presence of gas hydrates in Krishna- Godavari, Mahanadi and Andaman basins. The expedition discovered one of the richest gas hydrate accumulations yet documented (Site 10 in the Krishna-Godavari Basin), documented the thickest and deepest gas hydrate stability zone yet known (Site 17 in Andaman Sea), and established the existence of a fully-developed gas hydrate system in the Mahanadi Basin (Site 19).


Proceedings of the National Academy of Sciences of the United States of America | 2012

Reply to Boehm and Carragher: Multiple lines of evidence link deep-water coral damage to Deepwater Horizon oil spill

Helen K. White; Pen-Yuan Hsing; Walter Cho; Timothy M. Shank; Erik E. Cordes; Andrea M. Quattrini; Robert K. Nelson; Amanda W.J. Demopoulos; Christopher R. German; James M. Brooks; Harry H. Roberts; William Shedd; Christopher M. Reddy; Charles R. Fisher

Our original study (1) used visual inspection as well as biological and geochemical analyses of corals and the surrounding sediment to provide complementary and compelling evidence linking the Deepwater Horizon (DWH) oil spill to the presence of damaged deep-water corals and brittle stars 11 km from the site of the leaking oil.


Geophysical Research Letters | 2016

The connection between natural gas hydrate and bottom‐simulating reflectors

Urmi Majumdar; Ann E. Cook; William Shedd; Matthew Frye

Bottom-simulating reflectors (BSRs) on marine seismic data are commonly used to identify the presence of natural gas hydrate in marine sediments, although the exact relationship between gas hydrate and BSRs is undefined. To clarify this relationship we compile a data set of probable gas hydrate occurrence as appraised from well logs of 788 industry wells in the northern Gulf of Mexico. We combine the well log data set with a data set of BSR distribution in the same area identified from 3-D seismic data. We find that a BSR increases the chances of finding gas hydrate by 2.6 times as opposed to drilling outside a BSR and that the wells within a BSR also contain thicker and higher resistivity hydrate accumulations. Even so, over half of the wells drilled through BSRs have no detectable gas hydrate accumulations and gas hydrate occurrences and BSRs do not coincide in most cases.


Archive | 2009

Multicomponent Seismic Technology Assessment of Fluid-gas Expulsion Geology and Gas-hydrate Systems: Gulf of Mexico

Bob A. Hardage; Paul E. Murray; Randy Remington; M. De Angelo; Diana Sava; Harry H. Roberts; William Shedd; Jesse Hunt

Four-component ocean-bottom-cable (4-C OBC) seismic data acquired in deep water across the Gulf of Mexico were used to study near-sea-floor geologic characteristics of fluid-gas expulsion systems. Although these 4-C OBC data were acquired to evaluate oil and gas prospects far below the sea floor, the data have great value for studying near-sea-floor geology. The research results summarized here stress the importance of the converted-shear-wave (P-SV) mode extracted from 4-C OBC data. In deep water, the P-SV mode creates an image of near-sea-floor strata that has a spatial resolution an order of magnitude better than the resolution of compressional wave (P-P) data regardless of whether the P-P data are acquired with OBC technology or with conventional towed-cable seismic technology. This increased resolution allows the P-SV mode to define seismic sequences, seismic facies, small-throw faults, and small-scale structures that cannot be detected with P-P seismic data.


Journal of the Acoustical Society of America | 2011

Acoustic properties of natural gas hydrates and the geophysical assessment of the subsurface distribution of hydrates in the Gulf of Mexico and Atlantic.

William Shedd; Matt Frye; Paul Doucette Godfriaux; Kody Kramer

Natural gas hydrates are a solid form of natural gas found in the deep water marine margins of continents and under permafrost in Arctic regions worldwide. They have been recognized as a very significant potential energy source in the future. They form under high pressure and low temperature. Hydrate saturated sediments are acoustically faster and slightly less dense than water saturated sediments, but much faster and denser than gas saturated sediments. These properties allow for the identification of marine hydrate saturated sediments that are underlain by gas saturated sediments. The resulting geophysical reflector, referred to as a bottom simulating reflector, or BSR, often mimics the seafloor in areas where geothermal gradient is laterally consistent. The Bureau of Ocean Energy Management, Regulation, and Enforcement has used three‐dimensional seismic data in the Gulf of Mexico and two‐dimensional seismic data in the Atlantic to (1) map the distribution of BSRs, (2) drill six wells in the GOM with mo...


Marine and Petroleum Geology | 2012

Subsurface gas hydrates in the northern Gulf of Mexico

Ray Boswell; Timothy S. Collett; Matthew Frye; William Shedd; Daniel R. McConnell; Dianna Shelander

Collaboration


Dive into the William Shedd's collaboration.

Top Co-Authors

Avatar

Matthew Frye

United States Minerals Management Service

View shared research outputs
Top Co-Authors

Avatar

Harry H. Roberts

Louisiana State University

View shared research outputs
Top Co-Authors

Avatar

Ray Boswell

United States Department of Energy

View shared research outputs
Top Co-Authors

Avatar

Jesse Hunt

United States Minerals Management Service

View shared research outputs
Top Co-Authors

Avatar

Timothy S. Collett

United States Geological Survey

View shared research outputs
Top Co-Authors

Avatar
Top Co-Authors

Avatar
Top Co-Authors

Avatar

Paul Doucette Godfriaux

United States Minerals Management Service

View shared research outputs
Top Co-Authors

Avatar
Researchain Logo
Decentralizing Knowledge