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  • Deepwater Hydrocarbon Seep Detection: Tools and

    Techniques using Multibeam Echosounders

    Garrett Mitchell1, Jim Gharib2, David Millar3

    1Project Geoscientist, Fugro Marine GeoServices, Inc. 6100 Hillcroft, Houston, Texas 77274

    Email:[email protected] Phone: + 1 (713) 778-6880 2Global Product Line Manager for Seep Studies, Fugro Marine GeoServices, Inc. Houston, Texas 3President, Fugro Pelagos, Inc. San Diego, California

    Abstract

    Despite recent declines in oil and gas market expenditures, demand for marine hydrocarbon seep

    surveys continues to grow. Geochemical analysis of seafloor seep sediments is an effective

    hydrocarbon exploration tool. Identifying and sampling sites where thermogenic hydrocarbon

    fluids have migrated to the seafloor provides information on reservoir characteristics and

    commercial viability. Hydrocarbon seep features are ephemeral, small, discrete, and often difficult

    to precisely sample on the deep seafloor. Low to mid-frequency multibeam echosounders are an

    efficient exploration tool to remotely locate and map seafloor features associated with seepage.

    Geophysical signatures from hydrocarbon seeps are evident in bathymetric datasets (fluid

    expulsion features), seafloor backscatter datasets (carbonate outcrops, gassy sediments, methane

    hydrate deposits), and midwater backscatter datasets (gas bubble and oil droplet plumes).

    Interpretation of these geophysical seep signatures in backscatter datasets is a fundamental

    component of seep hunting. Degradation of backscatter datasets resulting from environmental,

    geometric, and system noise can interfere with the detection and delineation of seeps. We present

    a relative backscatter intensity normalization method and a 2X acquisition technique that can

    enhance the geologic resolution within seafloor backscatter datasets and ultimately assist in the

    interpretation and characterization of seafloor hydrocarbon seeps. As frontier exploration surveys

    migrate into deeper waters in search of oil and gas reserves, it is necessary to evaluate and develop

    tools and techniques that improve both data quality and the interpretation of multibeam datasets.

    Fugro has conducted over fifty seep hunting campaigns globally since 2001 and include single

    exploration blocks to multi-client mega surveys in Indonesia, Brazil, and most recently an

    industry-funded multi-client seep survey the Otos multibeam survey (353,700 km2) in the

    northern Gulf of Mexico and the Gigante multibeam seep survey (625,000 km2) in the Southern

    Gulf of Mexico and Caribbean Sea. In total, over two million square kilometers of seafloor have

    been mapped with modern multibeam systems optimized to detect hydrocarbon seeps. This paper

    will provide an overview of seep detection methodologies applied during our marine seep hunting

    surveys.

    Author Biography

    Garrett Mitchell is a Project Geoscientist with Fugro Marine GeoServices, Inc. He has been

    involved with marine seep hunting surveys in the Exploration Department within Fugros Global

    Center of Excellence for Seep Studies in Houston, Texas since 2013.

    mailto:[email protected]

  • U.S. Hydro 2017

    1

    Introduction Deep seafloor exploration and the present understanding of the geomorphological and biophysical

    processes that shape it and closely linked to advances in multibeam echosounder (MBES)

    technology (Mayer, 2006). Low to mid-frequency (12 30 kHz) acoustic waves generated by

    MBES sonars can penetrate kilometers of water column and remotely measure the deep seafloor

    and shallow subsurface. Bathymetric and reflectivity measurements are both extracted from MBES

    datasets. An acoustic waves reflected energy provides information on seafloor geometry (local

    angle of incidence), physical characteristics (rugosity and density), and intrinsic properties such as

    composition, surficial and volumetric scattering (Lurton, 2010). Analyzing the geophysical

    signature of reflected acoustic beams has demonstrated to be an effective quantitative and

    qualitative tool to remotely characterize the lithologic composition and geologic nature of the

    seafloor (Fonesca and Mayer, 2007). Analyzing seafloor backscatter, and more recently midwater

    backscatter has wide-ranging applications (Colbo et al., 2014) including fisheries research

    (Trenkel at al., 2014; Innangi et al., 2016), marine biomass (Korneliussen et al., 2009), benthic

    habitat mapping (Brown and Blondel 2009), geological classification (Lamarche et al., 2011),

    subsea engineering and geohazard mitigation (Chiocci et al., 2011), and hydrocarbon seep studies

    (Orange et al., 2002; Skarke et al., 2014; Weber et al., 2010).

    The rapidly-developing science of multibeam backscatter among users in various fields is

    prone to imperfect acquisition and processing methodologies that affect quality and ultimately

    interpretability of the data. Numerous detrimental issues may exist including user error from a lack

    of commonly-accepted acquisition and processing procedures, errors in sonar installation and

    calibration, acquisition hardware and processing software settings, specular reflection, grazing

    angles, and beam pattern residuals can degrade these datasets and interfere with geologic

    interpretation. Furthermore, differences in processing algorithms within the available software

    packages can create slightly varying backscatter imagery.

    To address these issues regarding consistency of multibeam seafloor backscatter data

    quality, members of the Marine Geological and Biological Mapping Group, GeoHab

    (http://geohab.org/), an international association of seafloor mapping scientists, formed the

    Backscatter Working Group in 2013. GeoHabs BSWG published a report identifying existing

    gaps in knowledge and presenting best practices and standardized guidelines regarding the use of

    seafloor backscatter (Lurton and Lamarche, 2015). In this study, we describe our efforts into

    incorporating these guidelines and recommendations into Fugros commercial hydrocarbon seep

    hunting practices. Specifically, we present the results of our multibeam backscatter intensity

    normalization and discuss an acquisition technique used to improve backscatter data quality for

    detecting and delineating seeps on the deep seafloor.

    Hydrocarbon Seeps

    Most of Earths major hydrocarbon deposits have been located in areas where petroleum fluids

    have migrated, accumulated, and pooled at the surface (Berge, 2013). Marine petroleum seepage

    involves the flow of buoyant hydrocarbon-rich liquids that are generated by the deep burial and

    heating of kerogen-containing source rock that percolates to the seafloor (Judd and Hovland,

    2007). Most significant hydrocarbon reservoirs experience varying degrees of fluid leakage where

    failures in the top seal of a reservoir allows buoyant fluids to migrate to the surface through

    networks of faults, fractures, and fissures (Aminzadeh et al., 2013). Upwelling hydrocarbon fluids

    reaching the seafloor can influence the chemical composition of the hydrosphere (Leifer et al.,

    2000; MacDonald et al., 2002; Milkov et al., 2003), atmosphere (MacDonald et al., 2002; Leifer

    http://geohab.org/

  • U.S. Hydro 2017

    2

    et al., 2006; Solomon et al., 2009), seafloor morphology (Len et al., 2007) and mineralogy (Canet

    et al., 2006), and sustain diverse chemosynthetic communities (Fisher et al 2007; Cordes et al.,

    2009). At seafloor seeps, the anaerobic oxidation of methane (AOM) increases the alkalinity in the

    sediment promoting carbonate precipitation (Roberts et al., 2010):

    Ca2+ + 2HCO3- CaCO3 + CO2 + H2O

    Petroleum fluid interactions where chemically-reduced hydrocarbons originating from

    deep anoxic environments react with shallow sulfate-rich pore fluids and create carbonate nodules,

    chimneys, slabs, and crusts in the subsurface and seafloor. These features are indicative of both

    active and fossil seeps. Deep thermogenic hydrocarbon fluids reach the seafloor as seepage along

    fault interfaces from commercially-important oil and gas deposits. These fluids are targeted for

    geochemical sampling by the oil and gas industry because they provide insight into the petroleum

    system and contain geochemical fingerprints that can source maturity, source rock, and thermal

    history (Abrams, 2005).

    Detecting Seafloor Seeps

    Locating and sampling seafloor seeps is an important component in offshore hydrocarbon

    exploration. Seepage can determine if an active petroleum system is present, identify areas with

    high potential and to risk prospects, and provide insight into the character of the oil (Abrams,

    2005). While hydrocarbon seeps are clustered along the edges on the continental shelf and slope,

    seeps can be found far offshore in deeper basins (Cordes et al., 2007; Cordes et al., 2010). High-

    resolution marine geophysical techniques are used to detect seeps by exploiting their acoustically-

    reflective properties. Hydrocarbon seeps and associated features are discrete, hard (carbonate

    production and seep fauna), and surrounded by softer hemipelagic sediments that produce

    characteristic patterns in acoustic reflectivity datasets. Various geophysical, biophysical, and

    morphological signatures associated with active and relic seeps are detected through both optical

    and acoustic remote sensing techniques. Seeps physically modify their depositional environment

    by supporting extensive chemosynthetic communities, precipitating authigenic carbonates, and

    sediment displacement via fluid expulsion. Such features were recognized on seafloor amplitude

    datasets originating from 2D seismic surveys and confirmed by subsequent dives to confirm the

    presence of chemosynthetic communities and seep features (Roberts et al., 2010; Roberts et al.,

    2010). Roberts et al., report analyzing patterns in reflectivity in BOEM seismic datasets, ranking

    areas of increased hardness and reflectivity amplitude, and then confirming with DSV Alvin dives

    in the Northern Gulf of Mexico (GoM) (Roberts et al., 2007; Roberts et al., 2010). Many of these

    areas predicted as potential seep sites using seafloor amplitude data were confirmed1 as areas of

    extensive authigenic carbonate hardgrounds supporting active chemosynthetic communities.

    Several of these initial seep sites are now considered some of the classic seep areas in the GoM

    and have been the focus for numerous studies of their geological and ecological characteristics of

    Lower Continental Shelf (

  • U.S. Hydro 2017

    3

    Remote Sensing of Seep Features

    Fluid expulsion processes at the seafloor are associated with mud volcanoes, pockmarks and

    localized depressions, dense aggregations of chemosynthetic fauna (clam, mussel, and tubeworm

    communities), subsurface faults serving as fluid conduits, gas hydrate deposits, and shallow gas

    accumulations. These distinctive features along with other seep indicators such as surface slicks,

    midwater gas bubbles, and oil droplets are detectable by their distinctive geophysical signatures in

    synthetic aperature radar (SAR) (MacDonald et al., 1996; De Beukelaer et al., 2003), 2D and 3D

    seismic (Roberts et al., 2006; Roberts et al., 2010), sub-bottom profiler (SBP) (Hovland, 2007),

    side-scan sonar (Coleman and Ballard 2001, Sager et al. 2004) and MBES datasets (Orange et al.,

    2002; Orange et al., 2010; Weber et al., 2012).

    Exploration Seep Hunting

    Geochemical analysis of seafloor seep sediments is an effective hydrocarbon exploration tool

    (Abrams, 2005, Orange et al., 2002; Bernard et al., 2008; Orange et al., 2008; Orange et al., 2009;

    Orange et al., 2010; McConnell and Orange, 2014). Seafloor geochemical exploration programs

    are based on the principle that hydrocarbons migrating upwards from deep source rocks and

    reservoirs can be sampled from seafloor and shallow subsurface sediments and analyzed to

    evaluate commercial potential. Though seepage is ephemeral across various time scales (Leifer et

    al., 2004), the geochemical and biological signals persist and can be directly sampled by simple

    analytical tools to determine the geochemical makeup and commercial viability. Seafloor features

    interpreted as hydrocarbon seeps are the primary targets for geochemical exploration programs.

    The association between seafloor seeps and commercial reserves is firmly established the direct

    linkage between the subsurface reservoirs, migration pathways, and seafloor seeps has been

    confirmed in calibration tests (Abrams and Dahdah, 2011). Identifying and sampling sites where

    deep fluids have migrated to the seafloor provides high quality geochemical data for evaluating

    deep hydrocarbon reservoirs.

    MBES Exploration Surveys

    With depressed oil prices, the industry seeks cost-efficient exploration tools and techniques that

    enabled the use of MBES systems to become an integral component of the offshore exploration

    survey workflow. The higher frequencies used in deepwater MBES mapping (12-30 kHz) are able

    detect most of the physical proxies of hydrocarbon seeps including small isolated areas of

    hardgrounds or chemosynthetic shell deposits and midwater bubble plumes that may not be

    detectable with conventional seismic mapping (Brooks et al., 2014). Seep hunting and geochemical

    surveys typically follow 2D reconnaissance surveys and occur before more expensive 3D and high-

    resolution AUV site surveys. Fugro geoscientists use an integrated science-based approach for

    locating, delineating, and sampling deep-water hydrocarbon seeps during MBES exploratory

    surveys2. Bathymetric datasets (~ 15 m gridded cells) allow for detailed identification of fine-scale

    seep-related features mud volcanoes, seafloor faults, salt diapirs, mounds, and depressions in

    water depths exceeding 4,000 m. Co-located multibeam backscatter imagery (5 m gridded cells)

    is used to find authigenic carbonate deposits, chemosynthetic shell clusters on and embedded in

    the sediment, and gassy sediments. Midwater backscatter imagery detects midwater plumes of gas

    2 https://www.fugro.com/our-services/marine-site-characterisation/marine-geotechnical/seep-hunting-and-

    geochemical-campaigns#tabbed1

    https://www.fugro.com/our-services/marine-site-characterisation/marine-geotechnical/seep-hunting-and-geochemical-campaigns#tabbed1https://www.fugro.com/our-services/marine-site-characterisation/marine-geotechnical/seep-hunting-and-geochemical-campaigns#tabbed1

  • U.S. Hydro 2017

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    bubbles and oil droplets (Figure 1). Integrating these MBES-derived datasets allows for

    characterization and ranking of seafloor seeps for coring targets during geochemical surveys (6 m

    piston or gravity cores) to sample sediments for geochemical analysis.

    Figure 1. Seep hunting methodology using multibeam echosounders. Three datasets are derived from multibeam sonar data that

    aid the remote detection of hydrocarbon seeps bathymetry, seafloor and midwater backscatter data.

    MBES Backscatter for Seep Detection

    Hydrocarbon seeps and their geophysical and biophysical proxies are acoustically-reflective

    features (Roberts, 2006). Multibeam backscatter is our primary tool to locate these features on the

    seafloor during exploratory seep surveying. Obtaining high-quality backscatter data is a critical

    component of a seep hunting survey the importance of knowing the accurate delineation and

    extents is required for successful geochemistry surveys. Accurate seep delineation is necessary for

    cost-effective ultra-short baseline (USBL) navigated coring. The geochemical signal found in the

    sediment near seeps has an exponentially-steep lateral chemical gradient (Abrams, 1996; Abrams,

    2005). Missing a coring target on the order of tens of meters may result in a negative geochemical

    result leading to flawed conclusions about the potential of the reservoir (McConnell and Orange,

    2014).

    This steep chemical gradient requires knowing seafloor reflectivity on a pixel-level

    resolution. To aid our interpretations and mitigate the slight differences in imagery between

    existing commercial processing software, we use three separate backscatter processing packages.

    Each of the software packages used for seep surveys convert the backscatter intensity signal

  • U.S. Hydro 2017

    5

    slightly differently, resulting in slightly different seafloor images depending on the algorithm used,

    especially in areas of complex surface relief and abundant specular reflection. Meter-scale seafloor

    backscatter data is used to pinpoint our USBL coring target location. Seafloor seeps are often

    associated with a distinctive, anomalous backscatter fingerprint on MBES data (Johnson et al.,

    2003) and we take a relative and qualitative approach to interpreting multibeam backscatter data.

    Coring has shown that seafloor seeps often appear as anomalous bright red bloodspots (using a

    rainbow palette in ArcGIS where high intensity backscatter = red, low intensity backscatter = blue)

    surrounded by relatively lower backscatter (Figure 2). This classic signature is related to the harder

    and discrete authigenic carbonate deposits and chemosynthetic fauna (active and relic)

    encompassed by softer hemipelagic muds and clay. This fingerprint needs to be analyzed in each

    software package in both 2D and 3D in light of beam geometry, seafloor morphology and various

    shaded relief surfaces with varying artificial sun azimuths and low artificial sun elevations to

    exacerbate noise-related rugosity that may affect interpretation (Orange et al., 2010). We find that

    this signature on a pixel-level scale can change dramatically and we aim to minimize that change

    through a comprehensive understanding of the various survey hardware and software parameters

    in light of beam geometry related to local seafloor slope.

  • U.S. Hydro 2017

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    Figure 2. Seafloor backscatter signatures of hydrocarbon seeps using Caris Geocoder, Fledermaus Geocoder, and Kongsberg

    Poseidon processing software. Note the variations of the anomalously high backscatter areas as a function of software used. This

    example shows a sector intensity imbalance that is muted with angle-varying gain in the Geocoder imagery. The imbalance is

    more severe and can mask features of interest in Poseidon. Panel L shows a sector intensity and a hydrocarbon seep intensity

    that have similar magnitudes. Use of a cleaned reference surface can help alleviate the anomalously low areas of backscatter due

    to local slope angle shown in the Fledermaus Geocoder and Poseidon imagery.

  • U.S. Hydro 2017

    7

    The acoustic response of hydrocarbon seeps is dependent on MBES frequency and can

    challenge interpretive efforts and coring operations. While directly coring areas of anomalously

    high backscatter using USBL-navigated cores may provide confirmation of hydrocarbon fluid

    presence on the seafloor, authigenic carbonate or hardground outcrops can easily bend core

    barrels leading to significantly increased exploration costs (Digby et al. 2016). ROV investigations

    of low frequency (12-30 kHz) seafloor backscatter datasets show that these areas of high

    backscatter can be due to surficial scattering due to exposed carbonate pavement on the seafloor

    or volumetric scattering due to areas of scattered shells or mineralogical fragments embedded in

    sediment saturated with near-surface hydrocarbon-rich fluid favorable for coring. The science of

    seep hunting relies in obtaining a core close enough to the seep that the chemical fingerprints can

    be measured without bending the core barrel on exposed authigenic carbonate (Figure 3). In coring

    operations in deepwater, a single core can take several hours and therefore both the backscatter

    dataset and interpretation of the dataset need to be high quality. Understanding the frequency

    sensitivity of seep features with properly acquired and processed seafloor backscatter can assist

    interpretation on whether surficial or volumetric processes (penetration) predominate. As frontier

    exploration moves into deeper waters in search of oil and gas reserves, studies that examine the

    acoustic frequency responses of seep features in deep water multibeam systems as well as a

    comparison of the processing software and acquisition parameters are critical to understanding the

    limitations of these datasets. To aid interpretation, Fugro employs two survey procedures to fine-

    tune both the quality of our multibeam data and the coring locations an intensity balancing

    normalization procedure prior to a survey and a 2X or 200% oversampling acquisition technique

    to better resolve geologic features in areas of high interest.

    Figure 3. USBL coring operations using multibeam backscatter datasets for targeting thermogenic hydrocarbon seeps. The

    difference between a bent core (upper left) and one filled with hydrocarbon fluids (right) can be meters. Seafloor backscatter

    data needs to be optimal for interpretation and cost-effective exploration.

  • U.S. Hydro 2017

    8

    Backscatter Intensity Normalization

    Collecting high-quality multibeam data starts with proper calibrations of the system. Prior to the

    start of a seep survey, MBES settings and processing parameters are optimized to locate seafloor

    seeps. During calibration of the MBES, we perform two bathymetry patch tests in shallow and

    deepwater in addition to a relative backscatter intensity normalization procedure. Uncalibrated

    backscatter often appears as along-track bands or striping artifacts in the seafloor imagery (Figure

    4). These artifacts are often due to offsets (gain differences) in the acoustic backscatter intensity

    levels between transmit sectors. It is important to normalize these acoustic offsets between sectors

    because they can increase the likelihood of missing seafloor and water column evidence of seeps

    (de Moustier, 2015). This intensity misalignment may result from improper installation or

    incorrect values in the BScorr.txt (backscatter correction) file within Kongsbergs Seafloor

    Information System (SIS). The factory-installed text file stores beam pattern coefficients for each

    transmit sector to compensate for the gain differences and incorrect or missing values in this file

    can create large intensity offsets between sectors that appear as banding artifacts between sectors.

    If these offsets are large enough, the artifacts can conceal features of interest on the seafloor and

    water column. Adjacent along-track pixels having sonar-related gain differences and variations in

    transmit sector intensity levels will degrade the overall quality of data by masking the underlying

    acoustic backscatter characteristics of the terrain leading to missed targets on the seafloor and

    water column. A normalization procedure involving analysis of reflectivity curves of two adjacent

    lines over a flat, featureless area and an iterative, manual modification of the BSCorr.txt file will

    balance the backscatter intensity across sectors so any observable differences in backscatter

    imagery are environmentally-related (i.e. seafloor features or composition) and not system-related.

    (Figure 5). The foundation for this relative backscatter normalization is based on the sea trials of

    the Kongsberg EM302 installed on the R/V Falkor (Beaudoin et al. 2012) and discussed in Orange

    and Kennedy (2015). A thorough background of multibeam backscatter calibration techniques can

    be found in Rice et al. (2015).

    Figure 4. Banding artifacts in seafloor and midwater backscatter datasets caused by artificial differences in intensity between

    sectors. Hydrocarbon seeps have reflective signatures whose anomalous intensity may be masked by the artifact. Both seafloor

    and midwater datasets are affected by intensity imbalances.

  • U.S. Hydro 2017

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    Figure 5. Relative normalization correction. A BSCorr.txt file with incorrect coefficients will create an angular response curve

    that has sector-step offsets across the swath (blue). A relative intensity normalization will normalize these offsets (red) creating a

    consistent seafloor image across the swath on a flat a featureless seafloor.

    Increasing Geologic Resolution with 2X

    Following an exploration survey that maps 100% of the seafloor with typically 10-20% overlap

    between adjacent lines, a 2X or 200% survey is acquired in areas of interest or of suspected

    seepage. By mapping the same area of seafloor with a different beam geometry, noise-related

    artifacts can be suppressed while increasing the signal to noise ratio (SNR) of anomalous

    backscatter areas analogous to seismic stacking techniques. Decreasing the survey line spacing

    with offset lines (typically half the original line spacing) allows for oversampling creating high-

    sounding densities. The overlap between adjacent lines is significant enough that when

    overlapping pixel values are averaged during the mosaic generation, the increased SNR enhances

    the geologic resolvability of reflective seafloor features (Orange et al., 2015, Digby et al., 2016).

    Averaging of pixel dB values is fundamental to 2X. Oversampling helps dampen the effect of

    irregular seafloor geometry, beam position, and signal attenuation (Figure 6). This type of

    acquisition takes advantage of the sweet spot or MBES paradise between 15-60 grazing in

    the beam fan swath (Lucieer et al., 2015, Rice et al., 2015). The grazing angle sector of 30-60 is

    a low slope plateau in the graph of the backscatter strength versus grazing angle. Regions within

    0-10 tend to be dominated by specular reflection and higher intensities shown by the characteristic

    nadir stripe in backscatter mosaics. Far outer beams (> 60) are lower intensity with noise due to

    attenuation and loss of resolution from increased beam footprint size. By decreasing line spacing,

    more of the seafloor can be imaged in the 15-60 zone and will help suppress undesired background

  • U.S. Hydro 2017

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    noise that can result from angular response, seafloor grazing angles, and beam pattern residuals

    (Kluesner et al. 2013). In areas of complex seafloor topography, slope geometry can mask seafloor

    features where more acoustic energy is reflected off surfaces facing the transducer resulting in an

    artificially high return and slopes facing away can result in a lower return. By covering the same

    area of seafloor with 2X acquisition using different angles of insonification and headings these

    image artifacts can be averaged out creating a vastly cleaner, more interpretable image.

  • U.S. Hydro 2017

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    Figure 6. 2X backscatter acquisition technique. By decreasing line spacing and heading, undesired effects from seafloor

    geometry and grazing angle can be suppressed while enhancing naturally high impedance areas on the seafloor.

  • U.S. Hydro 2017

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    Gigante and Otos Seep Surveys

    Fugro is currently involved in two seep surveys covering close to 1,000,000 km2 of seafloor from

    the U.S. Gulf of Mexico to Belize Gigante3 (2015-2016) and Otos4 (2017) industry-funded

    multibeam and geochemical sampling surveys in partnership with TGS and ONE LLC (Figure 7).

    Three dedicated survey vessels, Fugro Brasilis (30 kHz Kongsberg EM302 MBES, 1 x 1), Fugro

    Americas (30 kHz Kongsberg EM302 MBES, 0.5 x 1), and Fugro Gauss (12 kHz EM122 MBES,

    1 x 2) collect high-resolution MBES bathymetry, seafloor backscatter, and midwater backscatter

    identifying potential hydrocarbon seeps. The survey coincides with the denationalization of

    Mexican waters over one of the most prolific hydrocarbon-bearing basins on Earth and the

    geophysical data acquired will be used to identify and characterize seafloor seeps for geochemical

    coring operations. Because of the importance in obtaining high quality backscatter data, significant

    time and effort were invested into developing protocols and standardizing data acquisition and

    processing settings prior to the start of the survey.

    Figure 7. Gigante and Otos Seep Surveys. Prior to the start of the Gigante survey, a seep calibration study was carried out over

    Green Canyon Block 600 to optimize the EM302 for deepwater seep detection.

    3 https://www.fugro.com/media-centre/fugro-world/article/worlds-largest-offshore-seep-hunting-survey

    4 http://www.tgs.com/News/2017/TGS_announces_new_Multibeam_project_in_U_S__Gulf_of_Mexico/

    https://www.fugro.com/media-centre/fugro-world/article/worlds-largest-offshore-seep-hunting-surveyhttp://www.tgs.com/News/2017/TGS_announces_new_Multibeam_project_in_U_S__Gulf_of_Mexico/

  • U.S. Hydro 2017

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    During sea trials of the newly-installed EM302 MBES on Fugro Americas, significant

    along-track bands visible as artificial striping artifacts were observed in the seafloor backscatter

    imagery. This striping artifact was caused by large (3-5 dB) offsets in intensity level between the

    transmit sectors within Medium, Deep, and Very Deep Modes in the Kongsberg Seafloor

    Information (SIS) real-time acquisition software (de Moustier, 2015). The sea trial analysis

    concluded that these 3-5 dB differences across sectors led to the banding artifacts because the

    BSCorr.txt file was not properly applied during sonar installation and required adjustment to

    compensate for the intensity offsets. A small diagnostic survey acquired data for Kongsberg and

    was processed with Angle-Varying Gain (AVG), a post-processing function that corrects for the

    change in backscatter strength as a function of angle-of-insonification. The results of the small

    survey showed that the striping was indeed lessened by AVG but it also tended to smear

    backscatter anomalies both along-track and across-track in Fledermaus Geocoder (FMGT) and in

    some cases completely erase them using Caris Geocoder. A full backscatter intensity normalization

    was planned to correct the sector imbalance before the Fugro Americas involvement in the Gigante

    seep survey. The probability of missing seep-related features on the scale of a few tens of meters

    would increase without normalizing these gain differences across the sectors in each of the depth

    modes.

    Study GC600 Seep Calibration Site

    During the backscatter normalization procedure, we conducted a pair of small seep detection

    surveys in September 2015 in approximately 1,250 m of water over Green Canyon (GC) Block

    600 in the Gulf of Mexico (Figure 7 inset map). Seep exploration surveys differ from traditional

    hydrographic surveys and nuances in survey parameters can dramatically impact the detectability

    of hydrocarbon seeps and related seafloor features and we wanted to fine-tune the system for seep

    detection before mapping in a largely unexplored offshore frontier basin. GC600 is an ideal site

    for the detection diagnostic survey because it is well-studied, close to the survey area, and actively

    emitting hydrocarbon fluids into the overlying water column (Roberts et al., 2007; Roberts et al.,

    2010; Brooks et al., 2014; Wang et al., 2014; Johansen et al., 2017). The availability of multiple

    sources of multibeam data (12 200 kHz) and seafloor imagery allowed us to analyze the

    frequency response of seeps over a range of frequencies and to evaluate penetration characteristics.

    Using an autonomous underwater vehicle (AUV) MBES dataset (Eagle Ray EM2000, 200 kHz

    at 50 m altitude) acquired from Ecosystem Impact of Oil and Gas Inputs to the Gulf (ECOGIG)

    consortium, and supplemented with near-seafloor imagery from the Mola Mola AUV (3 m

    altitude) as control (Conti et al., 2016), we assess the results of the intensity normalization, test

    various acquisition settings and software packages to optimize the EM302 MBES specifically for

    seep detection, and evaluate off-nadir plume detection limits.

    Geologic Setting of GC600

    The study area is located within Green Canyon Block 600 (27.370 N, 90.569 W), a 3 x 3 mile

    BOEM-designated lease area found along the lower continental slope (> 1,000 m) of the Northern

    Gulf of Mexico (Figure 8). GC600 is situated in a region of intensive natural hydrocarbon seepage

    among an area of complex salt-controlled topographical features. Salt tectonics in the area has

    created a network of subsurface faulting and fissures that promote hydrocarbon fluid and gas

    expulsion from the deep subsurface to the seafloor (Garcia-Pineda et al., 2010). Buoyant and

    mobile salt generates irregular geomorphic features such as domes, ridges, and knolls on the

  • U.S. Hydro 2017

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    seafloor from extensive subsurface faulting. Subsurface faulting promotes the vertical migration

    of hydrocarbons to the seafloor and is consumed by microbial consumption of methane that

    develop carbonate deposits through the anaerobic oxidation of methane (AOM). Seafloor seepage

    sustains chemosynthetic communities composed primarily of tubeworms, mussels, and microbial

    mats that flourish in response to the upwelling methane at this site (Roberts et al., 2010; Fisher et

    al., 2007).

    The geologically and biologically-complex seafloor was one of the first confirmed

    chemosynthetic sites in the Gulf of Mexico found at these depths. The site was initially tagged for

    exploration based on seismic amplitude and reflectivity analysis (Roberts et al., 2007). Subsequent

    dives on the DSV Alvin in 2006 (Dives 4174 and 4184) and by the ROV Jason in 2007. The main

    seepage site is located along an elongate low-relief ridge trending NW-SE in 1,180-1,250 m depth

    that separates two intraslope basins. The site features slabs, blocks, rubble, and hardground

    pavement of authigenic carbonate created by subsurface AOM. Sparse aggregations of

    chemosynthetic fauna such as mussels and tubeworms are located in the cracks of these porous

    carbonate outcrops (Roberts et al., 2010). Geochemical analysis of these carbonate slabs show

    traces of embedded biodegradable crude oil (Brooks et al., 2014). White and orange bacterial mats

    are observed with interspersed dead clam and mussel shells. Numerous active seafloor vents are

    found focused along cracks in the ridge line giving rise to such prolific plume emission sites as

    Birthday Candles and Mega Plume emitting gas and oil-coated bubbles (Wang et al., 2016;

    Johansen et al., 2017). Evidence of the persistent seepage of oily bubbles reaching the surface over

    GC600 are suggested to be relatively constant flux emissions over a decadal time scale based on

    satellite imagery of sea slicks above the study area (Brooks et al., 2014).

    Figure 8. Perspective view of GC600. Inset view shows a perspective multi-scale visualization of GC600 with mapped water

    column plumes acquired from the EM302 overlain on AUV acquired EM2000 MBES backscatter imagery.

  • U.S. Hydro 2017

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    Methods The Fugro Americas is a multi-purpose geophysical and seafloor mapping vessel outfitted with a

    hull-mounted, gondola-lowered 30 kHz Kongsberg EM302 MBES with 432 beams (0.5 fore-aft

    transmit beam width x 1 receive beam width) capable of dual-pinging in medium and deep modes

    for 864 soundings/ping. Results from the sea trials revealed a significant intensity imbalance across

    sectors in Medium, Deep and Very Deep Modes requiring normalization. To assess the results of

    the normalization and evaluate how an imbalanced MBES would ultimately affect seep detection

    and target identification, an initial survey was carried out over GC600 to provide baseline

    backscatter imagery. After the backscatter intensity normalization, the second survey at GC600

    assessed the results of the sector balancing in deep and very deep mode using a high-resolution

    AUV MBES dataset acquired from ECOGIG as control on the backscatter signature/pattern. Line

    spacing geometry was designed to allow for massive oversampling of soundings with significant

    overlap that allowed us to examine our 2X technique that we use to improve the quality of the

    backscatter and increase the geologic resolvability to account for nadir and slope artifacts.

    Processing settings within each software were examined to evaluate how varying each would affect

    the backscatter signature over the seep, i.e. cleaning the dataset prior to backscatter processing,

    using a reference surface to account for changes in slope geometry, use of time series vs. beam

    average, use of AVG with varying window sizes, among other settings. These backscatter analyses

    are supplemented with georeferenced seafloor imagery to ground-truth and assess the observed

    acoustic reflectivity patterns. The line geometry allowed for us to map the known plume emission

    sites at various take-off angles to test the far-nadir limits of detectability of plumes before using

    the EM302 for exploratory surveying of the Southern Gulf of Mexico and Caribbean Basins.

    The first survey of GC600 was designed with a line spacing of 950 m and with an obtained

    swath width of 4,500 m, provided 80% overlap between adjacent lines (Figure 9). Seafloor

    backscatter was processed in Caris Geocoder, Fledermaus Geocoder (FMGT), and Kongsberg

    Poseidon software, gridded at 5 m, and imported into ArcGIS for analysis. Plumes were extracted

    from midwater backscatter data using Fledermaus Midwater (FMMW) software using the

    automated Feature Detector toolkit (Gee et al., 2014).

    Figure 9. Line plan for the pre- and post-calibration survey at GC600. 3X coverage was acquired directly over the NW-SE

    trending plume ridge. Mapped plume emission sites from the first survey allowed for specific take-off angle detectability to be

    analyzed.

    The backscatter normalization of the EM302 is intended to balance the reflectivity intensity

    across sectors, pings, swaths, and modes. Through a manual and iterative process, the method

    adjusts the beam pattern coefficients embedded in the BSCorr.txt file to normalize intensity values

    over sectors. Prior to the start of the normalization, a copy of the existing BSCorr.txt was

    downloaded from the Kongsberg Power Unit (PU) and an expendable bathythermograph (XBT)

    and sound velocimeter (XSV) were acquired at the site. Accurate salinity (mean value representing

  • U.S. Hydro 2017

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    the water column) is critical for the calculation of the absorption coefficient which is necessary for

    determining backscatter intensity. The absorption profile is used to estimate transmission loss in

    the water column. Two reciprocal lines over a flat, uniform seafloor approximately 2,000 m deep,

    appropriate for both Deep and Very Deep Modes of the EM302, were run at 6 kts using the SIS

    acquisition settings intended for the seep survey. A line heading of 0/180 was perpendicular to

    slope to avoid potential across-track intensity changes. Select direction of line to limit impact of

    motion on vessel (pitch, roll, and heading). The length of the line included several thousand pings,

    large enough to provide a robust statistical analysis of the reflectivity dataset (Augustin and Lurton,

    2005). The Angular Response Curve (ARC) was extracted using all pings from these raw

    Kongsberg. all files and analyzed to determine the residual intensity offset values for each sector

    in both Deep and Very Deep Modes. Using Excel, the Median Reflectivity (dB) vs. Transmit Angle

    () is plotted and corrections for each swath (fore and aft) are obtained by holding mid-swath

    sectors constant and adjusting offset adjacent ones until seamless. The sector dB offsets were

    added to the corresponding sector values in the BSCorr.txt file. After this file was modified and

    uploaded back into SIS, the process was repeated using the reciprocal line for QC and a validation

    line was acquired to confirm to absence of the banding artifact. Figure 10 shows a flow chart of

    the steps involved in the normalization process.

    Figure 10. Flow chart of the backscatter normalization process. Adopted from Orange and Kennedy (2015)..

    Following the backscatter normalization, a second survey was carried out over GC600 to

    evaluate the results, the value of 2X in improving the geologic resolvability when comparing the

  • U.S. Hydro 2017

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    data to the 1 m gridded AUV backscatter dataset, and assess near-seafloor plume detectability in

    the outer beams. The line plan was slightly offset from the original lines in the pre-calibration

    survey (Figure 9) and were acquired in both Deep and Very Deep Modes. The overlap between

    adjacent lines provided 3X coverage over the main ridge containing the plume emission sites. The

    seafloor backscatter data was gridded at 5 m, 2.5 m, and 1 m and the improvement in resolution

    was analyzed relative to the 1 m ECOGIG AUV dataset. To test water column detection limits of

    the EM302, plume emission sites along the ridge were imaged at 10-12, 32-34, and 45 take-off

    angles. Water column data were processed using Feature Detection in FMMW with normalization,

    threshold, and despeckle filters. A cluster analysis was performed to enhance the midwater

    backscatter signal of the plumes and improve interpretation of emission sites (Gee et al., 2014).

    Backscatter acquisition parameters and processing software settings were analyzed in order

    to optimize the MBES for detecting and delineating seafloor seeps during the GC600 surveys. Best

    practices for commercial seep hunting dictate that acquisition settings and processing procedure

    remain constant throughout the survey to ensure a consistent product (Rice et al., 2015). We

    developed a best practices acquisition guideline for seep detection using the EM302 that we used

    for the Gigante and Otos seep surveys:

    To maximize ping rate and sounding density dual-pinging Deep Mode on the EM302 is entirely used throughout the survey in 500 3,000 m water depth to ensure high-density

    along-track data density and faster survey speeds. Step changes in acoustic backscatter

    intensity of up to 5 dB may be observed when changing depth mode leading to patchwork

    quality backscatter mosaics.

    A fixed FM-enabled dual-swath mode is preferable for backscatter data density in deep waters (3,000 m +) using Deep Mode.

    Sector coverage settings in the SIS Runtime parameters use an Auto angular coverage mode for improved bottom detection with high density equidistant beam spacing and a max

    swath width of 68/68.

    Pitch and yaw stabilization are turned on with a head tilt of 1 to 3 to mitigate/prevent Eriks Horns.

    In the Filter and Gains tab, the penetration filter and sector tracking are off. Using a tilted head, a penetration filter will create a false bottom detection that creates a very low

    backscatter signature dubbed Bobs Blobs. Sector tracking normalizes the backscatter

    intensity across the swath in real-time during acquisition but does not record the process

    and irreversibly alters the file.

    We developed a best practices processing guideline for seep detection using the EM302 that we

    used for the Gigante and Otos seep surveys:

    Daily sound velocity profiles and salinity measurements are performed using CTD, XBT, and XSV casts and independently calculated on a QC spreadsheet. This check alleviates

    potential poor-quality data resulting from bad profiles before they are added into SIS.

    Bathymetry editing is light to avoid over-smoothing of data to aid interpretation of fine-scale features (Orange et al., 2010). Hillshaded relief is created with azimuths of 45, 135,

    225, 315 with a low artificial sun grazing angle to highlight fine-scale features.

    Use of three backscatter processing software packages assists with interpretation.

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    Individual settings for each of the three packages used:

    Caris Geocoder v. 9

    Geocoder processing algorithm

    Time series with anti-aliasing

    Auto Gain Correction

    Auto TVG

    AVG Adaptive 300

    Avoid despeckle this functionality averages anomalous backscatter data with surrounding cells

    Use a cleaned reference surface

    Full blend gridding method

    Fledermaus Geocoder v. 7.5

    Tx/Rx Power Gain Correction

    AVG Adaptive 300

    Use a cleaned reference surface

    Poseidon v. 2.4

    2D interpolating filter of 9

    Footprint size of 50%

    Seafloor backscatter data are processed by line (-5 to -65 dB intensity range, red = high reflectivity,

    blue = low reflectivity) and imported into ArcGIS with a custom model builder script. Mosaics are

    generated using the mean functionality in Image Analysis. Analysis of various processing settings

    in each software was performed using remotely-acquired data from GC600 and ECOGIG AUV

    backscatter imagery to compare settings and software packages. The high-resolution Eagle Ray

    AUV 1 m backscatter imagery was used a gold standard to compare the software processing

    analyses to ignoring fine-scale differences due to frequency and penetration differences between

    the 200 kHz and 30 kHz MBES.

    Results and Discussion

    Backscatter Intensity Normalization

    Intensity imbalances were observed between swaths (aft and fore in dual-pinging Deep Mode),

    sectors, and modes and the BSCorr was manually modified to normalize these differences. The

    normalization was performed on a flat seafloor devoid of any naturally-occurring features to

    eliminate potential errors in both Deep and Very Deep Modes. Deep mode dual-swath has eight

    transmit sectors (central four transmit sectors are continuous wave (CW) with the outer two sectors

    powered by linearly frequency modulated (LFM) pulses) each with a different acoustic frequency

    for both fore and aft swaths. Each of the sectors has an individual beam pattern coefficient that

    normalizes backscatter intensity offsets across sectors, swaths, and modes contained in the factory-

    installed BSCorr.txt file. Very Deep Mode operates in the same manner but with six sectors

    operating in LFM pulses.

    The magnitude of the banding artifacts was similar to many of the anomalous backscatter

    anomalies that will mask potential hydrocarbon seeps (Figure 11). An observed sector imbalance

    of up to 3 dB was observed across sectors in Deep Mode and banding is especially pronounced

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    along the port side sectors. The port side is generally lower intensity that exhibited discrete bands

    of higher intensity. The starboard side appeared to have higher overall intensity across a flat a

    featureless seafloor. Within Deep Mode, there are visible > 1 dB differences between fore and aft

    swaths leading to a pixelated along-track banding pattern. A significant visible difference between

    modes is observed in the data with up to a 5 dB variation between Deep and Very Deep Mode

    (Figure 11).

    Figure 11. Unnormalized seafloor backscatter with strong sector banding (adopted from Orange and Kennedy, 2015). SIS

    display Deep vs Very deep (Line_0000) showing a large step change (> 5dB difference) when changing modes and > 1 dB

    differences in intensity between fore and aft swaths.

    Figures 12 show the results of the normalization using angular response curves (ARC).

    Line_0000 was collected with a heading of 0 at 6 kts over the selected area. The fore and aft

    swaths were balanced using Line_0000. Figure 12A shows the ARC generated from the pings

    along this line. Swath 1 uncorrected aft is shown in blue and swath 2 uncorrected fore is in green.

    The apparent tilt shown in the port sectors is contributing to the relatively lower backscatter

    intensity compared to the starboard side (refer to Figure 11). During the normalization procedure,

    a -1 dB adjustment was applied to the fore swath to normalize the fore to the aft swaths.

    Line_0001 was collected at a 180 heading back over Line_0000 evaluated the ARC in

    Very Deep Mode. Figure 12B shows the normalization of Very Deep Mode where blue is the

    uncorrected and the 1st iteration of the corrected ARC is shown, by sector, in alternating red and

    green for differentiation. The corrections for each sector are located in the table on the graph. After

    normalizing between sectors and fore and aft swaths in Deep Mode during Line_0000, and across

    sectors in Very Deep Mode during the reciprocal Line_0001, a normalization across modes was

    performed. This is a relative normalization and Very Deep was chosen as the standard ARC

    requiring a bulk shift of -5.25 dB applied to the swath-balanced Deep Mode (Figure 12C). Figures

    12D and 12E show the results of the shift per swath where 12D shows the corrected aft (swath 1)

    with the corrected Very Deep and 12E shows the corrected fore (swath 2) with the corrected Very

    Deep Mode.

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    Figure 12. Angular response curves (ARC) for the normalization.

    Figure 13 shows the results of the pre- and post-calibration lines run over GC600. Initial

    efforts into reducing the sector banding using AVG was discussed prior to the normalization. This

    survey is regional-scale and there was concern after analyzing AVG that this would not only

    potentially wipe out small seep anomalies, but also affect the aesthetic quality of the final mosaics.

    AVG corrects for the change in backscatter strength as a function of angle-of-insonification. The

    AVG algorithm in Geocoder computes an average signal level over a specific range of grazing

    angles and fits a curve to the average across-track variation. The user specifies the number of pings

    along track to average over. The larger the number of pings specified, the more the imagery is

    potentially smeared along-track. The first column of Figure 13 shows the pre-calibration Line 001

    processed with Caris Geocoder (Adaptive AVG 300), FMGT (Adaptive AVG 300), and Poseidon.

    Poseidon does not have AVG functionality. In the Caris Geocoder example, the portside banding

    is eliminated but with a reduced intensity signal over the NW-SE trending seep ridge. The AVG

    algorithm used in Caris Geocoder eliminates the sector intensity differences but also much of the

    anomalous high backscatter signal on the hardgrounds along ridge. Cariss AVG algorithm

    diminishes the areal extent and strength of the high backscatter feature both along- and across-

    track. The ECOGIG Eagle Ray AUV 1 m backscatter data is shown for control. In the FMGT

    example for the pre-calibrated line, use of AVG removes almost all of the across-track step changes

    in acoustic intensity but smears pixel clusters of anomalously high backscatter along-track. Sector

    banding is severe in Poseidon and without a normalization this dataset would be difficult to

    interpret.

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    Column 2 shows the equivalent calibrated line (same azimuth Line 147) using AVG

    (Adaptive 300) in Caris Geocoder and FMGT. It appears AVG has adequately suppressed the

    sector imbalance in the Geocoder examples (Line 001 vs. Line 147), at least on a localized scale.

    Slight differences can be seen along the seep ridge line where higher intensities exist in the post-

    calibrated lines. This clearer delineation of the hardground and seep-influenced seafloor is the

    objective of balancing the sectors before a seep survey. The sector balancing normalization results

    are most apparent in the Poseidon example. The iterative balancing alleviated the strong port side

    sector and normalized the overall intensities across the entire swath (recall that the port side had

    the more severe high banding surrounded by overall lower intensities while the starboard side was

    generally higher). A strong nadir strip is apparent in the Poseidon calibrated backscatter image.

    This region of intense specular reflection is dampened by use of AVG in FMGT and Caris

    Geocoder.

    Column 3 shows FMGT and Caris Geocoder without the use of AVG in pre- and post-

    calibration lines. Both of Line 001 and 147 are dominated by the nadir strip. In the pre-calibration

    lines, this strip in addition to the banding, creates almost a useless product for interpretation.

    Normalizing balances the sectors, but AVG is clearly needed to suppress the nadir strip during

    post-processing. Column 4 shows the effect of the sector balancing without the use of AVG. While

    the sector banding artifact is reduced the pronounced nadir stripe has an intensity magnitude equal

    to the seep feature leading to potential missed targets. The images indicate that a backscatter

    normalization performed in acquisition with the use of AVG in processing is optimal for

    identification of anomalous backscatter areas. Note that unbalanced backscatter affects water

    column interpretability. Severe sector misalignment is observed in the water column data that

    would likely lead to missed bubble cluster reflectors in the dataset. In addition, automated plume

    extraction tools require a clean dataset and a sharp contrast between reflector and background

    intensity.

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    Figure 13. Results from the surveys over GC600 show pre- and post-calibration results.

    2X Seafloor Backscatter Acquisition

    Both surveys over GC600 showed prolific plumes in the water column regardless of the intensity

    normalization. During an exploratory survey, the presence of plumes in the water column would

    signify active seepage in the area and therefore focus our seafloor interpretations near the suspected

    emission site. Interpreted plumes in the water column will validate areas of anomalously high

    seafloor backscatter as seep-related features. While there is plume positional uncertainty involved

    in addition to the highly ephemeral nature of plume emission sites, we will begin to analyze the

    seafloor backscatter patterns near the emission site. At a site like GC600, a 2X survey would be

    run over the site to sharpen the high backscatter anomalies and clean up the dataset. While time

    consuming and therefore expensive to run additional lines, geoscientists need to balance well-

    placed cores with the cost of coring operations. During exploratory surveys with a hull-mounted

    system, we would not know if this high acoustic return was due to exposed carbonate pavement or

    scattered shells in hydrocarbon-soaked sediment ideal for coring. 2X would allow for a cleaner

    delineation of the anomalys extent for interpretation of the seep. After a 2X survey, the decision

    to core directly into the high backscatter anomaly versus taking a more conservative and cautious

    approach by coring on the peripheral of the anomaly is as much philosophy, experience, and

    science. Interpreting if the backscatter anomaly is related to hardness of the seafloor, roughness of

    the seafloor, volumetric scattering, acquisition and seafloor slope geometry needs to be analyzed

    with other datasets to mitigate the risk of a bent core barrel (Orange et al., 2010).

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    Figure 14. Poseidon post-calibration seafloor backscatter showing 1X, 2X, and 3X.

    Figure 14 shows a post-calibrated line processed with Poseidon. The benefits of oversampling

    are clearly shown between the 1X-2X-3X coverage. The central 2X imagery suppresses the

    artificially-elevated nadir strip while 3X helps define both the seep delineation and lessens the

    noisy specular reflection. Of the three processing packages used during the seep surveys, only

    Poseidon offers a pixel averaging functionality during mosaic generation within the software

    package. Averaging the pixel values of overlapping cells is the fundamental principal behind 2X.

    Averaging pixel values can suppress random noise and enhance the signal of an area of anomalous

    backscatter. Caris HIPS and FMGT do not have this averaging functionality so each line will be

    processed individually and then averaged in the mosaic with ArcGIS Image Analysis.

    Figure 15 shows the results evaluating if geologic resolution increases with oversampling and

    a decrease in cell grid size. Seafloor backscatter imagery is typically gridded at 5 m regardless of

    water depth during our seep surveys. In 1,250 m water depth, would 2-3X coverage allow for the

    imagery to be gridded at a higher resolution? On the top row Panel A, is the 5 m gridded 3X. Panel

    B is gridded at 2.5 m, Panel C at 1 m, and Panel D is the Eagle Ray AUV 1 m dataset for

    comparison. There are slight differences between the 5 m to 1 m grids with increasing amounts of

    speckle apparent along the highly reflective plume ridge. Better delineation is negligible when

    compared to the 200 kHz AUV dataset. Keep in mind that the AUV data is high frequency and is

    likely mapping the upper few cm of sediment while the 30 kHz at an altitude of 1,250 m is

    penetrating > 1 m. The center row (Panels E to H) shows the differences in Poseidon from 1X

    coverage to 3X coverage compared to the AUV data. Progressively clearer delineation is noted

    from 1X to 3X coverage highlighting the effectiveness of increasing geologic resolution of the

    seep features. The bottom row (Panels I to L) shows the differences in processing packages for 3X

    acquisition. Panel I is Caris Geocoder showing the muted reflective response along the seep ridge

    and Panel J shows the FMGT 3X imagery product. Both of these Geocoder products used Adaptive

    AVG with a window size of 300. Poseidon 3X is shown in Panel K and has an overall consistent

    background reflectivity across the swath.

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    Figure 15. Analysis of gridding resolution (top row), 1X-3X coverage (middle row), and processing software (bottom row).

    Detection Limits of Midwater Plume Mapping

    During the first survey over GC600, plume emission sites were mapped in FMMW and the second

    survey was designed to run over the emission sites at various take-off angles. The objective of the

    test was to evaluate the detectability of plumes in the far outer beams. Previous work by Weber et

    al. (2012) consistently detected seeps with an EM302 over a swath width that was roughly twice

    the water depth. Figure 16 shows the survey design in plan view with the near seafloor pick

    representing the plume emissions sites. Below is a table containing values estimating the far off-

    nadir limits. Take-off angles in excess of 50 were plumes imaged occurred in three lines

    coinciding the estimation made by Weber et al. (2012). While reverberation masked many of the

    far off-nadir seeps making it difficult to extract using threshold filtering and other automated

    procedures, these plumes are visible and can be mapped by manual interpretive geopicking. Note

    that most of these far off-nadir plumes are not visible in FMMW stacked view. The data file must

    be viewed in beam fan view to see these plumes. This small diagnostic test provided information

    that was latter used to plan line spacing ion unexplored frontier areas in the Southern Gulf of

    Mexico.

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    Figure 16. Analysis of EM302 midwater detection limits.

    Conclusion Prior to commencing the Gigante multibeam seep survey, Fugro performed a seep calibration over

    GC600 using a newly-installed Kongsberg EM302 multibeam. The multibeam system had a faulty

    factory-installed BSCorr.txt and required a backscatter intensity normalization to balance the

    acoustic intensity across pings, swaths, and modes. The EM302 collected lines over GC600 before

    the normalization and after to assess the magnitude of potential interference caused by the banding

    artifact over a well-studied hydrocarbon seep. In addition to the intensity normalization, the

    effectiveness of 2X oversampling and off-nadir midwater plume detection limits were evaluated.

    The study found that the backscatter normalization was effective in eliminating the banding

    artifacts. The intensity magnitude of the striping artifacts in many areas were as elevated as

    backscatter anomalies interpreted to be seep-related hard hardgrounds. Uncalibrated backscatter

    will affect intensity in both seafloor and midwater imagery, two datasets primarily used for seep

    detection and characterization. Seeps are acoustically-reflective features and will be potentially

    overlooked if normalization is not performed prior to a large survey such as Gigante and Otos. The

    use of AVG in post-processing suppressed specular reflection in the nadir strip, another source of

    interference in the imagery datasets. The study indicates that issues related to data quality (such as

    a bad BSCorr.txt file) should be corrected in acquisition and not relied on in the post-processing

    pipeline, a suggestion made in the Lurton and Lamarche report (2015). AVG functionality helps

    but will potentially wipe-out or lessen many of the small characteristic high backscatter anomalies

    that the seep survey is seeking for coring targets.

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    Backscatter normalization should be performed when a multibeam is installed to fine-tune

    the BSCorr.txt values, when along-track banding is noticed, and after transducer maintenance and

    cleaning. Time-varying drift of backscatter intensity has been observed during long periods of ship

    operations because of biofouling on the transducer.

    2X acquisition is a simple technique used to enhance the SNR in multibeam reflectivity

    data. It minimizes artificial acoustic returns that result from topographically-varied areas,

    suppresses noise resulting from specular reflection due to angle of insonification, and will enhance

    or saturate areas that are hard on the seafloor aiding seep detection. This technique enhances

    delineation of hydrocarbon seeps that will assist USBL-navigated coring and ultimately providing

    a greater success of obtaining a full core of sediment saturated with seep fluids. Figure 17 shows

    a perspective view of the high-resolution ECOGIG AUV dataset (1 m) with plume locations and

    a 5 mm orthomosaic of seafloor imagery acquired from the ECOGIG Mola Mola AUV at an

    altitude of 3 m above the seafloor. A 3D perspective of a Poseidon 3X imagery product is shown

    to compare the resolution of a hull-mounted EM302 with near-seafloor datasets. By using 2X+

    acquisition coverage with a MBES optimized for seep detection, remotely-acquired seafloor

    imagery data quality can be improved leading to better interpretation of resolvability of features.

    Figure 17. 3D perspective of GC600 showing ECOGIG's AUV data with Poseidon 3X seafloor imagery. Through optimization of

    acquisition and processing settings, a comprehensive backscatter intensity normalization, and 2X oversampling, remote seafloor

    backscatter imagery can be vastly improved.

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