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(M35) Arctic Petroleum Geology Y. Kristoffersen 45

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Chapter 45 Geophysical exploration of the Arctic Ocean: the physical environment, survey techniques and brief summary of knowledge YNGVE KRISTOFFERSEN Department of Earth Science, University of Bergen, Alle´gaten 41, N-5007 Bergen, Norway (e-mail: [email protected]) Abstract: The areal extent of the ice covered Arctic Ocean is about four times the size of the Mediterranean Sea. More than 50 years after identification of the main bathymetric features in the deep polar basin, our coverage of modern multichannel seismic data is still limited to what a single ship would complete under open-ocean conditions in about two and a half months. In addition, an estimated one-fifth of the deepwater area is inaccessible to icebreaker surveys with surface-towed equipment. Signal-to-noise levels achieved in multichannel seismic data acquisition from icebreakers are sufficient to identify acoustic basement below more than 3 s (two-way travel time) of sediments in spite of reduced source and receiver arrays. Our current reconnaissance stage in deep basin exploration will at least include the coming decade as surveys by diesel-driven icebreakers are largely restricted by contemporary patterns of open leads in the sea ice cover.

The large water depths encountered during the drift of Fram (1893 –1896) came as a surprise to Nansen, who had brought 200 m of bronze wire, 1200 m of single-cord steel line and 1900 m of hemp line to measure ocean depth. The drift track from the Laptev Sea Shelf to the Yermak Plateau passed over the abyssal plains of the Nansen Basin (Fig. 45.1), and led him to conclude that the North Polar Basin was one large basin (Nansen 1904). Harris (1904), who had studied tides on the north coast of Alaska, observed that the tidal wave arrived from the west and was delayed in comparison to the expected arrival of a wave travelling from the North Atlantic across a uniformly deep polar basin. The delay required a bathymetric obstruction in the form of ‘a tract of land, an archipelago or an area of shallow water’. Fifty years later, Worthington (1953) noticed that the deep water in the Canada Basin was 0.5 8C warmer than Nansen’s observations and postulated a barrier reaching 2000 m water depth. The obstruction turned out to be the submarine Lomonosov Ridge, which divides the Arctic Ocean into two large sub-basins; the Amerasia Basin north of Alaska and Siberia and the Eurasia Basin bordering the European polar margin (Fig. 45.1). The ridge rises about 3000 m above the flanking abyssal plains to a water depth as shallow as 500 m, but generally 1000 –1200 m. Lomonosov Ridge was first discovered in 1948 by Soviet ‘High Latitude Air Expeditions’ followed by more systematic mapping in the subsequent years (Ostrekin 1954). Chukchi Cap was discovered in 1950 by the Soviet ice drift station NP-2 (Hunkins et al. 1962), and Alpha Ridge in 1954 by US ice drift station T-3 (Crary 1954). Publication of the first bathymetric map of the Arctic Ocean by the Soviet Union in 1954 showed a detail which profoundly surprised Western scientist and testified to the magnitude of the postwar Soviet effort (Weber 1983). With the information gathered by the time of the International Geophysical Year 1957/1958, all major submarine features of the polar basin had been identified. Historical and modern datasets comprising soundings from Canadian, Russian and US ice stations, US and British nuclear submarine cruises (1958 –1988), echo soundings from the SCICEX-programme 1993–1999, and data from cruises of icebreakers and research vessels of Canada, Germany, Norway, Russia, Sweden and the United States have now been compiled into a new International Bathymetric Chart of the Arctic Ocean (Jakobsson et al. 2008). The data is available at: http://www. ngdc.noaa.gov/mgg/bathymetry/arctic/ibcaoversion2.html.

Arctic Ocean: the physical environment Sea ice A sea ice cover in the Arctic Ocean is maintained by a strong and stable vertical stratification in the upper 200 m of the ocean, which supresses heat transfer from the warm Atlantic Layer below. Also, the high surface albedo of snow-covered ice (snow c. 0.8 v. ,0.1 for water) limits absorption of heat from incoming radiation and further contributes to a low-energy state. The extent of the sea ice cover varies with the annual cycle by a factor of 2, with a maximum in March and minimum in September, and there is evidence for a long-term decrease of about 6% per decade in areal extent (Johannessen et al. 1999) as well as a decrease in ice thickness (Rothrock & Maykut 1999). Q1 Ice drift. Sea ice drift in the Arctic Ocean is wind-driven with

a first-order pattern expressed by an anticyclonic Beaufort Gyre and the Transpolar Drift forced by a mean high sea-level pressure over the Arctic Ocean. Variations in the forcing on time scales from weeks to a decade are revealed by multivariate analysis of sea-level pressure which transforms the data into uncorrelated orthogonal components. The first principal component which accounts for most of the variability (59%) is called the Arctic Oscillation (Thompson & Wallace 1998). A second principal component (13% of total variance) defined for the winter season has a strong meridional component in the wind and is important for sea ice export (Watanabe & Hasumi 2005). In a negative phase of the Arctic Oscillation (AO), high air pressure at sea-level enhances anticyclonic circulation, the Beaufort Gyre becomes wider (Fig. 45.2a), and an intensified Transpolar Drift removes younger ice faster from the Eastern Siberia and the Laptev Sea margin (Proshutinsky & Johnson 1997; Rigor et al. 2002). During the positive phase, circulation in the Beaufort Gyre is reduced and its centre moved towards Alaska at the expense of a wider Transpolar Drift (Fig. 45.2b). On average, it takes more than 6 years to drift from the Beaufort Sea to the Fram Strait. It takes one year longer during positive AO phases, but ice travels faster from the North Pole to the Fram Strait and induces divergence and production of more thin sea ice over the Eurasia Basin (Rigor et al. 2002).

From: Spencer, A. M., Embry, A. F., Gautier, D. L., Stoupakova, A. V. & Sørensen, K. (eds) Arctic Petroleum Geology. Geological Society, London, Memoirs, 35, 685– 702. 0435-4052/11/$15.00 # The Geological Society of London 2011. DOI: 10.1144/M35.45

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500 km Fig. 45.1. Bathymetry of the Arctic Ocean from http://www.ngdc.noaa.gov/mgg/bathymetry/arctic/ibcaoversion2.html with present coverage of published multichannel seismic lines across the surrounding continental margins. Drilling location of Arctic Coring Expedition (ACEX) on Lomonosov Ridge and IODP Sites 910– 12 north of Svalbard indicated by white dots. Locations of seismic sections shown in Figure 45.14 by heavy red lines.

Ice thickness. Model results suggest that undeformed sea ice may

thermodynamically become over 1 m thick during the first year, ,2 m thick after the second year and reach a limit of about 3 m (Maykut & Untersteiner 1971; Vancoppenolle et al. 2006). Sensitivity studies show that the ice thickness is most sensitive to changes in heat flux from the ocean and the insulating effect from incoming radiation if the snow cover is more than 80 cm (Untersteiner 1990). Further increase in thickness is from mechanical thrusting and ridging in convergent zones, most often involving thrusting of younger and thinner ice as refrozen leads close. The sea ice cover is made up of a mosaic of individual floes of dimensions tens of metres to kilometres. Floe perimeters are marked by pressure ridges (,10 m high) or by freeboard steps (,0.5 m) between young and old ice. The sea ice thickness is generally 2– 3 m in the Central Arctic Ocean, 1 –2 m in the Beaufort Sea and Chukchi Borderland area, and around 2 m in the Nansen Basin (Rothrock & Maykut 1999). Any vessel traversing through the pack ice will also meet irregularly dispersed much thicker multiyear flows. Pressure ridges

criss-cross the ice surface, on average 0.5–2 ridges per kilometre (Weeks et al. 1971). Their keels extend three to four times deeper than their surface sail height (Tucker 1989) and their mean total widths cluster around 70 m (Wadhams 1994). The roughness of the ice –water interface has a spectral distribution broadly resembling the roughness of ocean waves (Rothrock & Thorndike 1980). However, for wavelengths ,20 m the spectral density of subice roughness is over 30 dB larger and scattering will affect frequencies above 35 Hz more severely (Dyer 1984).

Ambient noise Arctic Ocean ambient noise levels are strongly related to ice dynamics (Buck 1968; Makris & Dyer 1986). Noise levels build up and decay over periods of at least a day (Kutschale 1969). Drag from wind and currents on ice surfaces of varying top and bottom roughness, frictional forces and inertial motion leading to cracking, shearing and pressure ridging, are all processes which

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Fig. 45.2. (a and b) Principal patterns of ice drift in the Arctic Ocean after Rigor et al. (2002). Isolines indicate the time required for the ice to exit the Arctic Ocean through the Fram Strait during high Arctic Oscillation index (a) and low Arctic Oscillation Index (b). (c) Extensive melt ponds form on the sea ice surface during the melt season. Picture from Makarov Basin mid-August 1996. (d) The seasonal surface melt removes c. 0.5 m of ice and surface objects will pedestal (photograph courtesy of A. Heiberg).

radiate energy into the water over a wide range of frequencies (Fig. 45.3a). Maximum noise energy during low ice activity appears to be centred around 10 Hz with a 5 dB/octave roll-off to 1 kHz (Dyer 1984). The general spectral shape appears unrelated to noise levels varying about 15 dB between quiet and noisy conditions. Also, the noise is quite isotropic at high levels, but partly anisotropic during quiet conditions (Shepard 1979; Chen 1982). Buck (1968) monitored noise level as a function of depth below the ice by placing a reference hydrophone at 91 m depth and raising a second hydrophone in 6 m steps. For any particular frequency, the noise level increased by about 20 dB down to a depth of one-half wavelength and remained essentially constant below this depth (Fig. 45.3b). Buck & Greene (1964) also compared signal-to-noise ratios (frequency .10 Hz) between a hydrophone suspended at 60 m depth and a seismometer embedded in the ice and demonstrate that the ratio for the hydrophone is about twice that of the seismometer (Fig. 45.3c).

Wave propagation The speed of sound in sea ice varies from 3.1 to 3.8 km s21, being highest at low temperatures (Hunkins 1960). The Arctic Ocean water masses differ from lower latitude oceans by relatively small variations in temperature (21.7 to þ1 8C) and relatively large salinity variations (30 – 35 p.s.u.) from top to bottom. For this reason, the associated sound speed profile is primarily controlled by the salinity structure. Water mass properties change most dramatically in the upper 200 m. An uppermost cold and relatively fresh well-mixed surface layer down to 50 m depth is

frictionally coupled to the ice (Untersteiner et al. 1976). The resulting sound speed (Fig. 45.3d, left panel) has a minimum of 1437 m s21 at the top of the mixed layer, a large positive gradient associated with the halocline (50 –200 m depth) followed by a small constant gradient to abyssal depths (Kutschale 1969). Positive velocity gradients result in upward refraction of propagating energy, forming a near-surface wave-guide (Fig. 45.3d, right panel). Arrivals of the direct wave during a sonobuoy measurement will form a curved line with increasing offsets. The turning point for rays at offsets ,30 km will be shallower than about 1200 m depth (Fig. 45.3b). In the open ocean the axis of the wave-guide (or SOFAR-channel) is at about 700 m depth.

Working conditions in the pack ice Return of daylight by mid-March makes it possible to visually inspect the ice surface in a target area from the air in search of ice floes suitable for establishing an ice camp. Air temperatures at this time may be –25 to – 40 8C. Mid-March to the end of May is the optimum time window for aircraft-supported Arctic operations, with often clear skies and a firm frozen surface to land on. The occurrence of low-level Arctic stratus clouds increases between April and June due an increase in cyclonic activity (Serreze et al. 1993). Low clouds imply reduced light contrast of surface features and frequent white-out conditions. The snow surface starts to melt when the mean air temperature passes 21.2 8C and melt ponds (Fig. 45.2c) appear at 858N at about 1 July (Doronin 1970). Freezing starts again as air temperatures fall below zero during the last half of August. Ship operations

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in the Central Arctic Ocean are generally carried out between mid-July and the end of September. During the annual cycle, a c. 0.5 m thick layer is melted on the surface during the summer period and about the same thickness of new ice added to the underside during the winter. This vertical ‘conveyor’ makes surface structures pedestal (Fig. 45.2d) and transports sediments frozen to the underside of the ice to the surface.

Research platform alternatives There are five principal ways of carrying out research in an ocean covered by perennial sea ice: (1) establish a camp on the ice and drift passively; (2) force your way through with an icebreaker; (3) go under the ice with a nuclear submarine; (4) ride over the ice surface with a hovercraft; or (5) fly over the polar ice pack with an an airplane or satellite. Aero-surveys and satellites are cost-effective for potential field measurements and microwave imagery of sea ice and water, but waterborne sensors are required for acoustic subsurface imaging.

Ice drift stations

Fig. 45.3. (a) Characteristics of the ambient noise level in the Arctic Ocean at 93 m depth modified from Makris and Dyer (1986). (b) Ambient noise levels v. depth in the Arctic Ocean for various frequencies. After Buck (1968). (c) Signal-to-noise ratios of a hydrophone in the water compared with signal-to-noise ratios of a seismometer deployed on sea ice in the Arctic Ocean. After Buck and Greene (1964). (d) Typical sound velocity profile in the Arctic Ocean (left) and ray paths of the water borne energy between a source and receiver. Modified from Kutschale (1969).

Camps on the ice will most often be on multiyear sea ice (2 –4 m thick) and in rare cases on large ice shelf fragments (ice islands) broken off from outlet glaciers on the north coast of Ellesmere Island (Koenig et al. 1952; Jeffries 1992). The ice island T-3 was 13  8 km (Hunkins 1967) and was determined by electrical resistivity measurements to be about 60 m thick (Plouff et al. 1961). Deployments of small temporary camps when the daylight returns by the middle of March are usually by Twin Otter aircraft. Larger camps are supplied by landing larger planes and air drop or low-altitude parachute extraction from C-130 Hercules (Weber 1979; Johnson 1983). A 2 month camp with 20 persons involves moving 40– 50 tons of cargo plus 70– 150 tons of fuel. One or more helicopters are often available in the camp for regional surveys. The start of the melting season is associated with increasing occurrences of low clouds and white-out conditions and back-haul flight operations rarely go beyond the end of May in the Eurasia Basin and a couple of weeks later in the central Arctic Ocean. Ice camps move with the general large-scale sea ice drift pattern modulated by the local wind field. Extended periods (days to months) with unusual passages of smaller pressure systems may, however, result in superimposed excursions of more than 100 km or alternatively periods of little progress. US ice drift station T-3 made four 150 km long traverses across Alpha Ridge under circumstances like this during the summer and autumn of 1968 and 1969 (Hunkins & Tiemann 1977). An ice camp may have primitive facilities, but represents excellent working conditions for multidisiplinary science programmes: ample space, low ambient noise and an opportunity for all participating scientists to fully focus on their respective objectives. Another advantage relative to open ocean conditions is the possibility to maintain large instrument array geometries over time. In general, the ice surface moves as one unit on scales from kilometres to many tens of kilometres, but may suffer episodic local convergence or divergence events forced by shifts in speed and direction of the surface wind (Popelar & Kouba 1983). The consequences of relative ice movements may be significant for cableconnected array elements (Baggeroer & Dyer 1982), but less so for arrays of single self-contained instruments or sensors connected via radio link. Geoscience programmes in ice camps may include navigation, bathymetry, 3.5 kHz chirp echo sounder, sediment coring, seismic reflection and refraction measurements and gravity observations. Magnetic field intensity is best obtained by airborne surveys or a gradiometer configuration due to the time variations

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in the geomagnetic field (Coles & Taylor 1990). A regular land gravimeter placed on the ice is sensitive to long-period vertical motion and needs extra damping for convenient readout (Crary & Goldstein 1957). Echo sounder transducers are suspended below the ice through a hydro hole inside a scientific work space. Making a hole through c. 2 m thick ice with a small auger and chainsaw may take a man-day; the building is later put up over the site. The air gun may have a separate hole and is suspended shallow enough (3– 5 m) to ensure air released from each shot is vented through the hole. Accumulation of air pockets below a camp may generate local stress nodes which could attract crack propagation in the event of regional ice dynamics. A small diver compressor (140 l min21) can supply air sufficient for a 0.6 l air gun fired at 50 m shot spacing or about every 4 min during fast drift. Air guns operated at a low repeat cycle may not seal properly in the cold water ( –1.7 8C), but do in general work well. Traces of alcohol in the air line prevent freezing and increased solenoid voltage improves reliability. Alternatively, one may use a sparker source as in the case of the 9 kJ system on T-3 (Hall 1973, 1979). The seismic signals are received by a single hydrophone deployed 30–50 m away from the source and recorded on a laptop. A complete seismic single channel field system based on modern technology may weigh less than 200 kg (Kristoffersen & Mikkelsen 2006). Figure 45.4 shows examples of data recorded from ice station field camps by analogue and digital single channel seismic systems using air gun or sparker source. In spite of the limited

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source strength, it is possible to define acoustic basement below the main submarine ridges in the Arctic Ocean. The 9 kJ sparker yields a penetration of 2 s travel time below the abyssal plain. Water depths away from the shelf areas are sufficiently large, so interference from water bottom multiples is not important. Russian investigators have operated seismic reflection programmes on eight of their over 30 ice stations beginning with North Pole-13 in 1965 (Gramberg et al. 1991; Sorokin et al. 1999). They have consistently used detonators (three to five) as seismic source fired at the centre of a cross-legged (550  550 or 1150  1150 m) receiving array. Each leg comprised 12 channels recorded on analogue tape and shot spacing was mostly c. 500 m. The analogue traces were later digitized and summed to form a centre trace. The data has good signal-to-noise ratio and an example from North Pole-28 is shown in Figure 45.4 (lower right). We may further exploit the sea ice surface by placing continuously recording sonobuoys offset at right angles to the drift direction and obtaining simultaneous parallel lines (Kristoffersen & Mikkelsen 2006). However, the maximum offset must be less than the critical distance for emergence of a bottom refracted arrival and is thus water depth-dependent. This concept may be expanded to emulate a full 3D survey by aligning detectors and several seismic sources perpendicular to the prevailing drift direction. We may also emulate a multichannel seismic cable by aligning the row of sensors with the average drift direction as carried out from US ice station Fram-4 in 1982 (Kristoffersen & Husebye 1985). Hydrophones from 20 modified continuously recording sonobuoys were deployed through the sea ice at 100 m intervals trailing the main camp (Fig. 45.5a). Hydrophone depth was 60 m and the source was a 2 l bolt air gun fired at 13 m depth. During 34 days of continuous operation, the ice surface moved at of 0– 25 cm s21 (maximum 15 km per day) and firing rates were continuously updated from one to three satellite fixes per hour to maintain a 50 m shot interval (Fig. 45.5c). The ice floe orientation was monitored daily by theodolite sun shots and stayed within +38 of its starting value (Tiemann et al. 1982), but periods of easterly Q2 wind caused significant cross-array drift (Fig. 45.5b). We were forced to operate the air gun at maximum 100 bar instead of 140 bar to reduce leaks and recorded bottom reflections with a signal-to-noise ratio of 33 dB during periods of slow drift (3 cm s21) and 6 dB or less during fast drift (16 cm s21). Vibrations from vortex shedding along the hydrophone cable became significant above a drift speed of 20 cm s21. This experimental setup successfully acquired about 200 km of multichannel seismic data. Normal move-out corrections are small for the case of a short streamer (2 km) relative to the water depth (3.8 km) and we assumed interval velocities representative of a deep ocean environment to generate stacking velocities. Varying degree of array feathering was clearly a problem as common mid-points within a 50 m bin would be scattered over a distance of more than 500 m perpendicular to the track in the worst cases. The consequence is minor over a level abyssal plain, but a strike line over bottom and subsurface layers sloping 58 would imply a travel time difference of 56 ms between zero and 308 array feathering for the far offset trace. Stacking efficiency would, in this case, be degraded unless traces were selected so that midpoints lay on a line perpendicular to profile direction (Levin 1983). Results of the experiment are shown in Figure 45.5d. The advantage of the ice cover to maintain receiver array geometry has also been successfully used for recording microearthquake activity on the Gakkel spreading centre by a sonobuoy array (Kristoffersen et al. 1982) and seismometer arrays (Schlindwein et al. 2007). Q3 Measurements of heat flow through the seabed in the deep Arctic Ocean are carried with thermistors spaced out on a lance or sediment corer as used in the open ocean. A heat flow programme initiated in 1963 by US Geological Survey on US ice station T-3 produced observations at 356 localities within the Amerasia Basin (Lachenbruch & Marshall 1966, 1969). Other measurements

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from ice stations have been made by Canadian (Judge 1980; Taylor et al. 1986) and Russian groups (Lubimova et al. 1973, 1976). Heat flow measurements have been accompanied by sediment coring to obtain estimates of the conductivity.

Icebreakers The Russian nuclear icebreaker Arktika was the first surface vessel to reach the North Pole – a ‘scientific –practical experimental voyage’ (Anonymous, Polar Record 1978). The Murmansk to Murmansk trip was made in August 1977 with an average speed of 11.5 knots. Today, over 40 years later, there are unfortunately still no reports of a nuclear icebreaker ever being used as a primary research platform for geoexploration. The first penetration of a diesel-driven icebreaking research vessel in 1987 heralded a new era in marine geoscientific research in the Arctic Ocean. Polarstern reached beyond 868N north of Svalbard, carrying out a full complement of geophysical measurements and geological sampling except for the use of towed equipment (Thiede 1988). Towing of seismic equipment in heavy pack ice was pioneered in 1988 by Arthur Grantz of the US Geological Survey from US Coast Guard icebreaker Polar Star in the Northwind Ridge area (Grantz et al. 1992). The air gun was suspended below a 1.27 ton steel ball and a two-channel 150 m long hydrophone cable

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Fig. 45.5. (a) Cartoon of the array of recording sonobuoys emulating a seismic streamer trailing the Fram-IV camp site along the prevailing drift direction. (b) The array kept its orientation, but drifted sideways in crosswinds. (c) The ice drift followed closely changes in the surface wind. (d) Sample processed section of data acquired over 32 h of drift in the Nansen Basin at the end of April 1982. Modified from Kristoffersen & Husebye (1985).

was fed through a protective hose and effectively towed from the depth level of the air gun (20 m). This arrangement was later expanded to include six air guns (15 l) attached to a triangular frame below the steel ball (Fig. 45.6). The tow line was now an armored umbilical which carried all feeder lines. A single cable for source and hydrophone cable avoided tangling. About 2295 km of seismic reflection data and 28 sonobuoy measurements were made during the 1988, 1992 and 1993 seasons without loss of equipment (Grantz et al. 1993). Polarstern uses a seismic source of eight air guns suspended within a frame for operations in light ice conditions (Fig. 45.6). The first seismic lines across Lomonosov Ridge (Jokat et al. 1992) were acquired in 1991 using one or two air guns towed below a weight, as done by Grantz (1993). Q4 Broken ice of cubic metrre sizes sweeps along the ship’s hull and enters the turbulent wake behind the stern. It is imperative that cables enter the water as close to the stern as possible. However, from time to time the protective hose gets caught behind an ice block and all the gear is forced to the surface. The heavier the gear, the greater the strain on tow cables. Loss of four air guns from Oden in 1996 prompted the use of a depressor (Fig. 45.6) for downward pull and reduced equipment weight (Kristoffersen 1997a). The depressor is easy to handle, but not as effective as a heavy steel ball in keeping the gear close to the stern, which implies that the gear will more often be forced to the surface. Another concern is towing depth. Towing at 20 m

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Fig. 45.6. (Upper) Towing arrangments for seismic sources used during data acquisition in sea ice by Polar Star (Grantz et al. 1993), (middle) by Oden (Engen et al. 2009) and (bottom) by Polarstern (Jokat et al. 1992).

depth means the gear is below the main propeller wash, closer to the stern and less likely to be forced to the surface – a ‘survival mode of operation’. The downside is lower seismic resolution from a notch at 40 Hz in the source and receiver spectra created by the delayed surface ghost reflection. Towing with a depressor and at shallower depth gives better resolution, but represents a greater risk for loss of equipment – ‘suicide mode’. The greatest risk is related to the hydrophone cable, particularly in situations where sharp course changes are made. The turbulent wake behind the icebreaker is progressively filled up by blocks of broken ice moving randomly with great force. Once the seismic source is forced to the surface, the entire streamer will follow with a high risk of getting the cable pinched between moving blocks of ice (Fig. 45.7c, d). The inevitable result is torn internal signal wires and loss of hydrophone groups, or, if the ice is under some pressure, loss of major parts of the cable. A practical length of a hydrophone cable behind an icebreaker in heavy ice of less than 500– 300 m is most often used. The cable length compared with water depths greater than 1 km implies that reliable stacking velocities cannot be derived by conventional analysis. Velocity information has to be obtained from from sonobuoys. Useful signals from sonobuoys can be received for offset distances out to about 30 km (Jokat 2003; Engen et al. 2009). Sample shot records (Fig. 45.7a) and the resulting stack (Fig. 45.7b) acquired in heavy ice in Makarov Basin with only 11 live channels out of 24, still yields useful data with about 2 s penetration. Use of a second icebreaker in front of an icebreaking seismic acquisition vessel may in general translate into steadier progress,

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but only if there is no pressure on the ice. The assistance of Russian nuclear icebreakers has been used in two-ship operations in areas influenced by the thicker ice of the Beaufort Gyre (Jokat 2003; Marcussen 2008). A nuclear icebreaker may keep a straight course in þ3 m thick ice, while a diesel-driven icebreaker operating alone prefers to follow leads. Breaking and ramming intact ice may double fuel oil consumption and is restricted to transitions from one lead to the next aligned with the general direction of travel. Leads tend to have frequent choke points (every few hundred metres) where forward momentum is lost and ramming is required. In this situation, the ship may ease astern (þ50 m) with the seismic gear out and accelerate forward again – otherwise the gear has to be retrieved temporarily and redeployed when the obstruction is passed. Seismic data acquisition in heavy sea ice is characterized by high noise levels, the main contributions being the fundamental frequency and higher harmonics of the ship’s propeller and engines (Buravtsev 1995). The noise levels (rms mbar) during single ship operation in 2– 2.5 m thick ice are three to four times the levels where a clear channel has been made by a lead vessel or in open water (Jokat et al. 1994). Observed noise levels diminished dramatically with offset out to about 280 m from the stern and levelled out for more distant channels. A modern icebreaking research vessel has facilities for a complete suite of geophysical measurements and heavy equipment for geological sampling. Introduction of multibeam swath survey capabilities and high-resolution sub-bottom profiling during the first penetration of Polarstern to 868N north of Svalbard in 1987 (Thiede 1988) represented a huge step forward. From 2007 and onwards, three Western icebreakers (Healy, Oden and Polarstern) routinely collect fundamental seabed information in this manner. The bottom track may be lost during active ramming in heavy ice due to air bubbles in the turbulent water. Important data can, however, be obtained by making the ship turn 1808 in one spot to insonify an area of diameter equal to the swath width (Jakobsson & Marcussen et al. 2008). Underway gravity data is also routinely acquired by Polarstern and Healy.

Nuclear submarines The first attempt to reach the North Pole in 1931 in a diesel-driven submarine was aborted, but the expedition successfully demonstrated the potential of a submarine as a science platform. HU Sverdrup carried out water sampling down to 3000 m depth as well as sediment coring through an open hole in a pressurized compartment of the submarine Nautilus at the ice edge north of Svalbard (Sverdrup 1931). US nuclear submarines Nautilus and Skate recorded the first continuous echosounder profiles across the Arctic Ocean in 1958 and 1959 and outlined the main features of the basin morphology (Dietz & Shumway 1961). During 1997, 25 years (1957 –1982) of soundings collected by US submarines were released to the public (Anonymous 1997). For many scientific disciplines, a submarine research platform would represent the ultimate solution for efficient scientific data acquisition in an ice-covered ocean. The Science Ice Excercise (SCICEX) programme (Fig. 45.8) allowed US scientists access to US Navy nuclear submarines either as ‘accommodation missions’, which allocated time to obtain unclassified data on otherwise classified missions (1993 –2001), or to carry out dedicated scientific surveys in the Arctic Ocean (Edwards & Coakley 2003). A major achievement was implementation of swath mapping capabilities and sub-bottom penetrating chirp sonar attached to the belly of USSN Hawkbill (Chayes et al. 1998). The submarine platform moved at 16 knots below the ice and collected swath bathymetry (width three times the water depth), high-resolution images of the upper þ50 m of sub-bottom sediments, gravity measurements as well as sampling a number of

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water mass properties. The dedicated cruises in 1998 and 1999 (Fig. 45.8) acquired geophysical data along 39.250 km of survey track, primarily over the Alaska continental margin, Chukchi Borderland, Lomonosov Ridge, Gakkel Ridge and Yermak Plateau (Edwards & Coakley 2003). Continued access to nuclear submarines for science has become difficult following a substantial reduction in the US submarine fleet.

Aerosurveys Airplanes such as the P-3 Orion aircraft cruising at 450 km h21 with an endurance of up to 6000 km, are very efficient platforms for regional potential field surveys (Childers et al. 2001). Minimizing the effect of temporal field variations is also a major concern in magnetic field intensity measurements. Rapid field changes are important in high latitudes, particularly in the auroral oval where large areas may have changes of .160 nT h21 (Coles & Taylor 1990). The earliest Soviet reconnaissance aeromagnetic surveys were initiated in 1946 (Demenitskaya & Hunkins 1970). A more systematic effort was undertaken from 1961 onwards and results from the Eurasia Basin were published by Rassokho et al. (1966) and Karasik (1968). Karasik (1974) presented a magnetic anomaly map including the Amerasia Basin. The US efforts began with field campaigns over the entire Arctic Ocean in 1950–1952 (King et al. 1964) and later in 1961–1963 (Ostenso & Wold 1971). These surveys documented a first order pattern with a ‘Central magnetic Zone’ of high amplitudes

Oden 2001

Fig. 45.7. (a) Shot files (low cut at 10 Hz) acquired during Healy cruise 0503 from Makarov Basin illustrating signal levels and (b) the result of processing. (c) Successful seismic data acquisition in progress from Healy in 2005 and (d) a case of difficult ice conditions with the entire seismic cable on top of the ice.

over the Alpha and Mendeleyev ridges and more subdued amplitudes in the Eurasia Basin. Canadian surveys in the 1960s covered over the outer Canadian Arctic islands and the continental shelf (Coles & Taylor 1990). Renewed effort by US Navy agencies in the years 1972 –1978 effectively translated into new understanding of the geological history of the Arctic Ocean; identification of a magnetic lineation pattern in the Eurasia Basin supported Karasik’s (1968) earlier work and tied basin evolution to the Cenozoic opening of the North Atlantic (Vogt et al. 1979), and a set of magnetic lineations in the Canada Basin associated with Mesozoic seafloor spreading (Vogt et al. 1982). An international effort to compile and integrate all aeromagnetic surveys carried out prior to 1990 was spearheaded by Geological Survey of Canada and published in 1996 (Verhoef et al. 1996). An update (Fig. 45.9) has been presented by Kovacs et al. (2002). Missions which included gravity, magnetic field intensity and sea surface heights were flown by the US Naval Research Laboratory during 1992–1999 (Brozena et al. 2003). Track spacing was 11–18 km and the resolution in the gravity signal along-track (22 –34 km) was effectively constrained by the low-pass filter used to extract the signal from the noise (Childers et al. 2001). Survey cross-over errors were ,2 mGal. More limited aero gravity surveys have been flown north of Greenland and Svalbard by Denmark, Germany and Norway. The inventory of Russian gravity data from the Arctic Ocean appears mainly in the form of on-ice gravity measurements made during aircraft landings (Maschenkov et al. 1999).

CHAPTER 45 ARCTIC OCEAN GEOEXPLORATION

553 554 555 556 557 558 559 560 561 562 563 564 565 566 567 568 569 570 571 572 573 574 575 576 577 578 579 580 581 582 583 584 585 586 587 588 589 590 591 592 593 594 595 Ubiquitous coverage of the gravity field south of 81.58N is pro596 vided by the satellite gravity field derived from the European 597 Space Agency’s Earth Remote Sensing (ERS) satellite altimeter 598 data. Advanced processing of the full waveform has made it poss599 ible to extract the gravity field over ice-covered areas (Laxon & 600 McAdoo 1998). Although track spacing at 758N is c. 2 km, the 601 size of the radar’s foot print makes it impossible to resolve wave602 lengths ,15 km in the gravity signal (Childers et al. 2001). An 603 example of a comparison between the airborne gravity measure604 ments in the Beaufort Sea region with the ERS-derived field 605 Q5 (ERS 1998) yielded an rms difference of 2.55 mGal. Compilation 606 of all available gravity data is the focus of the Arctic Gravity 607 Q6 Project (Keynon et al. 2008), a special study group under the Inter608 national Association of Geodesy with contributions from the 609 circum-Arctic countries, Finland, Sweden, Iceland, the UK, 610 France and Germany (http://earth-info.nga.mil/GandG/wgs84/ 611 agp/abstract.doc). The data (Fig. 45.10) is available from the 612 website: http://earth-info.nga.mil/GandG/wgs84/agp/agp_08/ 613 ArcGP_GRV.scn. 614 615 616 Hovercraft 617 618 Although a hovercraft can move with relative ease across open 619 water and sea ice of any thickness, its potential as an Arctic logistic 620 alternative remains unexplored (Fig. 45.11). A new hovercraft 621 dedicated to polar research was tested for the first time north of

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Fig. 45.8. Track lines for science missions by US Navy nuclear submarines. Figure courtesy of B. Coakley.

Svalbard during the summer of 2008 (Hall & Kristoffersen 2009). The craft can carry a payload of 2.2 tons, has sleeping quarters for four persons and is equipped with echo sounder/chirp sonar for high-resolution sub-bottom surveys, compressor and air gun for seismic reflection measurements (0.3 l air gun), EM-probe for ice thickness measurements, CTD and winch (to Q7 500 m) for oceanographic measurements and a sediment corer and winch (1100 m). The craft can, under favourable conditions, travel about 500 nautical miles between fuelling points. Some 3300 nautical miles of track were covered during the first summer (ultimo June –primo September). Its performance in the pack ice was up to expectations and the platform may be used in an ice drift station mode or act as a survey vessel in open leads. Use of hovercraft in conjunction with an icebreaker is expected to greatly enhance the efficiency of the total operation.

Autonomous underwater vehicles Detailed mapping and sampling at a submarine volcanic eruption site on the Gakkel spreading centre have been successfully carried out by two autonomous underwater vehicles (AUV) and a tethered platform, providing real-time high-definition video imagery (Sohn et al. 2008). The AUVs completed nine dives in water depths up to 4062 m. In some cases the vehicles surfaced below unbroken ice, but were located and successfully recovered after the floe had been cut by the icebreaker.

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622 623 624 625 626 627 628 629 630 631 632 633 634 635 636 637 638 639 640 641 642 643 644 645 646 647 648 Colour 649 online= 650 colour hardcopy 651 652 653 654 655 656 Fig. 45.9. Map of anomalies in total magnetic field intensity over the Arctic 657 Ocean of Kovacs et al. (2002). Track spacing is ,20 km (Childers et al. 2001). 658 659 660 Autonomous data buoys 661 662 Much of the thick sea ice in the Beaufort Gyre north of Canada and 663 Greenland appears inaccessible for surface vessels using towed 664 665 666 667 668 669 670 671 672 673 674 675 676 677 678 679 Colour 680 online= 681 colour 682 hardcopy 683 684 685 686 687 688 Fig. 45.10. Gravity map over the Arctic Ocean compiled by the Arctic Gravity 689 Q19 Project (Keyon et al. 2008). Data from http://earthinfo.nga.mil/GandG/ wgs84/agp/agp_08/ArcGP_GRV.scn. 690

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Fig. 45.11. Hovercraft as research platform may conduct surveys in open leads or operate as a drift station depending on ice conditions. (http://www. polarhovercraft.no/).

equipment, and support of manned ice drift stations is costly. Autonomous data buoys recording position, meteorological and oceanographic parameters have been in operation in the Arctic Ocean since 1979, but the ARGOS system can only handle small datasets (Untersteiner & Thorndike 1982). More data-intensive measurements can be transferred via the Iridium satellite system (Double et al. 2006). A prototype autonomous buoy for acquisition of seismic reflection data (Fig. 45.12) has recently been successfully tested north of Svalbard (Meyer et al. 2008). A 4.8 kJ sparker source is fired under GPS control and the data are recorded by a single hydrophone and stored on a flash disk. The first second of sub-bottom reflection is extracted from the dataset and subsequently transmitted to shore as short burst telegrams via the Iridium system. System power is from solar panels and a windmill, which limits operation to the light season of the year – April to August. A prototype data buoy for bathymetry is also under development (Hall 2008).

The Arctic Ocean: state of geophysical exploration A growing recognition of the need to compile and join datasets has, within the last decade, produced a new International Bathymetric Chart of the Arctic Ocean based on historical and modern datasets previously unavailable (Jakobsson et al. 2008), continuing improvements in merging old and new aeromagnetic datasets (Litvinova & Glebovsky 2008) and successful progress of the Arctic Gravity Project in compiling a 50  50 Free Air and Bouguer database (http://earth-info.nga.mil/GandG/wgs84/ agp/agp_08/ArcGP_GRV.scn). Bathymetry and the potential field data are our first-order tools for making meaningful interpretations of the geological evolution of the Arctic Ocean as well as planning future surveys. Next is our need to image sub-bottom layering and geological basement structures. About 16 000 km of multichannel seismic reflection data have been acquired to date in the Arctic Ocean, half of that by icebreaker cruises in 2005, 2007 and 2008. The inventory of seismic reflection data from ice stations is 15 648 km (Kristoffersen & Mikkelsen 2004). It is possible to successfully acquire good-quality seismic reflection data from an icebreaker in .2 m thick ice provided the pack ice field is not under pressure. Experience shows that the thick ice north of NW Greenland and the Canadian Arctic Archipelago is not accessible to surveys with towed equipment (Jokat 2003; Marcussen 2008). Other approaches must be used or advantage taken of situations where huge leads exist for days in the thickest ice as evident from satellite imagery. We will highlight some key points in our state of knowledge of the circum-Arctic continental margins, their marginal plateaus and the submarine ridges in the polar basin.

CHAPTER 45 ARCTIC OCEAN GEOEXPLORATION

691 692 693 694 695 696 697 698 699 700 701 702 703 704 705 706 707 708 709 710 711 712 713 714 715 716 717 718 719 720 721 722 723 724 725 726 727 728 729 730 Colour 731 online= 732 colour 733 hardcopy 734 735 736 737 738 739 Fig. 45.12. Autonomous seismic data buoy with a sparker source and recording 740 by a single hydrophone. Data are transmitted in real time as short burst messages 741 via the Iridium satellite system. 742 743 744 Eurasia Basin 745 746 Amundsen and Nansen basins. The active Gakkel spreading centre 747 divides the Eurasia Basin into two sub-basins (Fig. 45.1). Only 748 the western part of the Eurasia Basin is explored by multichannel 749 seismic surveys (Fig. 45.13). Rough basement topography is 750 covered by .2 km of sediments below the respective abyssal 751 plains (Jokat et al. 1995; Weigelt & Jokat 2001; Jokat & 752 Micksch 2004). The Nansen Basin, proximal to the glaciated 753 Barents – Kara Sea margin, is about 300 m shallower and sediQ8 ments are thicker (Glebovsky et al. 2004; Engen et al. 2009). 754 755 Amundsen and Nansen basins are associated with linear, albeit 756 low-amplitude magnetic lineation patterns that are symmetric 757 with respect to the Gakkel spreading centre and correlated with 758 the Cenozoic geomagnetic polarity time scale (Vogt et al. 1979; 759 Glebovsky et al. 2006).

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Gakkel Ridge spreading centre. The western 1000 km of the

1800 km long Gakkel spreading centre is covered by modern multibeam swath mapping surveys and with the effort of the joint Arctic Mid-Ocean Ridge Expedition (AMORE) in 2001 became one of the best surveyed ridge segments in the world’s ocean (Michael et al. 2003). The effort started with Polarstern in 1987 (Thiede 1988), continued in 1991 (Jokat et al. 1995) and was pursued by an extensive survey using a nuclear submarine (Fig. 45.8) during SCICEX (Cochran et al. 2003). East of 708E, the rift valley is filled with sediments. Melt production appears not to scale down directly with eastward-decreasing spreading rate as expected, but is either high or low within segments along the spreading centre (Michael et al. 2003; Jokat et al. 2003). Svalbard–Severnaya Zemlja continental margin. The margins bound-

ing the length of the Eurasia Basin are considered to be rifted, passive continental margins because the Gakkel spreading centre, located in the middle, is flanked by deep basins associated with ridge-parallel magnetic lineations (Karasik 1968; Brozena et al. 2003; Glebovsky et al. 2004). Six seismic reflection lines cross the continental margin (Fig. 45.1) west of 308E (Baturin et al. 1994; Geissler & Jokat 2004). Basement in this area remains shallow to about 100 km south of the shelf edge. The eastern 1500 km of the margin is covered by Russian potential field data, but unexplored by multichannel seismic reflection measurements. Basement tectonic lineaments along the entire margin trend about normal to the present continental margin (Bodganov et al. 1998; Johansson et al. 2005). Q9 Laptev Sea continental margin. The Laptev Sea continental shelf

(Fig. 45.1) is the continental extension of an active oceanic spreading centre where the present average divergence is 0.57 cm/year (DeMets et al. 1990) and estimated Cenozoic crustal extension is about 300 km (Gaina et al. 2002; Brozena et al. 2003). More than 25 000 km of seismic reflection data have been collected since 1984, suggesting that crustal extension on the shelf has been accommodated by a wide rift bounded to the east by a major detachment fault (Lazarev Fault) extending to the middle crust (Franke et al. 2001). Basement topography below the continental slope is interpreted as a shear zone which represents the transition between localized extension at the Gakkel spreading centre and distributed deformation on the shelf (Drachev et al. 1999; Sekretov 2002). Sediment thickness below the present shelf edge is about 7 km and reaches 13 km within the rift centre of the Ust’ Lena Rift Basin on the shelf (Franke et al. 2001; Sekretov 2002). No deep stratigraphic boreholes exist. Lomonosov Ridge northslope. Four seismic reflection transects and

two seismic refraction profiles extend from Lomonosov Ridge into Amundsen Basin (Fig. 45.13). The slope appears to be formed by a staircase of narrow blocks, and the difference in level between acoustic basement in Amundsen Basin and basement on top of Lomonosov Ridge is about 5 km (Jokat et al. 1995; Butsenko & Poselov 2004; Langinen et al. 2008). Gradients are gentler and the Free Air gravity low and magnetic low associated with the foot of slope are also less distinct between the North Pole and the Laptev margin than between Greenland and the North Pole (Brozena et al. 2003).

Marginal plateaus Morris Jesup. Morris Jesup plateau forms much of the North

Greenland continental margin and is presently the least known structure in the Eurasia Basin (Fig. 45.1). Available data include a traverse by ice station Arlis-2 in 1965 (Ostenso & Wold 1977), a brief visit over its northern tip by Polarstern (Jokat et al. 1995) and aerosurveys of magnetic and gravity measurements (Brozena et al. 2003). The plateau has a steep eastern scarp and more

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Fig. 45.13. Tracks of seismic reflection data in the Arctic Ocean. White tracks represents ice stations, red lines indicate multichannel data collected by Polarstern, Oden, Healy and Russian vessels, black lines are multichannel surveys by Polar Star. Blue lines represent tracks of Healy and Louis St. Laurant in 2008 (from http:// walrus.wr.usgs.gov/infobank/1108ar/html/1-1-08-ar.nav). Scientific drill sites shown by large white dots.

subdued sloping topography towards west and north as well as a strong east – west trending gravity gradient associated with the foot of slope to the north. The origin of the plateau has been tied to formation of the northeastern part of the Yermak Plateau (Feden et al. 1979; Jackson et al. 1984), or alternatively it may be part of a larger Arctic Cretaceous Large Igneous province (Engen et al. 2009). Yermak Plateau. Yermak Plateau forms two different structural trends, a western NNW trend and a northeastern part striking NE (Fig. 45.1). Aeromagnetic data show two domains – a northeastern part associated with high-amplitude (700 –900 nT) magnetic anomalies in contrast to a rather featureless magnetic field over the western and southern part (Feden et al. 1979). Earlier interpretations of magnetic, seismic refraction and gravity data suggested a purely volcanic northeastern part and a continental crust below the rest of the plateau (Feden et al. 1979; Jackson et al. 1984), including a western boundary formed by a transform related ridge of

massive basalt intrusions (Crane et al. 1982). A grid of multichannel seismic data acquired across the plateau west of 108W (Fig. 45.1) shows variations in basement topography up to 3000 m buried below a more than 50 km wide level crest of the plateau (Jokat et al. 2008). The horst forming Sverdrup Bank is considered an extension of tectonic lineaments associated with the Hornsund Fault Zone along the west coast of Spitsbergen farther south. Also, the northeastern Yermak Plateau may be stretched and intruded continental crust (Jokat et al. 2008; Engen et al. 2009).

Amerasia Basin Canadian Arctic continental margin. Crustal transects across the

Canadian polar margin north of Ellef Ringnes Island are based on seismic refraction measurements and gravity modelling (Sobczak et al. 1986). The northern rim of the Sverdrup Basin was uplifted during Campanian–Maastrichtian with erosional

CHAPTER 45 ARCTIC OCEAN GEOEXPLORATION

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truncation of Upper Triassic to uppermost Creataceous rocks over the distance from Ellef Ringnes Island to Banks Island (Balkwill et al. 1983). The Arctic Terrance wedge deposited north of the rim and below the present outer shelf comprises Maastrichtian and younger clastic sediments (Sweeney et al. 1990). A seismic reflection and refraction transect in the Beaufort Sea –Mackenzie area and gravity modelling suggest a rifted passive margin with a narrow transition zone in the eastern part and a broad area of transitional crust towards the west (Cook et al. 1987; Dietrich et al. 1989; Stephenson et al. 1994; Lane 2002). Arctic margin of Alaska. A single deep seismic reflection line

crosses the northeastern Chukchi Shelf (Fig. 45.1) at 1658W (Klemperer et al. 2002) and acoustic basement is not observed anywhere else in the oceanic domain along the continental slope of Arctic Alaska (Grantz et al. 1994). Regional uplift starting in Early Cretaceous (Valanginian) accentuated as well as eroded a structural high, the Barrow Arc, which extends from Yukon to NE (1638W) Chukchi Shelf (Mickey et al. 2002). The north flank of Barrow Arch represents a hinge line with a dramatic increase in sediment thickness (.10 km) above a Lower Cretaceous Unconformity as well as crustal thinning (Saltus & Bird 2003). The crest of Barrow Arch subsided and a thin condensed Hauterivian sediment section accumulated above an unconformity considered to represent the breakup unconformity at a passive rifted continental margin (Mickey & Haga 1987; Grantz et al. 1990). The Alaskan margin has no associated linear magnetic field signature which could reveal contrasting continental and oceanic crustal domains (Kovacs et al. 2002). Also, in spite of exceptionally thick sediment accumulations along the margin, the free air gravity anomaly is of lower amplitude and more

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discontinuous than observed along both rifted and sheared North Atlantic continental margin segments. Chukchi Borderland. The Chukchi Borderland (Fig. 45.1) appears

as an assemblage of north-trending linear fault blocks. Gravity modelling suggests that the crustal root of the borderland extends down to 27 km depth (Hall 1990). The geomagnetic field appears smooth over Northwind Ridge and Northwind Plain, but high and uniform over Chukchi Cap (Kovacs et al. 2002). Two depth-transects of piston cores up the steep eastern slope of Northwind Ridge recovered rocks which represented every Phanerozoic system except Devonian and Silurian and document the probably continental nature of the ridge (Grantz et al. 1998). East Siberian Sea continental margin. The continental margin

includes a shelf area up to 800 km wide (Fig. 45.1). Multichannel seismic transects exist north of De Long Island (1608E) (Franke et al. 2001; Sekretov 2001), and a summary of a refraction section has been presented by Grikurov et al. (2003). Thin sediments cover basement over De Long High, increasing to 8 km below the shelf break and over 9 km below the continental slope in 2000 m water depth. The crust is about 7 km thick below the lower continental slope. The geological structure associated with the junction of Mendeleyev Ridge with the continental margin is not known. The East Siberian continental margin appears to have the characteristics of a rifted margin. Lomonosov Ridge –Makarov Basin margin. The Amerasia Basin

facing the upper slope of the Lomonosov Ridge shows a prograding wedge (Fig. 45.14) below the early Cenozoic planar

Fig. 45.14. (a) Seismic section across Mendeleyev Ridge acquired by Healy in 2005 and (b) over Lomonosov Ridge by Polarstern in 1991.

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unconformity in the central part of the ridge (Jokat et al. 1992; Kristoffersen et al. 2004). Distinct linear bathymetric expressions which include the Marvin Spur and buried basement segments extending towards the Siberian margin are present at the foot of slope accompanied by co-located gravity and magnetic anomaly trends (Jokat 2005; Cochran et al. 2006). Chaotic reflection segments are observed in four crossing multichannel profiles. This tectonic trend has been associated with a major shear zone postulated in models of the Amerasia Basin formed by clockwise rotation of an Alaska –Chukota block (Green et al. 1986; Grantz et al. 1998; Cochran et al. 2006). Canada Basin. Canada Basin is the largest of the polar sub-basins

(Fig. 45.1) and the estimated thickness of predominantly terrigenous sediments varies from .6 km in the western part to more than 12 km towards the Beaufort shelf (Grantz et al. 1990). The relative contribution of hemipelagic sediment input can be assessed from the thickness of the sediment drape (0 –7 –0.8 km) covering the high-standing Alpha and Mendeleyev ridges to the north of the basin and unaccessible to turbidite deposition (Dove et al. 2009). Plate boundaries during evolution of the Canada Basin remain elusive (Grantz et al. 1998). The gravity field shows little variation except for a low-amplitude, but distinct linear trend running approximately north –south from north of the Mackenzie Delta to the foot of Alpha Ridge (Laxon & Q10 McAdoo 1994). Weak magnetic amplitude anomalies are colinear with this feature, which is suggested to represent an extinct spreading centre (Taylor et al. 1981; Kovacs et al. 2002). The intriuging possibility of the deep Canada Basin being floored by oceanic crust associated with this fan-shaped zone of weak linear magnetic anomalies and by extended continental crust elsewhere has been forwarded by Grantz et al. (2011). The sea ice is thickest north of Arctic Canada and the northeastern part of Canada Basin is not accessible for multichannel seismic surveys from icebreakers (Fig. 45.13). Submarine ridges – Lomonosov Ridge. Lomonosov Ridge reaches

water depths of 500–1000 m and divides the polar ocean into two sub-basins (Fig. 45.1). The ridge is 1750 km long and 40– 70 km wide in the central part and 150 –200 km at both ends. The structure appears to be formed by an ensemble of en echelon fault blocks slightly oblique to the main trend (Jokat et al. 1992; Cochran et al. 2006). The internal block stratification or structure remains unresolved. The postulated origin as a sliver rifted off the Mesozoic Svalbard – Severnaya Zemlja margin (Wilson 1963) is since supported by the presence of a prograding wedge on its south side (Jokat et al. 1992). Foresets are truncated by a planar unconformity and scientific drilling has documented ridge elevation at or near sea-level in the early Cenozoic (Moran et al. 2006). On the Eurasia Basin side, the rifted continental margin is formed by a steep staircase pattern of narrow blocks. Only the central part of Lomonosov Ridge (858300 –888N, 1508E) and the end north of Canada/Greenland (848300 – 888N) show peneplained surfaces below a younger sediment drape, indicating subaerial exposure, erosion and subsidence. Submarine ridges – Alpha and Mendeleyev ridges. Alpha and Mende-

leyev ridges form a 250–800 km-wide rise reaching water depths shallower than 2000 (Fig. 45.1). About 4000 km of new multichannel seismic data have been acquired over its accessible part (west of 1508W) by icebreaker cruises in 2005 and 2008 (Fig. 45.13). The ridges are covered by a 700– 800 m thick drape of hemipelagic sediments and acoustic basement is characterized by laterally varying, internal bright reflection segments and subbasement velocities in the 3.5 –5 km s21 range (Dove et al. 2009). Long-range refraction experiments on both ridges show velocity –depth relation distinctly different from a global average velocity –depth functions representing a wide range of continental settings (Forsyth et al. 1986; Christensen & Mooney 1995;

Lebedeva-Ivanova et al. 2006). The nature of acoustic basement as well as the seismic velocity of its deeper structure suggest a volcanic origin of the ridges.

Scientific drilling A proposal for scientific drilling in the central Arctic Ocean (Proposal 533) matured from events which included the seismic documentation acquired in 1991 of a c. 450 m thick hemipelagic drape on top of Lomonosov Ridge (Jokat et al. 1992), a stationkeeping test in drifting sea ice by Oden in 1991 (Kristoffersen et al. 1992), an unsuccessful attempt to sample sediments on the ridge by shallow drilling (Kristoffersen 1997b) and transition to an Integrated Ocean Drilling Program which embraced the concept of mission-specific platforms. An ice-strengthened drilling vessel assisted by two icebreakers penetrated 420 m of Cenozoic sediments unconformably overlying Campanian (c. 80 Ma) shallow marine sands (Moran et al. 2006). The section has a stratigraphic gap of 26 Ma (44 –18 Ma). Scientific highlights include documentation for bi-polar emergence of ice prior to 40 Ma and enhanced bi-polar ice growth at c. 14.5 Ma. The Eocene section contain 4 –14% organic carbon.

Concluding remarks Camps on drifting sea ice and aerosurveys were the principal platforms during the first 50 years of Arctic Ocean exploration. The sea ice drift pattern is irregular and camp programmes were not optimized for sub-bottom exploration. New aerosurveys can improve definition of the gravity and magnetic fields, but the firstorder features are known. The pioneering acquisition of multichannel seismic data in heavy sea ice in 1988 (Grantz et al. 1992) marked the beginning of a new era in Arctic Ocean exploration. The other milestone was diesel-driven icebreakers reaching the North Pole in 1991 (Fuetterer 1992). These new opportunities have unfortunately not been fully realized because of half-hearted efforts to tailor equipment for handling and ice protection of seismic gear in the turbulent wake of an icebreaker, a consequence which directly translates into considerable waste of expensive icebreaker time. This issue needs attention. The efficiency of an icebreaker may be further enhanced by an accompanying hovercraft serving as an independent seismic vessel or mobile ice drift station depending on ice conditions. Our present inventory of seismic reflection data falls short of providing substantial clues on complex issues like the tectonic evolution of the Amerasia Basin. Nevertheless, the reflectivity and reflection geometries of hemipelagic deposits on elevated submarine ridges provide important constraints on the palaeoceanography of the basin and define targets for future scientific drilling (Moran et al. 2006; Dove et al. 2009). The author has enjoyed the benefit of joint seismic field operations in the Arctic Ocean with W. Jokat, B. Coakle and J. Hopper and numerous discussions with A. Grantz. The spirit of the captains and crews of Polarstern, Oden and Healy contributed to successful multichannel seismic operations under sometimes challenging conditions. GMT software (Wessel & Smith 1991) was used to generate some of the figures.

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