Introduction

The Siberian Arctic seas (Laptev–East-Siberian–Chukchi seas) are vast shelf areas that are now covered by shallow waters. However, because the shelves break at around 100 m water depth, this region was part of the Beringian permafrost landscape that once connected Arctic Eurasia with the American continent during times of major glacial sea level lowstands.

Of these seas, the Laptev Sea shelf is one of the key sites where the existence of subsea permafrost was first suggested from bathymetry data [21, 22], geological onshore data [53], as well as mathematical modeling [20, 43–45, 58] assisted by deep, and shallow seismic studies [12, 29, 30] as well as near-coastal and offshore drilling attempts [18, 32, 36].

Purely mathematical modeling approaches would imply that major areas of the Laptev shelf are characterized by widespread ice-bearing and ice-bonded subsea permafrost, and so-called taliks, local areas of unfrozen ground within the permafrost. Judging on the onshore permafrost, the maximal thickness of the offshore permafrost is estimated to reach 500 m depending on the heat-flow values and lithology employed in the model [20, 45]. By contrast, direct evidence of the subsea permafrost is limited mainly to the shallow near-shore zone, whereas coast-distal information is still very sparse. Starting in the mid 1970s by Russian geological explorations, hundreds of boreholes were drilled offshore the Olenek and Khatanga interfluves, on the New Siberian Islands. These all documented as a subsea extension of the terrestrial permafrost (VNIIOkeangeologia internal reports).

More recently, a number of Russian–German seismic and echosounder surveys to the eastern Laptev Sea discovered a basal reflector (BR), likely to be indicative for subsea permafrost [8, 12, 29, 30, 37]. However, the spatial distribution of the BR remained unclear. Coastal and offshore permafrost drilling campaigns were performed within the framework of the Russian–German Cooperation Dynamics of Permafrost in the Laptev Sea [6, 36]. These and other near-shore borehole profiles all discovered ice-bearing relict continental permafrost submerged under the sea. By comparison, offshore evidence for the existence subsea permafrost was revealed through offshore drilling in 2000 [18]. That study clearly shows that relicts of permafrost also exist today on the outer shelf and below a sediment cover of Holocene age [16].

Summarizing the above, we conclude that the existence of ground data about the regional offshore permafrost distribution is still insufficient and, therefore, knowledge remains rather elusive and speculative. Although the mathematical models predict widespread offshore permafrost, drilling observations so far provided only limited and very local information but lacked insight into the spatial distribution of subsea permafrost. It is the intention of this study to employ high-resolution seismic (HRS) data with the aim to give the first regional generalization of subsea permafrost distribution on the eastern Laptev Sea shelf. This research is based on the interpretation of a multitude of HRS lines which were collected during various ship campaigns between 1998 and 2006.

Study area, dataset, and methods

The study area is located on the eastern Laptev Sea shelf at water depths of 15–60 m and between the Lena River delta and Kotel’ny Island (Fig. 1) within a subsea continuation of the North Yakutian coastal lowlands. The latter is an area of widely distributed Ice Complex (IC). The term IC is applied to permafrost sequences which usually consist of fine-grained, loess-like sediments with syngenetic ice wedges. On the northern Siberian lowlands, ICs formed during the Late Pleistocene regression (MIS 4-2), thus probably also including most of the drained Laptev Sea shelf. As these Siberian shelves remained largely unglaciated during the Late Pleistocene, sustained subaerial exposure led to the development of continuous permafrost hundreds of meters thick. This must have changed during Holocene inundation of the Arctic shelves, which ended at about 5–7 ka [3, 55], and during which air temperatures in the Arctic increased, also resulting in enhanced thawing of submerged permafrost [19].

Fig. 1
figure 1

Location map of the study area in the Laptev Sea. White lines show PARASOUND profiles obtained during ARK-XIV/1b cruise [17]. Solid black lines indicate HRS profiles of survey TDR-X. Dashed black lines HRS lines of MAGE [34]. Inset A shows location of TDR-X key area. The bold lines show location of the figures in the text

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Although this study is based on the complete HRS dataset available for the region at present (Fig. 1), data quality significantly varied [29, 30, 34, 37, 39]. The best signal-to-noise ratio stems from seismic data acquired during Russian–German expedition “Transdrift-X” (TDR-X) in 2004. Thus, the initial seismic model is mainly based on that dataset. To verify and extrapolate the seismic model over a larger area of the eastern Laptev Sea shelf, both PARASOUND lines from Polarstern cruise ARK-XIV/lb [17] and HRS data of Marine Arctic Geological Expedition (MAGE, Murmansk, Russia) [34] were also considered. Shipboard GPS navigation formed the basis for positioning, leaving an uncertainty on the order of a few tens of meters. The original bathymetric model was constructed by digitizing the large-scale nautical charts.

The TDR-X datasets were acquired by means of both “Sonic M-141” profiler system (VNIIOkeangeologia, Saint-Petersburg) and multichannel seismic (MCS) system of Bremen University, Germany [49]. Sonic M-141 comprises 4.5 kHz profiler and side-scan sonar mounted on the towed fish. MCS includes 48-channel streamer, BISON seismic recording system and a SODERA S-15 watergun. The seismic frequencies range from 100 to 500 Hz. Both “Sonic M-141” and MCS systems were operated simultaneously. The MCS system was towed at a distance of 100–150 m astern, whereas “Sonic M-141” was launched below the ship stem at a water depth of 6 m.

Since the main objective of the TDR-X cruise was to detect seismic signatures related to subsea permafrost, a number of seismic lines were acquired in scouting mode in order to select the most promising sites within the selected study area. Based on these scouting lines, the seismic survey focused near the SW foot of Semenovskaya bank at 15–39 m water depths (Fig. 1). A total of 42 HRS lines were obtained during TDR-X expedition, and 25 of them acquired from the TDR-X key area.

Seismic data were interpreted in “The Kingdom Suite” software (by Seismic Micro-Technology, Inc, Texas, USA) with routine seismic procedures for horizon identification, tracing, and mapping. Then all seismic horizons were exported into “Surfer” for 3-d imaging and spatial analysis.

Results

Seismic features

In this paper we describe permafrost-related seismic signatures and provide seismo-stratigraphic characteristics for HRS sections. The most prominent seismic feature found in the HRS data is a strong BR separating the lower acoustically transparent unit (ATU) from the upper stratified one. This boundary is a high-amplitude reflector with well-defined positive polarity, suggesting an increase in acoustic impedance (Fig. 2). Very often the BR looks like a non-stratigraphic, i.e., post-sedimentary, boundary, crosscutting the host strata. The BR occurs at the depths of 20 m below the sea floor (mbsf) in the central part of the TDR-X study area, but ascending up to 1 mbsf farther in the southeast (Fig. 3). In the central part, the BR forms a prominent hummocky surface with a number of flat, 0.5–6 km wide, highs and depressions with relative elevation changes of up to 20 m (Fig. 2e). In the remainder of the study area, the BR is more leveled and diffused.

Fig. 2
figure 2

Fragments of the 4.5 kHz “Sonic-141” profiler lines S-035 (a) with interpretation (b) and S-011 (c) with interpretation (d) and S-040 with interpretation (e). Location of the lines is indicated in Fig. 1A. Basal reflector (BR) is clearly observed at the top of acoustically transparent unit (ATU). Stratified sediment sequence above the BR is divided by the TR into the fill sequence (FS) and marine sequence (MS). The number of clinoforms occurred within permafrost overhungs (PO). Gas seeps (GS) appeared at the NW edges of the depressions. Other acronyms: LR lower reflector, STU semitransparent unit

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Fig. 3
figure 3

Seismic line GeoB04-011 of “BISON” seismic system shows the transition between facies zones A and C near Vasilievskaya bank. For location see Fig. 1A. Prominent seismic boundary with dissected topography marks the top of sands (ST). The semitransparent unit (STU) revealed beneath the ST is assigned to the Muruktian sandy deposits. Other acronyms: LR lower reflector, ATU acoustically transparent unit, GS gas seeps

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The sediment pattern above BR is subdivided into two units by a subhorizontal top reflector. The lower one, named fill sequence, occurs only in depressions while the upper one, marine sequence (see section “Interpretation”), overlies both fill sequence and acoustically transparent units in the depressions and on the highs, respectively (Fig. 2). A distinct lower reflector is observed in the lower part of fill sequence over the majority of depressions (Figs. 2, 3). The acoustic stratification is generally weakening upward in the seismic section.

The sea floor is characterized by V-shaped incisions 2–4 m deep and ≤40 m wide with one or two shoulders elevated above the adjacent seafloor (Fig. 2). We interpret these features as recent sea-ice ploughmarks, which were also evidenced from the side-scan sonar mosaics as linear, curvy-linear, and circular channels on the seafloor. Similar V-shape incisions, but filled with stratified sediments, are found on the HRS data (Fig. 2e) at depth of 3–5 mbsf. These featured are considered as an ancient, buried ploughmarks, which become less abundant downward in seismic sections and completely disappearing at subbottom depths >5 m.

Fill sequences are notably asymmetric. Near the southeastern parts of the depressions, they onlap acoustically transparent deposits, whereas at the western and northwestern side it forms a progradational stacking pattern with clinoforms (Figs. 2, 4). The clinoform package might indicate prevalence of sediment influx from the northwest of the depressions.

Fig. 4
figure 4

Fragments of the 4.5 kHz “Sonic-141” profiler lines # S-037, S-011, and S-035 with interpretation. For location see Fig. 1A. The package of the prograding clinoforms at the NW edge of depression is clearly defined within “permafrost overhung” (PO). T-shape line marks the recent location of the acoustically defined permafrost table. Gas seeps (GS) associated with taliks [39]. Other acronyms: ATU acoustically transparent unit, FS fill sequence, MS marine sequence, TR top reflector

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Remarkable transparent zones were discovered within a clinoform package at the NW edges of BR depressions (Fig. 2). As documented before [39], these zones can easily be traced across several parallel seismic lines headed both NW and SE directions (Fig. 5A). Therefore, we believe that these features do not represent seismic artifacts but features called “permafrost overhung” [2]. These forms are believed to originate from lateral freezing of lacustrine deposits under shallow water environments. Following that description, we adopted the name “permafrost overhung” for our found transparent zones [39].

Fig. 5
figure 5

Topography of the BR surface, interpreted as a top of acoustically defined permafrost. For location see Fig. 1A. Depressions are believed to be of thermokarst origin. Gas seeps (pink) appear in the centers of thermokarst depressions and are associates with taliks. The hatched areas along the west edges of the thermokarst depressions mark the permafrost overhung (PO) structures. Similar facies zones within Lena delta are shown on the inset A

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A large number of vertical acoustic blanking anomalies with an uneven, degraded surface on top were found on the seismic records (Figs. 2, 4). Within the TDR-X key site, they commonly occur within centers of deeply buried BR depressions (Figs. 4, 5) and are therefore likely due to concentrated gas discharge. We interpret them as areas of concentrated gas seeps. Another type of gas discharge is revealed in the central part of the study area and within a former Lena paleovalley (Figs. 6, 7). Its seismic signature is rather pervasive being diffuse or “fuzzy” and shows neither an apparent interface below nor inner reflectors. Such extended areas of scattered gas seeps may therefore be associated with subsea permafrost degradation below a paleovalley.

Fig. 6
figure 6

PARASOUND line PS98-12080 [17] in the eastern branch of Lena paleoriver valley (location is shown in Fig. 1). Obvious change of the seismic signature appears at the boundary between D and “Fuzzy” facies zones. Inset A shows spatial distribution of the “Fuzzy” features. Other acronyms: ATU acoustically transparent unit

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Fig. 7
figure 7

Map of the facies zones within the study area. The C, D and A, B facies zones are controlled by the local highs and terraces, respectively. The “fuzzy” zone in the pre-Lena paleovalley marks the area of extensive gas discharge caused by the permafrost degradation in the channel talik. The bathymetry is derived from digitizing of nautical charts. Inset A [46] shows an obvious increase in methane ratio in the atmospheric layer northeast of Lena Delta

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Sediment core features

No deep drilling data are available from our key study area. However, the giant gravity core (kasten corer) PS51/92 was taken from the eastern Lena paleovalley during Polarstern cruise in 1998. Radiocarbon dates show that the core’s chronology extends back to almost 9 ka (Fig. 8). Further analysis of geochemical features, which allow a distinction between terrestrial and marine organic matter (δ13Corg), in combination with micropaleontological investigations all clearly indicate that sediments before 7.5 ka (i.e., the lowermost 2 m of the core) were deposited under low-salinity conditions, i.e., under the influence of terrestrial river runoff carrying terrestrial organic material with a typical terrestrial carbon signature.

Fig. 8
figure 8

a PARASOUND acoustic section PS98-31071 showing the position and penetration of giant kasten corer PS51/92-12; b right inset indicates section track overview in the area (including nearby TRD-X S-011; see Fig. 10). c Stratigraphic length of PS51/92-12 and sedimentation rates based on AMS-dated shell material [4]. The geochemical and micropaleontological data including salinity reconstructions clearly demonstrate the stepwise change in depositional environment after ca. 9 ka [5]

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Transferring the seismic information, downcore data, and chronology of site PS51/92 to nearby HRS line S-011/15 supports our notion made above (Fig. 8) that the infilled depressions, which are so well stratified, must reflect a type of sediment that was deposited under terrestrial, permafrost conditions.

Interpretation

Permafrost produces a rapid increase in the acoustic velocity of the seismic signal. A number of field and laboratory studies have shown that the P-wave velocity of ice-bearing coarse-grained sediments is strongly dependent on the ice content. The theoretical seismic velocities of 2.5–2.8 km/s for sands with 0–40 % ice content and from 3.4 to as high as 4.35 km/s for 40–100 % ice in pore space were determined by Johansen et al. [14]. Modeling experiments have shown an average velocity in unfrozen sediment strata of ~1.4–1.8 km/s, whereas the acoustic velocity in permafrost and frozen sediments rises up to 3.0–4.5 km/s [35, 41, 42]. This all causes significant change in the acoustic impedance at the interface between frozen and unfrozen deposits. In the HRS data, it normally shows as a prominent high-amplitude reflector with positive polarity. Thus, the top of a permafrost stratum can be distinguished from seismic records as prominent positive reflector. Because most of the PARASOUND data from the central Laptev Sea revealed a strong reflector at depths of 2–20 mbsf, this reflector was interpreted as the top of subsea permafrost [17, 37, 39]. A similar technique was used in a number of other studies on subsea permafrost [7, 31, 38, 40, 41].

Using all the information together, a total of five distinct facies zones were mapped in the study area. These differ in geometry of the BR, reflection patterns, depths, and continuity of the reflectors (Fig. 7).

Facies zone A occurs in the center of the study area west of Semenovskoe shoal (Fig. 7) and has peculiar BR features (Fig. 2). The BR is identified as high-amplitude non-stratigraphic, i.e., post-sedimentary interface, which crosscuts the host reflectors and constrains a deeper penetration of the seismic signal. The hummocky topography of the BR within this zone is similar to the top of IC found in thermokarst-dominated terrains of the Yakutian lowlands [10, 11, 39, 50].

Therefore, we attribute this BR to the top of acoustically defined permafrost in the thermokarst-dominated terrain. As it was described earlier [50, 56], the thermokarst terrain was formed 13–12 ka and as a result of extensive thaw settlement of the top of the IC ice-rich deposits. Later on these features were filled with thawed structureless taberal deposits (i.e., permafrost sediments that thawed in a talik and then refroze). Modern remnants of such ice-rich deposits are ample on land, e.g., in the Lena Delta [25, 50–52]. At the beginning of the twentieth century, a few islands consisting of IC deposits still existed also on the southern Laptev Sea shelf [9, 15, 23]. These IC islands formed residual hills between the former branches of Lena and Yana paleoriver valleys and therefore were subject to intensive thermodenudation and wave erosion. Eventually they completely disappeared and turned into sandbanks with a modern water depth of ~5–8 m. The original bathymetric model, constructed by digitizing the large-scale nautical charts, provides new evidence for the existence of the IC remnants in the south of Laptev Sea. The pitted surface south of Semenovskoe shoal (Fig. 7) is supposed to be a bank formed recently at the place of the IC islands destroyed by the thermokarst processes.

The former existence of such IC remnants within the study area supports our assumption about the relation of the hummocky BR surface with the IC top. It also suggests that the deposits below the BR could be assigned to the Sartanian–Karginian IC deposits (correlative with MIS 3-2) of which the overlying sections (Fig. 2) are comprised of a fill sequence (uppermost Sartanian–early Holocene thermokarst deposits) and a marine sequence (middle and late Holocene transgressive deposits).

There seems to be a strong correlation between BR topography and “permafrost overhung” distribution, expressed in the development of a unified structure along the northwestern flanks of the BR depressions (Figs. 4, 5A). The basinward edges of the “permafrost overhung” are post-sedimentary boundaries, crosscutting, and partly blanking stratigraphic reflectors. This suggests that “permafrost overhung” resulted from bi-directional upward and downward freezing of lagoonal deposits. The occurring gas seeps mark zones of high sediment permeability, which are likely associated with taliks in the permafrost [39].

The narrow facies zone B is located northwestward of zone A (Fig. 7) and exhibits a fairly smooth topography of BR. It occurs at an average depth of 45 m below sea level. An ATU underlies the BR similarly to zone A, but the strength of this seismic boundary is slightly less. Thus, we suppose that the facies pattern within zone B is similar to those observed in facies zone A.

Facies zone C is outlined within Vasilievskaya and Semenovskaya banks and might be potentially found on similar shoals outside of the study area as well (Fig. 7). The sedimentary succession here differs strongly from those described above. Flat and diffused BR occurs at depths of 1–5 mbsf. An ATU wedges out at the boundary between A and B zones. Due to this the underlying semi-transparent unit appeared just below BR (Fig. 3). Based on the weak reflectivity of the BR and seismic signature comprising short seismic reflectors remnants, we assign the latter to a degraded ice-bearing permafrost within sandy deposits.

A correlative sedimentary succession was found in and near the Lena Delta [11, 50] where ancient ice-poor sandy sediments discordantly underlay the ice-rich Karginian–Sartanian IC. The former are assigned to the Muruktian ice-poor fluvial and/or alluvial sands [11, 25, 50]. However, reliable datings for this time interval [24, 50] are sparse and range from 88 to 37 ka. Based on this, the semi-transparent unit is considered to be pre-Karginian (pre-MIS-3, most probably Muruktian and uppermost Kazanian) ice-poor epigenetically frozen deposits [39].

Facies zone D comprises the hilly terrain in the northwestern part of the area (Figs. 7, 9). This zone is characterized by hummocky sea floor topography and shallow bedding of the BR. Significantly weak seismic penetration is caused by an extremely high reflectivity of the BR. The latter occurs just below the seafloor on the highs overlain by a very thin <2–3 m sediment veneer. In the depressions it dips down to 10–15 mbsf. The BR topography is similar to the thermokarst surface within facies zone A, but now exposed to the sea floor. The phenomena of the occurrence of subsea permafrost right below the sea floor might be explained by permanent tectonic uplift of this zone followed by persistent denudation of the upper sediments.

Fig. 9
figure 9

3D sketch of the PARASOUND lines from cruise ARK-XIV/1b [17] within the facies zone D. The hummocky on the seafloor is caused by the BR topography. For location see Fig. 1

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“Fuzzy” facies zone occurs within the Lena paleovalley (Fig. 7). Seismic records from this zone exhibit a chaotic acoustic image with an uneven, “fuzzy” base interface. Such a seismic signature may be caused by widespread subsurface gas discharge, which totally obscures the internal seismic structure. Spatial distribution of the “fuzzy” anomalies (Fig. 7) shows that they follow the ancient river valleys on the shelf. Taking into account the results of modeling [44] and geochemical evidence of methane venting [46] as well as the HRS data, we attribute them with a linearly scattered gas escape zones caused by river taliks.

To summarize, all the observations allow us to identify four seismic units correlative to regional sedimentary successions (Table 1). Acoustically semi-transparent deposits, related to polygenetic pre-Karginian (most probably Muruktian–uppermost Kazanian) ice-poor sandy deposits, occur at the base of the seismic section. Within zones A and B, they are discordantly overlain by acoustically transparent deposits (interpreted here as Karginian–Sartanian IC) and are strongly affected by thermokarst. These thermokarst depressions are filled with taberal sediments (probably of Sartanian age) and succeeded by early Holocene lagoonal deposits. The transformation of the thermokarst depressions into lagoons and the subsequent accumulation of lagoonal deposits began as soon as the advancing sea had reached the study area. The continuing sea level rise and, with it, the southward migration of the Lena River mouth eventually led to the deposition of the middle to late Holocene marine sequences.

Table 1 Overview of seismic features and interpretations
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The ploughmark incisions at the sea floor are the most recent features. According to Barnes and Reimnitz [1], such ice ploughmarks mainly form on Arctic shelves as a result of ice-scouring pack ice ridges in water depths between 10 and 50 m. Thus, the stratigraphic position of the buried ploughmarks may be indicative for the time when the transgressing sea reached the required water depth for their generation in the study area (Fig. 10).

Fig. 10
figure 10

Major features of environmental changes as identified within the HRS data set of seismic line S-011, nearby core site PS51/92 (see Fig. 8). Other acronyms: ATU acoustically transparent unit

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Paleoenvironmental reconstruction

It is quite obvious that a reliable paleoenvironmental reconstruction cannot be established using the seismic data only. A chronological attempt is therefore made to integrate the analyses of our HRS data with existing onshore paleoenvironmental information and conceptual models [11, 13, 24, 27, 44, 47, 48, 50, 57]. According to our stratigraphic sequence, we are able to distinguish between eight successive stages of offshore environmental evolution (see Fig. 11).

Fig. 11
figure 11

A schematic reconstruction of paleoenvironmental permafrost landscape changes over the eastern Laptev Sea shelf

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As is inferred from the HRS data showing the accumulation of the semi-transparent unit, the oldest stage of the landscape development may be as old as >80–37 ka (possibly uppermost Kazanian (?) to pre-Karginian/Muruktian). This unit may consist of epigenetically frozen marine deposits with syngenetically frozen terrestrial deposits on top (Fig. 11a).

During the following Karginian period (MIS 3), summer temperatures improved several times [13] causing thermoerosion of the sandy basements with only minor accumulation of syncryogenic deposits over the drained shelf. The Late Karginian (34–24 ka) was characterized by summer temperature still high enough for steppe species survival [13]. During the peak of the last glacial maximum, the Sartanian (24–15 ka), high aridity, and relatively low summer temperatures prevailed. Syngenetically frozen ice-rich deposits similar to those found onshore (Karginian–Sartanian IC) accumulated within terraces of the Lena and Yana paleovalleys and eventually formed acoustically transparent units (Fig. 11b).

During the first phase of deglaciation (~15–12.5 ka; Bølling/Allerød), extensive thermokarst processes are considered to be the leading landscape transformation factor [13], causing a rapid degradation of the IC landscape [44]. Thermokarst lakes occupied the recently formed depressions, and the lake water eventually accelerated thaw settlement rates. This led to the formation of a deeply dissected topography of the thermokarst terrain. The irregular BR surface marked this stage on the HRS records (Fig. 11c).

With the beginning of the Holocene the rising sea level led to the gradual inundation of most of the Laptev Sea shelf [3] and a southward retreat of coastlines and river mouths [26, 33, 54]. During this time of continuous retreat of shorelines and massive mobilization of terrestrial permafrost sediments on the shelf [28], thermokarst lakes and alases were transformed into lagoons. Fostered by high air temperatures in the Arctic [19] thermoerosion processes accelerated landscape leveling, transporting the deposits down the slopes where they accumulated in the nearby lake/alas depressions. This stage is presented on the HRS records as a well-stratified fill sequence, leaving a rather flattened topography (Fig. 11d).

According to the sea level reconstruction, the mid-shelf region with water depths ~35–40 m was flooded ~9.8–8 ka [3]. It provides the time constraint for the flooding of the TDR-X key site, including that of core PS51/92 (Fig. 10). The landward advance of the shoreline resulted in transformation of the onshore permafrost terrain into marine shoals accompanied by enhanced high-wave erosion (Fig. 11e). Minor positive relief forms were finally denudated, while lakes and lagoons were completely filled with sediments. On the seismic record, this geological event is reflected as a prominent top reflector (TR on the Fig. 2) and so typical for the central part of the study area.

Depending on water depth, the final stage of sea level rise (8–5 ka) was marked by modern shallow marine sedimentation developed (Fig. 10). Since no ploughmarks were observed on the HRS data within the lower part of the marine sequence (see Fig. 10), we suggest that water depth in the TDR-X key site did not exceed 10 m at 8 ka (Figs. 10, 11f). The sea level reached its modern position ~6–5 ka [3]. At that time shallow water stage F changed to marine stage G, providing typical marine depositional conditions over the study area (Figs. 8, 11g). As inferred from the HRS data, the transition from stage F to stage G is marked by frequent ploughmark activity (Fig. 11g).

Since then, thermal as well as sea-ice and wave-generated erosion caused a gradual disappearance of IC islands (Fig. 11h). Once the erosion front reached the top of the ice-poor sandy deposits, erosion rate significantly decreased and the former IC uplands were turned into subsea banks covered with sandy deposits.

Conclusions

Five seismic facies related to the evolution of subsea permafrost are documented using HRS data from the eastern Laptev Sea shelf. A prominent BR is interpreted as a top of acoustically identified permafrost. In places the topography of the BR bears resemblance with present-day onshore thermokarst terrain. Four seismic units inferred from the HRS data fit well with existing paleoenvironmental models for the region [11, 13, 24, 27, 44, 47, 48, 50, 57]. An acoustically semi-transparent unit at the base of the seismic sections may represent the pre-Karginian (most probably Muruktian–uppermost Kazanian) epigenetically and syngenetically frozen ice-poor sandy deposits. The latter are discordantly overlain by acoustically transparent deposits assigned as the Karginian–Sartanian ice-rich IC. The thermokarst depressions on the top of the IC are filled with lacustrine to lagoonal sediments concordantly overlain by well-stratified marine sequence.

The HRS data also revealed abundance of the gas seeps in the study area. Most of them mark the local permeable zones within the permafrost, which are most likely former thermokarst depressions (lakes/taliks). The “fuzzy”-facies of the gas seep anomalies are concentrated along the Lena and Yana paleoriver valleys and therefore may relate to river taliks.

Our seismic data also would indicate that the thermokarst terrain is exposed on the seafloor in the central part of the Laptev Sea shelf. This may originate either from the persistent denudation of the upper sediments due to the uplift of the region, or from a more recent destruction of formerly frozen sandy islands similar to Semenovsky and Vasilievsky.