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SUPPLEMENTARY INFORMATIONDOI: 10.1038/NGEO2007
Ebullition and storm-induced methane release from the East Siberian Arctic Shelf
Shakhova et al. Ebullition and storm-induced methane release from the East Siberian Arctic Shelf
1
SUPPLEMENTARY INFORMATION
Contents
Supplementary Figures S1-7
FigureS1.jpg: Snapshots of the winter drilling campaign performed in the study area in
April 2011 (238 KB)
FigureS2.jpg: Primary structural elements of the Laptev Rift System (166 KB)
FigureS3.jpg: Laboratory Delta-T calibration data (208 KB)
FigureS4.jpg: Seep plume class occurrence in the study area (summer 2009) (148 KB)
FigureS5.jpg: Summer 2009 sonar data from the study area (179 KB)
FigureS6.jpg: Best estimate contribution of each seep class to total flux in the study area.
(214 KB)
Figure S7.jpg: Data from in-situ bubble observations made in the study area (340 KB)
Supplementary Methods
This supplement contains detailed information on the sampling campaigns and data
processing and analysis, a description of modeling assumptions used to simulate the
current state of subsea permafrost in the coastal area of the ESAS, and details about the
sonar data acquisition and analysis used for estimating ebullition-induced flux in the
study area based on seep classification and apportioning the contribution of each seep
class to the total flux in the study area.
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1. Supplementary Methods
1.1. Estimation of population parameters using the maximum likelihood (ML) method41.
The best fitting function to describe data sets is a lognormal distribution. The maximum
likelihood estimates of the mean (m*) and variance (s*2) were calculated using equations (1)
and (2), respectively:
(1)
where n is the number of observations and xi is the methane (CH4) concentration, and
(2)
The parameters m* and s*2 were then used to estimate the arithmetic mean and median of the
lognormal distribution. For a lognormally-distributed population, the arithmetic mean (a) was
estimated by
(3)
From the definition of the arithmetic mean of a lognormal distribution, this value is always
greater than zero, guaranteeing that confidence interval estimates are always positive. This is a
major advantage compared to the confidence intervals of a normal mean, where, in contrast,
the lower bound of the confidence interval can be assigned a nonsensical negative value.
Because of the positive skewness of the lognormal distribution, the confidence interval of a
lognormal arithmetic mean is also skewed positively. The median of lognormally distributed
datasets was estimated by: *mex � (4)
1.2. Quantifying the dissolved CH4 concentration in the water column.
Conductivity/temperature/depth (CTD) profiles and water samples were collected with Niskin
bottles during upcasts at a series of stations. For CH4 measurements, water samples were
drawn immediately from Niskin bottles into replicate 500-ml glass bottles, overfilling 1.5-2
times with sample water. Sub-sampling was done carefully to avoid introducing air bubbles.
Bottles were sealed with silicon stoppers and metallic crimps. In the first analytical step of the
headspace technique, part of the bottle sample water was replaced with helium. Then, samples
were placed in a thermostatic water-bath shaker and the dissolved and gaseous phases were
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equilibrated for 30 minutes. The replicate samples were kept at ambient laboratory temperature
and analyzed within a few hours. CH4 concentrations were measured with a MicroTech-8160
gas chromatograph (GC) using a flame ionization detector (FID) with a helium carrier gas. The
GC analysis was isothermal (40˚C) and the maximum FID temperature was held at ≈250˚C.
Calibration used certified CH4 gas standards in a balance of air (Air Liquide, USA). The
standard deviation of duplicate analyses (3-5 replicates) was less than 2% and GC precision
was 1%. The concentration of dissolved CH4 in the water samples was calculated with the
Bunsen solubility coefficient for CH4 at the appropriate equilibration temperature using the
fit42:
� �2321321 )100/()100/()100/ln()/100(ln TBTBBSTATAA ������� (5)
where β is the Bunsen solubility coefficient, T is temperature in degrees Kelvin, and S is the
salinity in per mil. Calculated data were analyzed statistically with the Statistics 7.0 and Matlab
7.0 software packages. For graphical representation of horizontal surfaces, irregularly-spaced
data were interpolated onto uniform grids (using Krieging algorithms), allowing an area-
weighted mean to be calculated. Topographic plots of vertical profiles were generated by
mapping the irregularly-spaced station data using a minimum-curvature algorithm (Surfer 8.0).
1.3. CH4 mixing ratio in the atmosphere. CH4 concentrations were measured with a pre-
calibrated (by manufacturer) high-accuracy fast CH4 analyzer (HAFMA, DLT-100; response
time: <0.05 seconds; accuracy: better than 1% of reading; concentration range: 0.01-25ppmv;
www.lgrinc.com) at 10-12 Hz; two sonic anemometers (CSAT3, Campbell Scientific Inc.)
measured the 3D wind vector and sonic temperature; a Li-Cor 1400 meteorological station
measured wind speed and direction, moisture, and temperature; and a Li-Cor 7500 open path
infrared gas analyzer measured H2O and CO2. Other instruments included a pressure transducer
(PTB 101, Vaisala) and a motion package (NAV440, Crossbow) that measured all 6
components of ship motion and the 3 components of acceleration, magnetic field, and position.
The package was mounted on a meteorological mast affixed to the vessel’s bow at 10-12 m
height.
1.4. Drilling of subsea permafrost from the fast ice. A heavy drilling technique was used for
drilling the subsea permafrost in the study area in April 2011. Fieldwork was accomplished
through the use of an equipment caravan which traveled over the sea ice to the drilling location
(Supplementary Fig. S1). The drilling rig, well tubes, boring casing, and additional equipment
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(including equipment for geochemical and microbial measurements) was delivered to Tiksi by
two cargo air freighters (AN-12s). The drilling was performed using a drilling rig (URB-2A-2)
with a hydraulic rotary-pressure mechanism operating without drilling fluid. Well tubes and
borehole casing 4 m long and 147 mm in diameter were used to preserve an undisturbed core
structure and prevent sea water infiltration. After extraction from the borehole the sediment
core was cleaned and generally described as frozen or unfrozen and including or not including
ice structures, debris, organic layers, and grain-size variations.
1.5. Thermal measurements in the boreholes. Temperature in each borehole was
measured 3 days after drilling using a chain of calibrated thermistors, according to the
Global Terrestrial Network for Permafrost (GTN-P) protocol (http://www.gtn-p.org). A
temperature logger (HOBO Temp PRO V2) was installed in the head of the probe,
allowing the temperature gradient within the frozen and unfrozen layers of both Holocene
marine sediments and Pleistocene permafrost deposits to be documented. The obtained data
was used in the model to constrain permafrost geophysical features.
1.6. Sea water temperature measurements. A pre-calibrated shipboard CTD sond attached to
a large metal rosette wheel was used to monitor variation of water temperature, salinity, and
density. Temperature of sea water at different water horizons was measured by lowering the
rosette on a cable down to the seafloor, and observing the water properties in real time via a
conducting cable connecting the CTD sond to a computer on the ship. A standard CTD sond
cast was performed at each of 570 oceanographic stations.
1.7. Modeling subsea permafrost in the study area. A modification of the model that has
been described in detail13 was performed as a case study. Recently obtained data on
temperature dynamics of bottom water during the last 14 years (1999-2012) were employed to
update the historical data set and to determine the thermodynamic state of sediments over
decadal and multi-decadal time scales. Thermal conductivity and the heat capacity of the
ground material were parameterized as functions of ice, liquid water, and salt concentration
(values of key parameters established from field data for the studied area). The thermodynamic
model was forced by seawater temperature dynamics computed by global circulation models
(GCMs). Since GCMs provide coarse-resolution temperature dynamics, we incorporated local
seawater warming effects. We used a 1-D realization of the thermodynamic model (the size of
a computational domain is 100 meters). The initial temperature distribution was set to
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measured values collected during drilling. To compute temperature dynamics at sites within
tectonics fault zones we utilized a 2-D realization of the thermodynamic model, which allows
the formation and evolution of an open talik to be simulated. The computational domain and
heat fluxes at its boundaries were determined as described13.
1.8. Sonar data acquisition and analysis. A 260 kHz 8-bit Imagenex Delta-T multibeam
sonar was used for the surveys because of its portability (shipped via aircraft carry-on
luggage), its durability (no moving parts, sensitive power transformers, or external beam-
forming computers), and ability to be run by a laptop computer. The system continuously
recorded water-column returns for all beams during the entire survey. The Delta-T has 120
across-track beams by 3 degree along-track swaths; beams were formed in real time and in
post-processing. One advantage of multibeam sonar data over single beam data for plume
characterization is that the plume geometry relative to the beam swath is precisely known, and
thus bubble plumes cannot be lost due to missing the beam, as is illustrated in sonar lander data
for the study area shown in Fig. 1b. These data show bubble plumes extending to near the sea
surface. Boat-based survey data reveal similar details (Fig. S6).
A lab calibration experiment with the Delta-T confirmed a positive correlation between
summed sonar return and bubble plume gas volume (Fig. S7). These data were collected by
rotating the sonar around a vertical axis in a 5-m-deep tank at a range of 6 m from a flow-
controlled air bubble plume. In this orientation, the sonar swath extended from below the tank
floor to above the water surface such that the long axis of the swath was parallel to the bubble
plume. Fig. S7 shows summed sonar returns from four rotations across the air bubble plume for
four flows. These data demonstrate that Delta T sonar returns are strongly sensitive to bubble
plume emission strengths. However, note the increase in sonar return with height above tank
bottom, even though the total number of plume bubbles remains approximately constant,
because hydrostatic pressure decreases are minimal and dissolution negligible. This signifies
complexity in the relationship between bubble plume spatial density and bubble size and the
return signal, preventing simple calibration. Thus, sonar return strength absent additional
information is only a quasi-quantitative value.
For the survey, a sonar pole-mount was fabricated such that the transducer head was
fixed 1 m below the sea surface amidships on the starboard gunwale and directed ~20 degrees
forward of vertical with the swath extending 60 degrees orthogonal to the boat’s direction of
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travel. This orientation improved the data by enabling easy discrimination between seeps and
electrical noise (noise is along-beam, which is tilted from vertical, while seeps rise vertically),
reduction of seabed return signal, and increased pings per seep plume.
Water-column multibeam sonar data were recorded throughout the survey as pings of raw
sonar return for 120 beams with 500 samples per beam regardless of range. This coordinate
system (range vs. beam angle, theta) is referred to as “R-Theta” space. Sonar returns were
normalized for acquisition gain to facilitate comparison across different data blocks. Sonar data
acquisition recorded 157 survey lines of variable duration that were imported from the
Imagenex Delta-T data files in intervals of 6000 sequential pings, hereafter referred to as
“blocks.” A total of 1178 blocks were created, representing between 100 m and 3175 m of
linear “along-track” survey distance. The mean length of the blocks was ~1600 m. Blocks were
subdivided into 200 m along-track intervals termed “sub-blocks”; a total of 8203 sub-blocks
were analyzed. Sub-blocks were filtered for erroneous pings and processed in R-Theta space.
Each block was manually inspected and assigned a density class and intensity class.
Conversion to a flux involved assigning a representative flux to each intensity class; this
process focused on several plume characteristics visible in the sonar data, including
persistence, spreading rate, and “clumpiness.” “Clumpiness” is the well-known tendency for
bubbles to aggregate in persistent groups from a few centimeters to half a meter in size19. This
estimation was based on saltwater laboratory experiments for bubbles from a sand and seashell
sediment bed over a range of different bubble fluxes. These laboratory experiments confirmed
a strong sensitivity of appearance to flux, in agreement with previous field measurement data
of natural marine hydrocarbon seep bubbles18,31 and laboratory data32 and showed that bubble
plume appearance in video and multibeam is strongly sensitive to flux.
Each data block was classified by two characteristics: spatial concentration of seeps, d,
which characterized spatial density, and the largest seep, which served as a proxy for seep
intensity. Spatial density equaled the number of seeps per sub-block averaged over the data
block. Seep density classes were d1: ~1-2.9 seeps, d2: ~3-4.9 seeps, d3: ~5-9.9 seeps, d4: ~10-
19 seeps, d5: ~20-39 seeps, and d6: ≥40 seeps (×10-4 m-2). Seep intensity classes were i1: short
clumps of bubbles, i2: bubble pulses that were >50% active, i3: thin continuous bubble
streams, and i4: thick continuous bubble streams (Supplementary Table S1). The magnitude of
sonar return integrated over the spatial domain was generally stronger for plume classes i3 and
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i4 than for i1 or i2. These classes are further described below. All block data with some
seepage exhibited examples of the smallest intensity seep class, i1. Therefore, the intensity
classification is the upper end of the range of seep intensities within each data block. Values of
seepage spatial density, d, were corrected for approximate sonar swath width (based on range
to seabed) to an area-corrected spatial density, D (seep number per km2).
Due to the large number of sonar blocks analyzed (8203) the number of seeps in each
class is well characterized except for the smallest, where misclassification of noise could lead
to an undercount. Fortunately, the contribution of the smallest intensity class was not dominant.
However, there is significant uncertainty in the flux assignment for each intensity class which
was addressed by estimating maximum likely limits that the flux classification probability
could be biased towards larger or smaller classes (Supplementary Table S1, calculations B and
C) or that the dominant bubble size could be different, while still maintaining the same bubble
plume appearance. Plume misclassification could have led to biases in the intensity
classification scheme, resulting in undercounting or overcounting in each of the classes with a
maximum likely shift of 30% assumed, but note that bias was not assumed to preserve the
number of plumes. Also note that the repeatability of the classification approach was tested by
repeating some of the analyses which were found to agree with the initial analysis to better than
10%, so 30% is a conservative limit on error bias. This caused a much smaller uncertainty of
about 10-25%. Shifts in bubble size were assumed to conserve the number of observed bubble
plumes. In these cases, the driving factor for the uncertainty limits used in this uncertainty
assessment was the results of laboratory experiments in which the levels were chosen because
larger uncertainties/biases would change the characteristics of the sonar images of the bubble
plumes in the data and thus would be apparent in the data. These maximum uncertainty limits
were then averaged to estimate the total flux in a range of 0.99 x102 to 6.3 x102 mg m-2 d-1.
1.9. Ebullition-induced flux estimates in the study area.
The probability of each class was determined for all datablocks in the study area and
found to be 43%, 29%, 25%, and 4% for intensity classes i1, i2, i3, and i4, respectively. The
probability of each class up to the highest seep class observed in the segment was calculated
for all data blocks in the study area, covering 32 km of linear tracks. Emission rates were then
calculated per square meter based on each segment’s along-track distance and swath width.
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Plume occurrence rates were 2.16×10-3, 8.56×10-4, 2.9×10-4, and 4.09×10-6 plumes m-2 for seep
classes i1, i2, i3, and i4, respectively (Fig. S5).
An effort then was made to assign a flux to each seep plume classification. Based on
experience with bubble observations and emission modes, best estimate bubble emission rates
of 3, 15, 25, and 100 bubbles s-1 per plume were assigned to density class i1, i2, i3, and i4,
respectively. Using an average bubble size of 3700 µm equivalent spherical radius based on
video bubble images obtained in 2012 (Fig. S7), seep density classes i1, i2, i3, and i4
correspond to emissions of 0.7, 3.3, 5.5, and 22 cm3 s-1, respectively. Combining seep plume
occurrences and seep plume emission rates yields a best estimate total seabed flux of ~290 mg
m-2 d-1. There are a number of significant uncertainties in these estimates, including bubble
size, seep plume bubble rates, and how representative the seep plume probabilities are (Fig.
S5).
References:
41. Jonsson, A., Gustafsson, O., Axelman, J., Suindberg, H. Global accounting of PCBs in the
continental shelf sediments. Environ. Sci. Technol. 37, 245 (2003).
42. Wiesenburg, D.A., Guinasso, N.L. Equilibrium solubility of methane, carbon monoxide,
and hydrogen in water and seawater. J. Chem. Eng. Data 24(4), 356 (1979).
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