Report of Activities on the RVIB N.B.
Palmer Cruise 02-04
The N.B. Palmer and the L.M.
Gould arrived at station 4 about
The work at station 3 in the
mid-afternoon consisted only of a pair of CTD casts. BIOMAPER-II was left in
the water and collected time-series data while the CTD casts were being done
and was then towyoed during the transit to station 3.
Work at this station, which was situated on the edge of the continental shelf
in water approximately 800 m deep, began with ice collection on a small floe
next the starboard side of the ship. The
presence of a long period swell with a ~1.5 m wave height and the lack of
consolidation of the floes in the area made it necessary to deploy a Zodiac
onto the floe for the ice collectors touse as a work platform. A single CTD cast was made to the sea floor
because CMiPS was being serviced and the water column
was too deep for the FRRF. An attempt was made to make a 10-m MOCNESS tow to
1000 m, but in the process of deployment, that electrical signal cable running
between the cable termination and the MOCNESS underwater unit was snagged and broken.
The tow was scrubbed because of the lateness of the hour and the time required
for the repair. Instead, BIOMAPER-II was
deployed and towyoed to station 1 approximately 12
miles away.
The weather on 1 September was
quite workable. The air temperature varied between -0.9ºC in the morning to -5ºC
in the evening. Barometric pressure dropped down from around 980 to 969.5 mb around
CTD Group report (Eileen
Hofmann, Bob Beardsley, Baris Salihoglu,
Chris MacKay, Francisco (
Today was a busy day for the CTD
group. We completed CTD casts at stations
4, 3, and 2 as we moved offshore along survey transect 1. At stations 4 and 3, two CTD casts were
done. The first was to 300 m for CMiPS sampling; the second included FRRF sampling in the
upper 100 m and extended to within a few meters of the bottom, which was at
about 340 m and 350 m, respectively.
Station 2 was at the shelf edge in 830 m of water. No FRRF sampling was done at this station, so
only a single cast was made to near the bottom.
The lowering speeds in the upper 200 m were appropriate for sampling
with CMiPS.
At station 4, surface waters were
just at freezing (-1.809ºC) and the well-mixed Winter Water layer extended to
60 m. Below this, temperature increased
to a maximum of 1.58ºC at 285 m, after which it again decreased to 1.42ºC at
the bottom. The salinity at the
temperature maximum was 34.70 and that at the bottom was 34.72.
At station 3, the surface waters
were above freezing at -1.78ºC. The well-mixed
Winter Water layer was the shallowest observed so far on the survey, extending
over the upper 50 m to 55 m of the water column. As observed at station 4, temperature
increased to a maximum of 1.58ºC at 255 m with a corresponding salinity of
34.70. Below this depth, temperature
decreased to 1.53ºC at the bottom. Bottom
salinity was 34.71. Water of 1.5ºC was
found from 217 m to the bottom, which results in a layer of
warm water that is almost 125 m thick.
This may be related to the warmer surface waters at this location. The data acquired from CMiPS
at this station, as well as at other locations, should help in understanding
how these water masses mix.
At the shelf edge (station 2), surface waters were colder than observed at the two previous shelf stations. The temperature in the upper 70 m was at the freezing point (-1.81ºC to -1.83ºC). Below this, temperature increased to 1.74ºC at 276 m and then decreased to 1.17ºC at the bottom. The corresponding salinity values were 34.67 and 34.72, respectively.
The thermohaline
structure observed at these three stations shows Upper and Lower Circumpolar
Deep Water at the shelf edge and on the continental shelf. The presence of Lower Circumpolar Deep Water
at station 2 is revealing because it suggests a relatively strong intrusion of
oceanic water onto the west
Sea Ice Observations (Chris Fritsen, Jenny Boc, Frank
Stewart, Sue Beardsley, Bob Beardsley, and
This is a preliminary analysis of
the ice observations taken over the past 24-plus hours starting on 31
August. During the transit from station
4 to station 1, we experienced a north to northwest swell running through the
ice pack. Hourly observations of the ice
conditions using standardized ASPeCT protocols
documented the gradient in ice conditions associated with the transit from deep
ice conditions to those nearer the ice edge and those imposed by the
swell. Specifically, there was a change
in the pack from that being dominated by 7 to 9 tenths coverage of first year
ice floes measuring 20 to 100 meters in diameter and 50 to 70 centimeters in
thickness near station 4 to small (5 to 10 meter in diameter) first year ice
floes measuring 30 to 50 cm in thickness at station 1. Brash and Shuga
appeared in the pack as we passed station 3 and continued to be present at 2 to
4 tenths coverage as we neared station 1.
The floes also became more rounded (indicative of prolonged exposure to
swell) compared to those inshore which had the rectangular shape, which is
indicative of recent swell-induced deformation.
Preliminary analysis also showed that weighted average thickness for the
undeformed ice floes changed from 50 cm to 25 cm over
the 60 nm distance. Such observations
when coupled with the Sea Surface Microwave Imager (SSMI) information should
allow better constraints on an ice budget for the region.
Seabirds (Chris Ribic and Erik Chapman)
The seabird and Crabeater seal
survey was conducted for almost six-and-a-half hours on 1 September as the ship
moved offshore between stations 4 and 2 on the northern-most line of the study
grid. Ice conditions were mainly 6 m
diameter first-year cake ice separated by small cracks of open water. A 0.5 m swell continued to run through the ice,
and the ship passed by several large ice-bergs, each associated with small
areas of open water.
The seabird species assemblage
was similar to that observed yesterday. We
continued to record relatively large numbers of Antarctic and Snow Petrels
milling over leads. A single Kelp Gull
followed the ship for much of the morning, periodically leaving the ship to fly
over water immediately adjacent to nearby icebergs. Two Southern Fulmars were recorded flying
directionally offshore, toward the ice edge.
Five Southern Giant Petrels were recorded in the survey, more than have
been observed on any previous day.
Twenty-four Adélie Penguins were
observed in several small groups. The Adélies appeared to be concentrated in a large area covered
by thin, gray, slushy ice that covered an old lead. They were less common in the larger,
snow-covered cake floes that covered most of the survey area. However,
two Emperor Penguins, including a juvenile, were observed in the cake ice.
A summary of the birds and marine
mammals observed on 1 September (YD 244) during 6 hours, 26 minutes of survey
time as the ship traveled between stations 4, 3, and 2 is the following:
Species (common name) |
Species (scientific name) |
Number observed |
Snow Petrel |
Pagodroma nivea |
23 |
Antarctic Petrel |
Thalassoica |
35 |
Southern Fulmar |
Fulmarus glacialoides |
2 |
Kelp Gull |
Laru dominicanus |
1 |
Southern Giant Petrel |
Macronectes giganteus |
5 |
Adélie Penguin |
Pygoscelis adelii |
24 |
Emperor Penguin |
Aptenodytes forsteri |
2 |
MOCNESS Report (Phil Alatalo, Peter Wiebe, Dicky
Allison, Ryan Dorland, Scott Gallager, Gareth Lawson)
Tow #10 for the 1 m2
net took place at Station 4 at 0700 on 4 September. Towing conditions at the
station were conducive for another successful tow in water 351 m deep. Biomass
of the nets matched the acoustic scattering seen on the Simrad
echo-sounder: peaks at 300-325 m and again between 75 and 25 m. Taxonomic
composition of these layers showed copepods in the deep layer and krill
dominating the upper water column. Abundant radiolarians were found at all
depths.
A high biomass was obtained from
net 0, which consisted mainly of copepods, euphausiids,
chaetognaths, ctenophores, and salps.
The high biomass of the deep net (325-300 m) was composed of chaetognaths, ostracods,
amphipods, and a siphonophore in addition to
copepods. Biomass dropped off
dramatically between 300 and 200, with chaetognaths and
smaller copepods replacing the large Paraeuchaeta sp. found in net 1. Between 200 and 100 m, a low biomass, high
diversity composition prevailed: siphonophores, pteropods, ostracods, amphipods,
and tomopterid worms.
Thysanoessa
(all stages) and occasionally E. superba
krill increased in number, peaking between 75 and 25 m. Of note was the low
number of copepods above 100 m. Pteropods, siphonophores, and a large
(6 cm) ctenophore made up the remainder of the shallow depth samples.
BIOMAPER II group report
(Gareth Lawson, Peter Wiebe, Scott Gallager, Phil Alatalo, Dicky Allison, Alec
Scott)
After a two-day hiatus from
towing the BIOMAPER II while we assisted the Gould in reaching its next position, on September 1 we recommenced
our broad-scale survey with a long towyo between
stations 4 and 2 along the northernmost of our survey transects. Scattering was
extremely low throughout most of the water column. A very diffuse shallow
scattering layer was present centered at 25 m and between 75 and 125 m we
observed occasional enhancements in scattering levels. At station 3, we kept
the BIOMAPER II in the water while a CTD was conducted. Further processing of
the acoustic data we collected while stationary should allow us to track
individual animals that moved through our sound beams. This should then allow us to make inferences
about the behavior of these animals.
As has been the case in many of our previous tows, VPR observations suggested that the plankton community in the upper 100 m of the water column was diverse and composed of diatoms, copepods (including calanoids), larvaceans, medusae, and radiolarians. Of these, diatoms were among the most abundant, particularly shallower than 50 m. We also made numerous observations of small krill, mostly associated with the weak layers that were evident acoustically. Individual images were also positively identified as a ctenophore, a pteropod, and a salp. At 1730, our VPR image-capturing was rudely interrupted when the strobe lens came loose. We thus had to finish the last two hours of the towyo without the benefit of any VPR data. Thankfully, repairing the lens was a simple task once the BIOMAPER II was back on board.
For the entire duration of the towyo, there was a strong scattering layer associated with
the bottom (325 m), extending 40 to 55 m above the bottom. Soon after the start
of the transect, a particularly intense region of
scattering developed right next to the bottom within this overall layer. Just
before sunset (1645), this intense region migrated from its position next to
the bottom to the top of the layer, 55 m above bottom.
As we've described in previous
reports, during much of this cruise we have been beset by problems with the
BIOMAPER II not flying perfectly level, and the associated problem of our
up-looking transducers occasionally receiving echoes reflected from the tow
cable. While we were in transit with the Gould,
we took advantage of the time on our hands to address these issues. Stian Alesandrini, one of our very
capable marine technicians, flattened out a bend that had developed in the towbail that attaches the tow cable to the BIOMAPER II. We
believe that this bend might have been the root of our problems. Thus far, straightening the bend appears to
have done a great deal towards keeping the towbody
flying level and keeping the tow cable out of the line of sight of the
transducers.
Current Position and
Conditions
Offshore stations take
considerable time to complete because of the very deep water depths (~3000 m)
and the time it takes to deploy the CTD to the sea floor or the net systems to
1000 m. Thus, we are now at the second station of the day (13), having just
started to work. Our current position at
2133 on 2 September is -66º 01.660′S; -71º 10.325′W. The air temperature is -5.1ºC and the
barometric pressure is 1002.1 mb and leveling
off. Winds are moderate at around 13 kts out of the west-southwest (240). Skies are partly
cloudy and visibility is good. The pack
ice is made up of small floes that are easy to work in. A low-amplitude long-period swell is running
through the region.
Cheers, Peter