Report of Activities
on the RVIB N.B. Palmer Cruise 02-02
6 May 2002
May 6 was a day of transition for the continental shelf
waters off of
The 6th of May was also notable for the remarkably clear
skies that stayed the day. Although
early morning found the Palmer some
60 nm from land, the mountains of
Work was completed at broad-scale survey stations 78, 79, 80
and 81 including 4 CTDs, an ice collection at station
78 and a 1-m ring net tow at station 80.
BIOMAPER-II was in for transits between the all of the stations. Seabird
and marine mammal surveys took place during the daylight period and two sonobuoys were deployed during the transit between stations
79 and 80.
CTD Group report (John Klinck, Tim Boyer, Chris Mackay,
Julian Ashford, Andres Sepulveda, Kristin Cobb)
The CTD group did four casts today at the outer shelf and
over the slope. The mixed layer at all casts was variable reflecting the
changing ice cover and varying, although, weak winds. The two deep stations were typical of other
casts in the ACC. The two shelf stations
were typical of stations in the southern part of the grid with no indication of
recent influence of oceanic intrusions.
Station 78 (cast 81, 488 m). There
was a uniform mixed layer to 50 m (-1.75ēC, 33.5 psu,
0.07 ug/l chlorophyll) and a relic Winter Water (WW) layer
centered at 100 m. Energetic temperature
reversals occurred from 100 to 150 m. The bottom temperature was 1.3ēC with no
temperature maximum.
Station 79 (cast 82, 427 m). A
uniform mixed layer occurred to 30 m (-1.8ēC, 33.45 psu,
0.1 ug/l chlorophyll) with two deeper uniform temperature
layers below (75 to 125 m and 140 to 160 m).
The temperature maximum (1.4ēC) was at 350 m.
Station 80 (cast 83, 2009 m). The surface layer had increasing temperature
and salinity to 50 m and a relic WW layer was centered at 80 m. The temperature maximum (1.8ēC) was at 250 m
and a cold layer, with lower salinity was at 550 m. Temperature declined with depth to the bottom.
Station 81 (cast 84, 1176 m). A uniform
mixed layer went to 70 m (-1.8ēC, 33.8 psu, 0.2 ug/l chlorophyll). A
second uniform temperature layer extended to 100 m. Some small-scale variability was present in
the pycnocline.
The temperature maximum (1.8ēC) was at 250 m and temperature declined
from there with depth to the bottom.
Marine Mammal report (Debra Glasgow)
The sun rose this morning at 0957 on 6 May to a colorful
pancake ice coated ocean with an air temperature of -7.8ēC. The mountains of
Sea Birds (Erik Chapman and Matthew Becker)
Observations were made today, May 6, as the ship transited
off the shelf break south of
Snow Petrels were observed in high densities throughout the
survey. A small number of Antarctic
Petrels were also seen, but in much lower numbers. The Snow Petrels appeared to be drawn to the
ship from nearby leads, and between 20 and 40 birds were recorded as followers
throughout the day. As the ship left the
pancake ice and entered grease ice, the followers remained, and they were
continually joined by additional birds.
Clearly, this is a particularly attractive habitat for Snow Petrels. Surveys in similar ice concentrations
elsewhere on the grid have not indicated high Snow Petrel numbers. However, previous surveys in ice have been in
areas with year-old ice floes, and the differences in petrel abundance may
reflect differing biology between the under-ice zooplankton community
associated with new ice and that associated with year-old ice. It will be
interesting to look at results from surface ring net and MOCNESS tows to see if
these sampling efforts indicate a difference in surface zooplankton communities
associated with these two ice types.
A night survey was conducted in the late evening as we headed toward station 81. We had again entered light pancake ice with about 7/10 coverage, however Snow Petrel numbers had dropped significantly, with only a handful of birds around the ship. While some birds are perhaps attracted to the NPB's spotlights as the ship scans for icebergs, we witnessed repeated feeding behaviors in the dark water off the portside. Feeding consisted of the birds hovering just above the surface (facing into the wind) and making repeated dips into the water with their bill, without actually landing on the surface. Presumably, this unknown prey item existed in high numbers locally, as the petrels were observed making as many as ten feeding attempts in one sequence (due to the winds, subsequent water conditions, and methodical feeding behavior it seems unlikely that these attempts constituted repeated aggressive pursuits of a single prey item). How the birds are able to discern their prey in near total darkness is unknown. In addition, why such feeding behavior was not observed during the day, and why the numbers of snow petrels dropped off so dramatically at night is unknown, but probably concerns changes in prey distributions and abundance. It is possible that the birds observed feeding at night had encountered a very localized nocturnal migration of zooplankton in the water column. Some of these zooplankton species are capable of bioluminescence, which might be an easily discernable trait on the water's surface to the well-trained avian eye.
A summary of the species and number of individuals of birds
and seals within the 300 m transect during 4 hours, 47 minutes of daytime
surveys between consecutive stations 78 and 80 is the following:
Species (common
name) |
Species (scientific
name) |
Number observed |
Snow Petrel |
Pagodroma nivea |
179 |
Antarctic Petrel |
Thalassoica Antarctica |
12 |
Southern Giant Petrel |
Macronectes giganteus |
1 |
Water Sampling for Microzooplankton
(Phil Alatalo)
Survey Line 8 began in George VI Sound in very thick ice.
Surface samples at Stations 56 and 57 were characterized by dense numbers of particles,
Mesodinium,
small diatoms, and large ciliates.
Particle abundance decreased as the survey progressed out of
Along the shelf, at stations 60 through 63, tintinnids and ciliates became more common as did the
diatom, Corethron. Here, the water surface was free of ice. Mesodinium continued to be restricted to surface
waters. Ciliate protozoans
were present at all three depths sampled at Station 62.
In deeper waters, diatoms (Chaetoceras, Corethron, Nitzschia,
Rhizosolenia spp) were
common in surface waters, along with the ciliate, Mesodinium. This agrees with the
increased chlorophyll values (0.3-0.4 ug chl/l) reported by the CTD group. Particle abundance and motility declined
sharply in the pyncnocline at Station 66, but further
offshore, assemblages similar to the surface were present as deep as 200 m at Stations
68 and 70.
Zooplankton (MOCNESS/BIOMAPER-II) report (Carin Ashjian, Peter Wiebe)
No MOCNESS tow was taken during 6 May
BIOMAPER-II was towyoed along the
survey tracklines on 6 May beginning at mid-shelf
station 78 and running out to shelf-break station 80 at the end of survey line
10 and then over to station 81, another shelf-break station on the seaward end
of survey line 11. During the transit along the mid-shelf region, there were
regions of strong scattering from 30 to 60 m depth and varying from 60 to 100 m
in vertical extent, then grading into lower backscatter at greater depths.
There were occasional very intense patches of backscatter in this depth
zone. Further out on the shelf between
stations 78 and 79, there was low scattering throughout the mixed layer, a
horizontal layer in the upper pycnocline, a zone of very
low scattering at mid-water depths, and a zone of higher backscattering
starting at the bottom, which was around 500 m, and extending up about 200
m. Intense small targets periodically
appeared in the mixed layer. Towards the end of this transit, thin layers developed
in a double pycnocline structure that was present.
On the run to the end of the line (station 80), there was
light backscattering throughout the water column with isolated discrete targets
at various depths. About this time, there were observations of whales making
deep dives near an iceberg. Steaming along the shelf break from station 80 to
81, the deep scattering layer became somewhat stronger for a time, but
scattering was low near the surface and in the pycnocline
around 65 m.
Cheers, Peter