Report of Activities
on the RVIB N.B. Palmer Cruise 02-02
On April 24, the broad-scale survey was conducted along the
inner and central area of
Winds were generally light to moderate - around 10 to 12 kts out of the east in the morning and 15 to 18 kts out of the north in the afternoon. The barometric
pressure was 983.7 mlb in mid-afternoon, up from
974.5 mlb around 0200. The air temperature ranged from -2.1ºC to 0.9ºC,
and in the afternoon, the sea surface temperature was near the freezing mark at
-1.693ºC and the salinity was 33.977 psu. On the trackline between stations, the ship steamed through a
mixture of b rash ice, large pancakes, and larger slabs of much thicker
year-old ice. Much of the new ice had a
golden greenish brown color indicating lots of algae and microzooplankton
were present in it in contrast to the year old slabs that were a purer white.
During the steam from station 40 to 41, the pack ice ended and station 41, at
the entrance to
During this day, work was completed at stations 38, 39, 40
and started at station 41. Three CTDs were made, a MOCNESS tow was made at station 40, an
APOP cast was made at station 41, and an ice collection was made at station 40.
Seabird and mammal surveys were conducted along the transits between stations
during daylight, and BIOMAPER-II was towyoed between
stations 38, 39, 40 and 41. Two Sonobuoys were deployed
along the survey trackline to record marine mammal calls.
CTD Group report (John Klinck, Tim Boyer, Chris Mackay,
Julian Ashford, Andres Sepulveda, Kristin Cobb)
The CTD group did three casts today in the center of
Station 38 (cast 42, 188 m). There
was a uniform surface layer to 45 m. Surface chlorophyll was 0.4 μg/l. There were thick layers (10-15 m) in pycnocline. No double diffusive variability was evident.
There was a steady increase of temperature and salinity to the bottom.
Station 39 (cast 43, 405 m). The surface layer went to 50 m with density
increasing with depth, but the temperature was about -1.8ºC. The surface chlorophyll was 0.6 μg/l declining to 0.3 at the
bottom of the mixed layer. The
Winter Water (WW) layer (30 m thick) was centered at 90 m. and the pycnocline extended from 100 to 250 m with little small
scale structure. There was no deep
temperature maximum. The bottom temp was 1.2ºC.
Station 40 (cast 44, 635 m). There
was a thin (15 m), cold (-1.7ºC) surface layer and increasing temperature and salinity
to the top of the pycnocline at 120 m. The surface chlorophyll was 0.5 μg/l declining to 0.15 at 30 m
and on down to detection limits at the top of the pycnocline. A few thin layers (2-4 m) occurred in the pycnocline. The deep
temperature was 1.3ºC, but there was no temperature maximum.
Marine Mammal report (Debra Glasgow)
The marine mammal survey began on 24 April at 0835 on the
transit to station 40 in overcast conditions and in 9/10 young discoloured brown ice. Three Adélie penguins were seen at
0850, which proved to be the most exciting event for the d ay as no cetaceans
were sighted. Few birds were recorded for the day, however. While stopped at station
40, Erik Chapman sighted a crabeater seal hauling out on the ice and I recorded
2 seals three nautical miles away but could not identify them at that distance.
These were the only sightings of the day.
Marine Mammal passive listening report (Ana Sirovic)
A total of 11 sonobuoys were
deployed during the six day period 19 to 24 April, all omnidirectional. April 19 and 20 were spent surveying the
outer shelf and shelf break. They were
busy days with multiple whale sightings and sonobuoys
were deployed after the sightings. Blue
whale calls were heard on all 4 sonobuoys deployed
and humpback calls (most likely a song) were recorded on 3 of the buoys. I also heard an interesting non-biological
noise on one of the buoys: a fairly loud earthquake. This occurred at 2234 on April 20. Unfortunately, I did not have a directional sonobuoy out at this time, so I could not determine the
location of the earthquake.
April 21 was a stormy day with decks closed for most of the
day during which just 1 sonobuoy was deployed. Again blue whale calls were recorded, but
there were also low-frequency (20-50 Hz) up-sweeps that were most likely of
biological origin. Unfortunately, I
don't know what animal could have made that noise.
April 22-24 were spent near to or inside
Sea Birds (Erik Chapman and Matthew Becker)
Seabirds were surveyed between stations 39 and 41 on 24
April for almost 4 hours in excellent observing conditions. We were well within
A summary of the species and number of individuals of birds
and seals observed during 3 hours, 47 minutes of daytime surveys between
consecutive stations 39 to 41 is the following:
Species (common name) |
Species (scientific name) |
Number observed |
Southern Fulmar |
Fulmarus glacialoides |
13 |
Antarctic Petrel |
Thalassoica |
16 |
Snow Petrel |
Pagodroma nivea |
36 |
Southern Giant Petrel |
Macronectes giganteus |
1 |
Kelp Gull |
Larus dominicanus |
2 |
Material Properties of Zooplankton Report (Dezang Chu, Peter Wiebe)
On 24 April en route from station 39 (68 41.238ºS, 67 59.760ºW)
to station 40 (68 28.890ºS, 68 47.940ºW), the measurements of sound speed
contrast on 7 big red amphipods (tentatively Eusirus) were repeated. Three
animals out of seven were dead at the start of the experiment (in the previous
day, there was one dead animal). This time there were no visible bubbles attached
to the exoskeleton during the measurements. The sound speed contrast was 1.0383
as compared to the value of 1.096 obtained in the previous day. This result may
be due to the presence of the mixture of alive and dead individuals or because
of unseen bubbles in the first experiment. More experiments are needed to
resolve this issue. The density contrast
was 1.051, heavier than krill we had measured so far on this cruise.
At station 41 (68 16.320ºS, 69 35.280ºW), an APOP cast was
done in the same way as the previous casts. At the end of the cast, we found
out that one of the broadband transducers (receiver) was not firmly mounted
onto the chamber. This might be a reason why a larger mean sound speed contrast
(1.0365) was obtained compared to the values obtained earlier (all less than
1.03). There was again no apparent depth dependence. Another interesting
phenomenon was that the difference between down cast and up cast was larger
than before, 1.0326 for the down cast and 1.0404 for the up cast. However, their
corresponding standard deviations were small, 0.0036 and 0.0037, respectively,
indicating they were self-consistent. Further examination of the data and more
experiments are needed to look into this problem.
Zooplankton (MOCNESS/BIOMAPER-II) report (Carin Ashjian, Peter Wiebe)
Our tenth MOCNESS tow was conducted on April 24 at station
40 in a deep basin (~650 m) in the center region of
VPR Report
The video plankton recorder on BIOMAPER has performed
excellently through much of the cruise.
The plankton composition differs markedly from that observed in this
region during fall 2001. Much of the shelf contained numerous algal mats
throughout the water column which apparently originated from blooms of diatoms
in the surface waters. Also observed on
the shelf were abundant radiolarians, some polychaete
worms, some small copepods. Very few
krill of any size have been seen. The
plankton composition near
The VPR system suffered two temporary breakdowns in the past
1.5 days. The first was caused by the strobe lens becoming loose and rotating
90 degrees within the strobe housing so that insufficient light was focused on
the imaged volume. The second breakdown
was caused by one of the cameras apparently losing alignment due likely to
vibration. Both situations were
competently rectified by Phil Alatalo and the other
VPR technicians. The VPR system is now
running well.
BIOMAPER-II functioned well during the transits between
stations 38 to 40. A ground fault in the
sonar system appeared just before the towed body was brought onto the deck at
the start of station 40 work. Although a
leaky connector on the up-looking 200 kHz transducer seemed to be the cause,
during the transit from station 40 to 41, the fault return and more recent
attempts to locate the cause have failed.
This ground fault may be related to a pattern of increased noise seen
recently on the 43 and 120 kHz frequencies and to a lesser extent on the 200
and 420 frequencies.
Once again, the scattering layers showed a diel migration pattern. Intense acoustics scattering was
located just below surface during the night and just before first light in 120 kHz
echograms and in 200 and 420 kHz echograms albeit with less intensity. By 0800, these three frequencies all showed
distinct migration of the backscattering downward. A clear area developed at the surface as the
sunrise took place. As the light of day brightened, the top portion of the scattering
layer got deeper. By mid-morning, the clear zone was about 50 meters deep
marking the top of the intense backscattering layer, which extended down to
about 100 m. Below 100 m, lighter
scattering extended into the depths. After
sunset, the higher levels of backscattering were again at the surface.
During the transit out from station 39, which was closest to
shore, to the more offshore station 41, the backscattering on the 120 to 420
kHz echograms became markedly reduced and reinforcing the notion that
backscattering levels in Marguerite Bay are substantially higher than in the
more offshore waters of the continental shelf.
Just before arriving at station 41 around 2200, a krill-like patch was observed
just below the surface that was small, but quite intense. None similar to this were observed in
Cheers, Peter