Atlantic Circulation and Climate Experiment
PALACE deployment cruise
TABLE OF CONTENTS
1 Cruise narrative
2 Description of measurement techniques
3 Preliminary analysis
4 Acknowledgements
5 Appendix
Table 1: CTD stations
Table 2: Mark 12 XBT deployments
Table 3: Mark 21 XBT deployments
Table 4: PALACE floats deployed
Table 5: Drifters deployed
Silvia Garzoli | AOML | garzoli@aoml.noaa.gov |
Robert Molinari | AOML | molinari@aoml.noaa.gov |
Claudia Schmid | CIMAS/ AOML | schmid@aoml.noaa.gov |
Douglas Anderson | CTD watch, PALACE | AOML | anderson@aoml.noaa.gov |
Claudia Schmid | Chief scientist | AOML/ CIMAS | schmid@aoml.noaa.gov |
Ryan Smith | CTD watch, ADCP | AOML | rsmith@aoml.noaa.gov |
Derrick Snowden | CTD watch | AOML | snowden@aoml.noaa.gov |
Gregg Thomas | CTD watch, XBT | AOML | thomas@aoml.noaa.gov |
CIMAS Cooperative Institute of Marine and Atmospheric Science
4600 Rickenbacker Cswy, Miami 33149, FL, USA
Additionally a closed box of CTD/LADCP stations in 6° S-4° N, 25.5° W-23° W as well as a section at 28° W were taken. A higher resolution in the upper ocean is achieved by XBT drops and velocity measurements from a vessel-mounted ADCP. The data set will be used to estimate the budgets of the box and to study the structure of the equatorial current system.
This cruise is part of a multi-year program sponsored by NOAA and NSF. Funds to buy the Palace floats have been provided by NOAA/OGP.
Fig. 1: Cruise track. The symbols are: + = CTD/LADCP station x = XBT,
P = PALACE float and D = surface drifter.}
The Mark 12 XBT computer is not Y2K compliant. The date on the Mark 21 computer was wrong during the whole testing phase of the Sippican board and software (it was thought to be not Y2K compliant, but this was not the case). Therefore the dates in all XBT files have to be corrected according to the log sheets.
CTD station 1 (test station) had to be terminated near the surface because no data could be recorded. After the termination as well as the slider and the brush were fixed a test station could be taken (CTD station 2). The data recording worked well but the closing of the bottles did not function properly. Only 4 of the 14 bottles were closed and their depth was not consistent with the tripping depth. The software configuration was changed in an attempt to solve the problem.
During CTD stations 3 through 7 only 8 or 9 out of 14 bottles were closed. All of them tripped at the correct depth. Thus the changing of the software configuration was successful. Since working on the carousel had not lead to any changes we finally decided to replace it. This improved the things considerably: All except for one bottle closed. After firing that bottle a dozen times on deck it worked from station 14 on.
The software of the vessel-mounted ADCPs had problems with bad data cycles from the p-code GPS. Since this problem might lead to gaps in the data we decided to use the ship-GPS for the on-line processing. This proved to be a much more stable configuration. In the final processing the p-code GPS can be used.
The NMEA was causing problems during the CTD casts. Thus it was turned off from CTD station 17 on. This does not pose any problems since the NMEA only adds GPS time and position to the file header. The time is also taken from the PC clock and the position is routinely typed in.
During CTD stations 43 and 44 the data quality deteriorated quickly. The profiles became increasingly spiky. After the spikes are filtered out the profiles are of good quality. The wiring of the CTD was thought to be the problem. After working on it we got much less error counts. We could not test it insitu since we already had reached the Brazilian waters.
Nearly everybody caught the flu during this cruise. Due to the high
motivation of everyone this did not cause any problems in keeping up with
the workload.
The LADCP is a RDI Broadband 150 kHz ADCP.
The Mark 21 system is a prototype which went through its first blue water test during this cruise. The XBTs were dropped adjacent to CTD casts to allow a comparison of the profiles. The system mostly worked well, but it was very sensitive and thus produced many loop resistance errors which are indicative for bad probes. These supposedly bad probes were later used with the Mark 12 system without any obvious problems.
The water masses in the upper 2000 m of the tropical Atlantic are the Tropical Surface Water (TSW), the Subtropical Underwater (SUW), the Central Water (CW), the Antarctic Intermediate Water (AAIW) and the North Atlantic Deep Water (NADW). The highest temperatures and lowest salinities of the TSW are observed north of the equator (1° N-3° N). At these latitudes the surface salinities at 23° W are lower than at 25.5° W due to heavy rain. Further down the thermocline with varying thickness is found. At 6° S it extends over 150 m whereas at 3° N the thermocline is only 50 m thick. The salinity maximum of the SUW is most pronounced at 6° S and in 2° S to 1° N (Fig. 5). It strengthens again from 3° N on northward. Around the equator the SUW coincides with the eastward Equatorial Undercurrent (EUC). North and south of the EUC the flow is weaker and the flow direction is more variable. Around 3° N to 4° N the flow is eastward at about 10 cm/s whereas it is mostly westward at and south of 3° S.
Between 500 and 1000 m the AAIW is found (Figs. 2 - 4). It is characterized by a low salinity, which increases slightly towards the north. Salinities below 34.5 reach further north at 25.5° W than at 23° W (to 0° 40'N instead of 0° ). The flow in this layer is quite variable when compared with the SUW flow (Figs. 5 - 6). Two currents can be identified easily. These are the Northern and Southern Intermediate Countercurrents (NICC, SICC) at 1° N to 2° N and at 2° S. There also is a westward flow band at 3° S (intermediate Southequatorial Current, SEC) and an eastward current at 6° S (intermediate Southequatorial Countercurrent, SECC). At the equator the upper part of the AAIW layer is governed by westward flow and the zonal velocities in the lower part are eastward (Figs. 2 - 4). The transition between west- and eastward flow is very close to the salinity minimum at 23° W and deepens toward the west, especially between 23° W and 25.5° W. This fact lies behind the change of the flow characteristics between 23° W and 25.5° W (Fig. 6).
All three sections show the surface SEC in the mixed layer (Figs. 2 - 4). Both at 25,5° W and at 28° W the current is split into two branches by the EUC. Only at 23° W the EUC is beneath a very thin layer of westward flow. South of the equator the eastward Southequatorial Undercurrent (SEUC) was found at 4° S to 5° S, 23° W and at 3° S and 4° S at the other two longitudes. It typically extends from the thermocline down to about 400 m with a westward current in and below the AAIW layer at the same latitudes. Only at 23° W the underlying intermediate depth flow is eastward underneath part of the SEUC. The geostrophic flow (not shown) at this location is not eastward and the eastward velocity derived from the LADCP is less than 5 cm/s. Thus it seems likely that this difference is due to a tidal current.
The equatorial flow at the target depth of the PALACE floats (1000 m) is eastward in 2° S to 2° N (Fig. 7). During a previous survey in the summer of 1997 the equatorial current was westward at this depth. This supports earlier studies which hypothesized that this current might be seasonal. At 3° S to 4° S the flow is westward, and at 6° S the velocities are eastward again. No preference of direction is observed at 3° N and 4° N.
Fig. 2: Section at 23W | Fig. 3: Section at 25.5W | Fig. 4: Section at 28W |
Table 1: CTD stations
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Table 2: Mark 12 XBT deployments
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Table 3: Mark 21 XBT deployments
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Table 4: PALACE floats deployed
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Table 5: Drifters deployed
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