1. Introduction
For the observation of ocean currents in certain limited regions we propose a new variant of the Ranging and Fixing of Sound (RAFOS) technology (Rossby et al. 1986). This Lagrangian technique for the observation of intermediate and deep ocean currents relies on the propagation of acoustic signals between moored sound sources and freely drifting RAFOS floats. A minimum of two sound sources are required. They transmit typically one sound package at 260 Hz of 80-s duration at fixed time windows. These signals propagate in all directions. Transmission times of all sources belonging to an array are delayed by 30 min. This allows a sound package at an averaged speed velocity of 1.5 km s−1 to travel about 2700 km before the next package of an associate source is emitted. Adjacent listening windows of the RAFOS receivers enable the determination of arrival times from the different sources. The float’s microprocessor correlates the incoming frequency modulated (FM) signal and stores the highest and second-highest correlation and their times of arrival. The latter recordings represent the base for later triangulation of acoustic radii resulting in trajectories of our roving floats. After the floats have finished their preprogrammed underwater mission, they drop their ballast weights, return to the surface, and transmit their data via satellite link (Systeme ARGOS).
In this paper we introduce a recently developed and field tested RAFOS float derivative: the dual release float. We call a cluster of moored dual release floats a “float park.” A park can sequentially release temporarily moored floats from the sea floor. Because of the compressibility difference between water and the glass housing of floats, they are buoyant while on the seafloor far below their intermediate mission levels. After their initial release has been triggered following a predetermined delay, they ascend to their intended mission depth where they act as Lagrangian current meters like regular RAFOS floats.
2. Purpose
The simple idea of a float park (Fig. 1) can be applied when an intentionally delayed start of Lagrangian time series is desirable. Technically this new RAFOS family member will be used in regions with expected unfavorable weather or ice conditions, or where logistical constraints prevent regular seeding of RAFOS floats. For example, the latter scheme was successfully carried out on a chartered sailing yacht during the Mediterranean Undercurrent Seeding Experiment (AMUSE) in the Gulf of Cadiz between 1993 and 1995 (Hunt et al. 1998). In general, float parks are especially suitable in regions with point sources where spreading of water masses and their subsequent eddy generation and transformation are of major interest (Richardson et al. 2000). The observational result of a float park consists of a collection of float trajectories which all start at the same origin and yield sequential drift estimates from intermediate depths that are representative for certain seasons and regions.
The dual release floats are passive while moored on the seafloor. They hibernate for predetermined times until they wake up for their drift mission. A secondary, but not yet realized, task for dual release floats lies in their capability to act temporarily as monitors on the sea floor (MAFOS) (König et al. 1991). The latter instrument class was developed to improve RAFOS navigation accuracy by enabling corrections for potential long-term clock drifts and erratic jumps in the time base of sound sources.
3. System description
The technical realization of the first RAFOS float park was conducted through the cooperation of the Institut für Meereskunde in Kiel, Germany, and SeaScan of Falmouth, Massachusetts. The instruments are a derivative of the float generation built by SeaScan according to the design and specifications evolved by T. Rossby and B. Owens and their teams at the University of Rhode Island and the Woods Hole Oceanographic Institution. They were part of the World Ocean Circulation Experiment (WOCE) Lagrangian drifter experiment (Zenk 1997). The useful life of the instrument depends on the details of the mission programmed in FORTH. It can typically exceed 18 months.
The float is housed in a borosilicate glass pipe with one end rounded and closed (top) and the other end open. An anodized aluminum end plate closes the lower opening. It supports all the mechanical penetrators such as the pressure port, two hexagonal blocks with burn wires, a vacuum valve, and hydrophone (Fig. 2). All internal components are mounted on a styrene backbone. Starting from top to bottom, there is an ARGOS antenna and transmitter, the electronic boards, and the battery pack.
For the dual release version a second electronic board was added to the standard WOCE FORTH board. Its elementary modules include a single conversion acoustic receiver, power supply, I/O interface, hardware clock, switches for the ARGOS transmitter, electronic burn wires, pressure and temperature circuits, CPU, and memory (16 kB ROM and 32 kB RAM). The available FORTH software had to be extended for the delayed functions. Newly introduced FORTH words include “wire on/off” for servicing the first release block, which separates the moored float from its 12-kg dinghy anchor. RS232 compatible communication with the instrument’s processor is established by an optical link directly attached to the glass hull for programming and down-load sessions. In terms of costs the dual release version exceeds its parent by less than 5%.
For a precise and gentle deployment of RAFOS floats with two release blocks we have developed a special launch apparatus. It houses one float and is positioned vertically on a standard rosette sampler with the conductivity–temperature–depth recorder (CTD) lowered from the support ship (Fig. 3). This release apparatus replaces one Niskin bottle. Without any extra communication link the launch release is triggered from the CTD deck unit. Distance from the bottom can be controlled by a pinger that is often part of the CTD system. In our first park we triggered the pipe release successfully 20 m above the bottom.
4. A first experiment
A first RAFOS float park was installed on 28 May 1997 at about 53½°N, 31°W, that is, roughly 110 km east of Charlie Gibbs Fracture Zone in the North Atlantic (Fig. 4). This region is at the northeastern margin of the subpolar gyre and is of special interest to oceanographers. Its position at the southern tip of the Reykjanes Ridge provides for an intensive exchange of intermediate and deep water masses across the Mid-Atlantic Ridge. Low salinity Labrador Sea water is formed by convection west of Greenland, and spreads east at about 1300–1700-m depth after penetrating the Iceland Basin through the Gibbs Fracture Zone (Sy et al. 1997). Due to their climate relevance, seasonal and interannual changes of the inflow of Labrador Sea Water are of special interest.
It was the aim of our first float park experiment to demonstrate the feasibility of monitoring the circulation of intermediate waters by Lagrangian current meters. Because the relatively low salinity of Labrador Sea water, small variations can have a profound impact on water mass transformations in the Iceland Basin.
The first experiment was started from the FS Meteor. In May 1997 we launched four floats, one standard RAFOS and three dual release floats. Their mission parameters are shown in Table 1. All four instruments performed satisfactorily and returned to the surface at prescribed times. Though we were scheduled to return to the region only a few weeks later in August 1998 after all members of the float park surfaced, we had not originally planned to recover any of our four expendable floats. However, with some coordination and good luck we managed to locate and recover three freely drifting and telemetering floats by a specialized ARGOS receiver (GONIO) on FS Poseidon (Fig. 5). The unexpected retrieval of 75% of the hardware from the first float park enabled us to examine the impact of corrosion and the long-term behavior of the first prototypes. All mechanical parts worked well. Signs of significant corrosion were observed on the slots of the pressure release valves in the end plate (see Fig. 2).
Overlaid in Fig. 4 are the trajectories from the first park floats. Basically, we expected a predominant easterly flow advecting fresh Labrador Sea Water into the Iceland Basin with superimposed eddy “noise.” Even if we assume 100 km to be a typical correlation scale for the intermediate inflow east of Gibbs Fracture Zone, we cannot detect a coherent spreading of Labrador Sea Water in these trajectories. With the exception of the southwest quadrant, all other flow directions were observed in the float park region. The trajectories of our winter float 414 with its northeastern drift best illustrates the expected flow regime. In contrast, float 412 started its mission at mid summer and was advected westward by a counter current into the Irminger Sea. Further observations and the evaluation of simultaneous Eulerian current meter data from just north of Gibbs Fracture Zone will assist us in explaining the peculiar return flow shown by float 412.
5. Conclusions
An instrument type has been built and successfully tested over 15 months that allows the establishment of a Lagrangian time series (cf. Rossby et al. 1995). Depending on scientific objectives, financial resources and accessibility of monitoring sites dual release floats in parks (also called “float farms”) can report representative currents and their natural variability. Their trajectories allow to estimate temporal and spatial means and variances.
Since the dual release float is derived from a standard RAFOS float, it constitutes a low-cost, expendable instrument that can be deployed in groups from the seafloor. For its control tasks it utilizes the existing capability of the microprocessor on board the standard float. In fact, it makes any additional apparatus with revolving triggers and separate time releases on the ground superfluous. In principle dual release floats can start their Lagrangian mission from a variety of underwater platforms, that is, a light anchor or a mooring of opportunity. We suggest that this simple new tool will become an integral part of the Global Ocean Observing System presently under discussion or in preparation by a number of bodies in operational oceanography. Float-park data will have the potential of detecting and monitoring climate changes and for understanding oceanic variability over a wide range of timescales in selected ocean regions (OOPC 1998).
Acknowledgments
This work has been supported by the Deutsche Forschungsgemeinschaft, Bonn (SFB 460). We thank the captains and the crews of FS Meteor and Poseidon for their skilled help during deployment and the unforeseen recovery exercises of our first dual-release floats. We also thank two anonymous reviewers for their valuable suggestions.
REFERENCES
GOOS Rep 33, 37 pp. [Available from UNESCO.].
Hunt, H. D., C. M. Wooding, C. L. Chandler, and A. S. Bower, 1998:A Mediterranean Undercurrent Seeding Experiment (AMUSE):Part II. Woods Hole Oceanographic Institution Tech. Rep. 98-14, 123 pp. [Available from Woods Hole Oceanographic Institution, Woods Hole, MA 02543.].
König, H., K. L. Schultz Tokos, and W. Zenk, 1991: MAFOS: A simple tool for monitoring the performance of RAFOS sound sources in the ocean. J. Atmos. Oceanic Technol.,8, 669–676.
Richardson, P., A. Bower, and W. Zenk, 2000: A census of meddies tracked by floats. Progress in Oceanography, Vol. 45, Pergamon, 209–250.
Rossby, T., D. Dorson, and J. Fontain, 1986: The RAFOS system. J. Atmos. Oceanic Technol.,3, 672–679.
——, G. Siedler, and W. Zenk, 1995: The volunteer observing ship and future ocean monitoring. Bull. Amer. Meteor. Soc.,76, 5–11.
Sy, A., M. Rhein, J. R. N. Lazier, K. P. Koltermann, J. Meincke, A. Putzka, and M. Bersch, 1997: Surprisingly rapid spreading of newly formed intermediate water across the North Atlantic Ocean. Nature,386, 675–679.
Zenk, W., 1997: North Atlantic anticipates biggest float fleet ever. Int. WOCE Newsl.,27, 32–34.
First RAFOS float park: Mission parameters and basic observational results