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TAO TIP 7 science reports

SCIENCE REPORTS

5.1 Seasonal Forecasting at ECMWF (D. L. T. Anderson, ECMWF)
ECMWF has set up an operational coupled model system to produce global seasonal forecasts. One of the main contributors to predictability on these timescales is ENSO. The 97/98 El Niņo, in particular its onset, was well predicted. Because the coupled model is global it can also represent the impact of ENSO outside the tropical Pacific, for example, on the high latitudes and the Asian Monsoon.

Errors in the forecasts can arise from uncertainties in the atmosphere model, ocean model and initial
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conditions (ocean, atmosphere, land). Some deficiencies in the coupled model forecasts of equatorial Pacific SSTs over the 90s are discussed. Errors in the forecasts due to uncertainties in the ocean initial conditions are examined using coupled forecasts starting from different initialization methods (with and without ocean data assimilation and different assimilation set ups). Results show the ocean data assimilation can have a large positive impact on the coupled model forecasts of ENSO. Links are found between these forecasts and uncertainties in the ocean initial state in the central and western equatorial Pacific, as well as the north western tropical Pacific, outside the TOGA-TAO array region. The lack of salinity observations means that errors in the salinity field cannot be corrected. Assimilating temperature but not salinity can lead to dynamical imbalances along the equator.

5.2 Basin-Wide Adjustment of Mass and Warm Pool Displacement During the 1997-98 El Niņo-La Niņa (J. Picaut, IRD/ORSTOM and NASA/Goddard Space Flight Center)
An intriguing feature of the successive 1997-98 El Niņo-La Niņa events is their appearance at depth months before their signature in sea surface temperature. The subsurface TAO data showed that the anomalous downward movement of the thermocline in the central-eastern Equatorial Pacific was underway several months before the appearance of the 1997 El Niņo warming in sea surface temperature. Similar feature, associated with an upward movement of the thermocline, was also evident prior to the sea surface cooling associated with the onset of the 1998 La Niņa. In situ and TOPEX/Poseidon derived currents indicate that strong mass transport within the equatorial wave guide was already pushing the warm pool toward the east (west) as early as February 1997 (January 1998). Possible mechanisms for these original features are explored through the readjustment of water masses in the equatorial wave guide associated with the displacements of the eastern edge of the warm pool. The role of horizontal and vertical advection, of equatorial waves and their reflection on both ocean boundaries in this readjustment of mass and of thermocline depth all along the equatorial band is investigated. This is done through the use of TOPEX/Poseidon and TAO data, the Gent and Cane oceanic general circulation model forced by observed winds and a simplified coupled ocean-atmosphere model. In particular it was found that the strong westerly winds bursts end of 1996 - early 1997 (much probably originating from the Indian Ocean and the North/Pacific) acting in phase with the basic ENSO oscillation, were the main reason for the 1997 El Niņo to be so powerful. As for the basic ENSO oscillation, it appears to be due to equatorial wave reflections on both ocean boundaries, in accord with the delayed action oscillator and the revised advective/reflective mechanisms. Similarly, the sudden shift into La Ni¤a appeared to be due to equatorial wave reflection on both ocean boundaries together with the remote effect of weak easterly winds in the far western Pacific.

5.3 Impact of TAO vs. ERS Wind Stresses On Simulations of the Tropical Pacific Ocean During the 1993-1998 Simulated by the OPA OGCM (C. Menkes, LODYC and IRD/ORSTOM)
A simulation of the 1993-1998 period is performed with the OPA OGCM forced by weekly ERS 1-2 wind stress data from IFREMER/CERSAT extending the work of Grima et al (1998) for the 1992-1995 period in which the quality of the ERS-1 forcing fields proved to give high quality OPA simulations of the tropical Pacific. Heat and fresh water fluxes used in this simulation are climatological, computed from the ECMWF 1979-1993 reanalysis. First, SSTs are restored to Reynold's weekly SSTs with a restoring term of 40 W m °K. The implied heat flux by this restoring term is stored during the simulation. Second, this heat flux is added to the forcing fluxes and the model is rerun using this fluxes without any restoring terms. This results in simulations in which SST is now a free parameter (Vialard et al., 1998).

The simulation is evaluated relative to different data sets. First, a comparison to TOPEX/POSEIDON sea level anomalies shows a mean correlation of 0.84 in the 5°N-5°S band and a mean rms difference of 4.3 cm. The mean rms of the model and data sea level anomalies are respectively 5.3 cm and 7.9 cm. That suggests that the ERS wind stresses may be too weak in the equatorial Pacific band. Second, comparisons with TAO equatorial currents are performed. At the surface (-15 m depth) , correlations and rms differences between model and TAO currents at 0°, 156°E, 0°, 170°W, 0°, 140°W and 0°, 110°W average to 0.72 and 22.4 cm. However, simulated zonal current display a well-marked bias at 140°W and 110°W in the vertical. This bias is characterized by too weak and too shallow an equatorial undercurrent, and variability of the current structure that is too weak in the vertical. Comparisons between ERS and TAO winds at 10 m reveal that the ERS wind zonal gradient along the equator is weaker than observed in the in-situ data. Secondly, the ERS stress variability is weaker than observed variability at TAO moorings by 10-20%. These results are consistent with the findings of Graber et al. (1996) who found such systematic biases when comparing 10 m neutral winds from different ERS products to TAO buoys. However, among those ERS products, the IFREMER/CERSAT product was the least biased. In any case, such biases in the ERS products are also consistent with the lack of variability observed in the simulation.

We aim at improving the model simulation by including the information contained in the TAO wind data. To do so stresses are computed at each TAO mooring using stability-dependent formulae based on Liu et al. (1979) and Smith (1988). A combined data set ERS+TAO is constructed by optimally inserting weekly TAO stresses into the ERS baseline forcing. A new simulation is performed using the ERS+TAO stresses. Significant improvements are observed. First, in terms of simulated sea level amplitudes, the mean rms of the model sea level anomalies are now 7 cm while mean correlation and rms difference are unchanged. Second, correlation with zonal currents are improved above the thermocline. For example, simulated surface current correlations and rms differences with TAO zonal currents amount to 0.79 and 22.6 cm. In the east, the EUC core is now well located, and the variability of the current structure in the vertical is much improved at 140°W and 110°W. Among the model parameters, SST is quite dramatically affected by such changes. In the ERS+TAO run, there can be changes greater then 2°C in the eastern Pacific compared to the ERS run, during the 1997-1998 El Niņo. Such changes are achieved and dominated by enhanced vertical processes such as enhanced entrainment of cold water at the mixed layer base and enhanced vertical diffusion processes.

To this day, ERS 1-2 IFREMER wind products are possibly among the best observed winds available on a long time period. However, these results tend to show that there are still unresolved biased when comparing to TAO buoys that need to be understood. In particular, Graber et al. (1996) show that other comparisons with buoy networks outside the equatorial band seem less biased. This point is being investigated. However, if such biases in the equatorial band are proven to be true, as these simulations suggest, this could have several implications for ocean atmosphere climate predictions in models that assimilate such remotely sensed data. Finally, these results point out how crucial it is to have synoptic observations of in situ data such as those provided by the TAO array and the developing PIRATA array.

References:
Liu, W. T., K. B. Katsaros, and J. A. Businger (1979), Bulk Parameterization of Air-sea Exchanges of Heat and Water Vapor Including the Molecular Constraints at the Surface, J. Phys. Oceanogr., 10, 1722-1735.
Graber, H. C, N. Ebuchi, R. Vakkayil (1996), Evaluations of ERS1 scatterometer winds with wind and wave ocean buoy observations, Technical Report, RSMAS 96-003
Grima, N., A. Bentamy, P. Delecluse, K. Katsaros, C. Levy, and Y. Quilfen (1998), Sensitivity study of an OGCM to satellite wind-stress forcing, Journal of Geophysical Research, in press.
Smith, S. D. (1988), Coefficients for sea surface wind stress, heat flux and wind profiles as a function of wind speed and temperature,Journal of Physical Oceanography,93, 15,467-15,472.
Vialard, J. (1998), The role of salinity in an OGCM during the 1997-1998 El Niņo, in preparation.

5.4 Genesis and Evolution of the 1997-98 El Niņo (M. J. McPhaden, NOAA/Pacific Marine Environmental Laboratory)
This presentation describes the onset, development, and sudden end of the 1997-98 El Niņo, using data from the Tropical Atmosphere Ocean (TAO) Array of moored buoys and other data sets of the ENSO observing system. Warm sea surface temperature (SST) anomalies erupted in the tropical eastern Pacific during April-June 1997, and by July 1997 SST anomalies were the highest observed in the past hundred years. SST anomalies in the eastern Pacific subsequently exceeded 5°C, making this the strongest El Niņos on record. The onset of the El Niņo was characterized by surface winds along the equator that were punctuated by a series of westerly events of increasing intensity and eastward fetch. These westerly episodes, associated with enhanced Madden and Julian Oscillations in the atmosphere, locally drove warm water eastward near the equator. These westerly events also excited downwelling equatorial Kelvin waves that propagated into the eastern Pacific, depressing the thermocline by over 90 m in late 1997. At the same time, the thermocline in the western Pacific shoaled by 20-40 m in response to anomalous upwelling Rossby wave generation. Changes in SST due to ocean dynamical effects and anomalous air-sea heat exchanges led to changes in the location and intensity of atmospheric deep convection and precipitation in the tropics. Resultant anomalous heating of the atmosphere altered the position of the sub-tropical jet streams and storm tracks, affecting weather patterns worldwide. The event ended abruptly with the return of normal trade winds in May-June 1998, which upwelled thermocline water to cool the surface in the eastern and central equatorial Pacific. These observations will be used to test the delayed oscillator theory for ENSO, and the implications for the predictability of ENSO will be discussed.

5.5 Rectification of the MJO into the ENSO Cycle (W.S. Kessler, NOAA/PMEL and R. Kleeman, BMRC)
An ocean general circulation model, forced with idealized, purely oscillating winds over the western equatorial Pacific similar to those observed during the Madden-Julian Oscillation, developed rectified low-frequency anomalies in SST and zonal currents, compared to a run in which the forcing was climatological. The rectification in SST resulted from increased evaporation under stronger-than-normal winds of either sign, from changes in the vertical temperature gradient that were correlated with oscillations of upwelling speed at the intraseasonal frequency, and from zonal advection due to nonlinearly-generated equatorial currents. The net rectified signature produced by the MJO-like winds was SST cooling (about 1°C) in the west Pacific, and warming (about 0.3°C) in the central Pacific, thereby flattening or reversing the background zonal SST gradient. It is hypothesized that, in a coupled system, such a pattern of SST anomalies would tend to spawn additional westerly wind anomalies as a result of SST-induced changes in the low-level pressure gradient. This was tested in an intermediate coupled model initialized to 1 January 1997, preceding the 1997-98 El Niņo. On its own, the model hindcast a (relatively weak) warm event, but when the effect of the rectified SST pattern was added, the hindcast El Niņo became about 30% stronger due to the hypothesized additional westerlies. The results suggest that the MJO can interact constructively with the ENSO cycle, and therefore is more than just "weather noise" that introduces irregularity to the cycle. This implies that developing the capacity to predict, if not individual MJO events, then the conditions that affect their amplitude, would enhance predictability of the strength of oncoming El Niņos over present abilities as demonstrated in 1996-97.

5.6 Yoshida Jet Detected in JAMSTEC Subsurface Current Moorings (K. Kutsuwada, Tokai University)
Long-term measurements of oceanic currents in the subsurface layers by upward-looking acoustic Doppler current profilers (ADCP) at three stations (142°E, 147°E and 165°E) on the equator have been performed as a part of the Tropical Ocean Climate Study (TOCS) by the Japan Marine Science and Technology Center (JAMSTEC). Time series of the current data are analyzed to examine variations which are related to the onset of El Ni¤o events. Some episodes in which strong eastward flow covers the upper layer above about 100 m are recognized during the period from December 1996 to November 1997, corresponding to the onset and mature phases of the 1997-98 El Niņo event. In these episodes of surface eastward jet, the vertically-averaged (0-100m) eastward flow was larger than 0.5 m s and attained to 1.3 m s at the westernmost station (142°E) during the strongest episode occurring in December 1996. The surface eastward jet in the onset phase of the El Ni&#ntilde;o event (December 1996 and March 1997) occurred in the western Pacific at all the three stations, while in the mature phase (from April to November 1997) it was recognized only at the easternmost station (165°E). To investigate variations of the wind stress during these episodes, we construct data sets of daily surface wind-stress vectors on a 1° x 1° grid in the tropical Pacific using satellite scatterometer data (ADEOS/NSCAT and ERS-2 supplied by JPL and IFREMER, respectively). In all the episodes, westerly winds (bursts) stronger than 5 m s are predominant over the western equatorial Pacific covering our mooring stations. Dominance of the westerly wind bursts (WWB) is confined to the west of 160°E in the onset phase of the El Niņo event, while the WWBs migrate eastward to an area east of the dateline in the mature phase after May 1997. We attempt to interpret the occurrence of surface eastward jets as Yoshida jets in response to local wind forcing. Results reveal that in some episodes such as the strongest one in December 1996, the enhancement of the surface eastward current estimated from NSCAT wind data is almost identical to that observed in the mooring data. This means that the onset of this episode is interpretable in terms of Yoshida jet dynamics. On the other hand, in the termination as well as in the onset of other episodes, significant discrepancies are found between the estimated and observed enhancements of the surface eastward currents. These results suggest that the effect of remote wind forcing plays an important role during these periods, indicating the necessity for information on the zonal pressure gradient along the equator.

5.7 Remotely-Forced Effects on Currents and Water Properties in the Coastal Upwelling System Off Northern and Central Chile (S. Hormazabal Fritz, Regional Program for Physical Oceanography and Climate, U. Concepcion)
A recent seven-year (1991-1998) continuous record of currents over the continental slope at 30°S off Chile, at 220 m, 485 m, 750 m depths in 850 m of water, is used to show interannual modulation of intraseasonal coastal trapped waves in the eastern South Pacific ocean. The first six years of the continuous records correspond to the physical oceanography component of the bilateral research program "Marine Natural Resources - SAREC contribution to the international JGOFS Eastern Boundary Current Study off Chile" (1991-1997). This study is jointly sponsored by SAREC/SIDA (Sweden) and CONICYT (Chile). The last nine months of data are from the continuation of the observations within the Chilean research program FONDAP-Humboldt (1997-2000), which is a study of the circulation and physical-biological interactions in the Humboldt current system, and their impacts on regional bio-geochemical cycling.

The analysis of these records of currents confirms earlier results (Shaffer et al, 1997) that show a remarkably efficient transmission through the ocean of strong 40-70 day waves, driven by equatorial wind events. These waves travel first as equatorial Kelvin waves, along to equator and later as coastal-trapped waves along the coasts of South America. Wavelet analysis of along-shore currents shows that intraseasonal time scale variability associated with coastal trapped waves is seasonally strongest during the austral summer. It is also strongest during El Nino events (1991-1992, 1994 and 1997-1998) and weakest during La Nina events (1995-1996). Currents observations at 750 m depth show clearly an enhanced equatorward flow near the bottom during warm ENSO events. The analysis of records of sea level, sea surface temperature and coastal wind collected during five years (1991-1995), and sea surface temperatures obtained through remote sensing in the austral summers (1991 and 1992), show that sea surface temperature is controlled by local wind through coastal upwelling and strongly modulated by coastal trapped waves in the coastal area of northern Chile (18°-33°S). In the intraseasonal band, the sea surface temperature signal does not propagate alongshore, and is not related to the wind stress, particularly off Iquique (20°S), but sea level perturbations are followed by sea surface temperature anomalies with an 11-12 day lag-time. These relations are explained by changes in the depth of the thermocline due to coastal trapped waves that generate differences in water temperature entering the upper mixed surface layer due to coastal upwelling, modifying its heat budget and the sea surface temperature. In this way, the sea surface temperature is being strongly modulated by coastal trapped waves.

Reference:
Shaffer, G., O. Pizarro, L. Djurfeldt, S. Salinas, and J. Rutlant (1997): Circulation and low-frequency variability near the Chilean coast: Remotely forced fluctuations during the 1991-1992 El Niņo, J. Phys. Oceanogr.,27, 217-235.

5.8 TRITON Salinity Measurements (K. Ando and Y. Kuroda, JAMSTEC)

The surface layer in the western equatorial Pacific is characterized by a warm and fresh water pool of surface water. The zonal displacement of this pool is strongly related to the ENSO phenomena. The surface fresh water is formed by the heavy rainfall over the area, and to this area high salinity surface water from the east is transported and subducted below the surface fresh water by the westward South Equatorial Current. The contribution of salinity to density change in this warm fresh pool cannot be neglected. For example, lack of salinity data will cause errors in estimation of dynamic height and buoyancy in the mixed layer. The measurement of salinity is therefore crucial to understanding the western tropical Pacific. Twelve conductivity/temperature (CT) sensors are attached to each TRITON buoy, and more than 140 CT sensors are planned in the upper (0-750 m) western tropical Pacific as part of the TRITON project. A necessary first step is to verify the quality of our salinity data for meeting TRITON scientific goals.

The current status of the TRITON salinity measurement project is the validation of salinity data from four buoys (48 sensors) in March-June 1998 along 156°E, as well as comparing laboratory pre- and post-calibrations of each sensor. The temperature calibration by JAMSTEC shows good agreement (within 2 mK difference for all sensors) with that by manufacturer (SeaBird Electronics). The conductivity calibration by JAMSTEC shows a 0.8 mS m difference on average (equivalent to about 0.004-0.008 psu in salinity). The drift of the temperature sensors is very small (within 2 mK per year) on average, and the drift of conductivity sensor is 0.002 psu per month (0.024 psu per year) on average. Salinity data from the buoys are sometimes missing because of hardware or electrical problems, and there are occasional unrealistic values. However, data return was about 80% in real-time. In the mixed layer, temperature data shows strong diurnal cycles, and salinity data seem to show realistic variability related to local rainfall events.

5.9 SSS Changes in the Western Tropical Pacific During the 1996 La Niņa and 1997 El Niņo period: The present ORSTOM-TSG network in the Pacific. (T. Delcroix, ORSTOM/Noumea)

Sea-surface salinity (SSS) changes during the 1996 La Niņa and 1997 El Niņo events are analysed along the Fiji-Japan shipping track, based on 20 thermosalinograph sections. In the equatorial band, above-average SSS (35.2 - 35.4 psu instead of 35 psu) were observed in 1996, consistent with a well-marked south equatorial current, an unusually-strong equatorial upwelling, and below-average precipitation. From January to August 1997, the SSS decreased sharply from 35.2 - 33.8 psu (lowest recorded monthly value over the last 20 years), compatible with a reversal of zonal current, the occurrence of equatorial downwelling, and above-average precipitation. From September to November 1997, the SSS remained almost constant (34.2 psu), consistent with the opposite effects of eastward current, likely bringing low saline water from the Pacific warm pool, and of evaporative cooling, vertical mixing and below-average precipitation which all tend to increase SSS. The impacts of the SSS changes on sea level are discussed. The present status of the ORSTOM thermosalinograph network in the Tropical Pacific is also presented together with scheduled studies for assimilating SSS data in numerical models.

5.10 Observing Tropical SSS in the Future by Integrating TAO and Satellite Data (G. Lagerloef, Earth and Space Research, Seattle)
The ability to measure surface ocean salinity by passive microwave (L-band) remote sensing has been known for several decades and demonstrated with airborne instruments. Satellite mission designs in the U.S. and in Europe are presently being considered by cognizant space agencies. Because requirements for salinity are very similar to requirements for measuring soil moisture, these missions will measure both parameters, although the radiometric signal over the ocean is much smaller than over land.

This presentation first outlined the basic considerations for tropical dynamics with the following points:

  1. Interannual SSS variations of ņ1 psu are observed in the tropics, caused mainly by variations in rainfall and advection.
  2. SSS fields are needed to balance the upper ocean freshwater budget, initialize coupled climate models and validate freshwater flux parameterizations.
  3. It is possible to improve the initialization of tropical ocean climate models with SSS data by adjusting T-S curves with SSS and altimeter sea level data (e.g. recent work by Reynolds, Ji, Vossepol).
  4. Tropical SSS retrievals likely will be more precise than those in temperate and polar latitudes because of brightness temperature sensitivity to salinity increases with SST.
  5. TAO/PIRATA SSS data will be essential to improving and validating satellite SSS measurements. Satellite SSS error covariances can be estimated.
  6. Optimal interpolation of satellite, TAO/PIRATA and other in situ SSS (similar to Reynolds SST) will provide the best estimate of SSS fields in the tropics. This will yield high-resolution SSS fields with known errors which are essential for coupled model development.

The physical principles governing salinity remote sensing then were presented, along with the various errors and corrections that must be applied. The satellite mission concepts were then be described, along with their approval status within agency programs. These include the HYDROSTAR mission proposed to NASA earlier in 1998 with selections to be announced before the end of the year, and the European MIRAS/RAMSES/SMOS sensor which will be proposed to ESA on 30 November 1998 with selections to be announced mid-1999. If approved, these satellites may be launched in the 2002-2003 time frame, and could be planned in sequence to extend the potential time series to more than five years. The relative salinity retrieval aspects were addressed, and it is apparent that large-scale climatological variability in the tropics will be resolved. Accuracies may be <0.5 psu at 1° x 1° resolution and ~1 week time scales, and perhaps ~0.2 psu on monthly time scales. Accuracies ~0.1 psu appear possible in the future with more precise radiometer systems under study. For additional reference, the draft of the First Workshop Report, Salinity Sea Ice Working Group (SSIWG), held at La Jolla, CA, USA, 7-8 February 1998, can be found at http://www/esr/org/lagerloef/ssisg/ssiwgrep1.v2.html .

5.11 Estimating Rainfall in the Tropics Using the Fractional Time Raining and New Efforts at Obtaining Minute Resolution Rainfall Data in the Pacific (J. Ensworth, University of Oklahoma)
The relationship between the fractional time raining and tropical rainfall amount is investigated using rain gauge data and a point process model of tropical rainfall, building upon the work originally published by Morressey et al (1994). Both the strength and the nature of the relationship are dependent upon the resolution of the data used to estimate the fractional time raining. It is found that highly accurate estimates of rainfall amounts over periods of one month or greater can be obtained from the fractional time raining so long as high-time resolution (minute) data are used. It is demonstrated that the relationship between the fractional time raining and monthly atoll rainfall is quasi-homogeneous within the monsoon trough region of the equatorial western Pacific. Optical rain gauges also reflect this homogeneity but with an overall offset/overcatch indicated. Programs have been implemented to make these minute resolution rainfall measurements through the University of Oklahoma's Environmental Verification and Analysis Center (EVAC). SPaRCE (South Pacific Rainfall Climate Experiment), GLOBE and the DOE/ARM projects involve school participation in rainfall collection using automated weather stations.

Reference:
Morrissey, M., W.F. Krajewski, and M.J. McPhaden (1994): Estimating rainfall in the tropics using the fractional time raining. J. Appl. Met., 33, 387-393.

5.12 Easterly Waves and Convective Organization in the Eastern Equatorial Pacific ITCZ (Y. Serra, University of Washington)
Atmospheric sounding data are used to identify easterly wave activity in the East Pacific Intertropical Convergence Zone (ITCZ) during the Tropical East Pacific Process Study (TEPPS). TEPPS collected surface meteorological data, Doppler radar volumes, atmospheric soundings and rainfall data from the NOAA ship RONALD H. BROWN while on station at 7.8°N, 125°W from 08-23 August 1997. The main objective of the experiment was to understand the discrepancies between satellite microwave and infrared radiometer estimates of rainfall in this data poor region of the Pacific. In addition to results related to this objective, easterly wave activity was discovered as a prominent time scale of variability in the meridional wind and humidity data. The meridional wind shows variability on the order of 4 days, with a amplitudes of -5 to 12 m s-1 from the surface to 2 or 4 km. Maximum amplitudes in moisture variance are >ņ1 g kg-1 from the surface to 4 or 6 km. There were three cycles of the wave observed in the data. The maxima in the moisture occurred about a day before the maxima in the southerlies for two of these three events. An in situ convective indicator, calculated from the radar data, confirms a connection between convection over the ship and the meridional wind variance, with the convection occurring in the enhanced southerlies. As the ship provides just a point measurement of the winds, the location of the convection with respect to the surface convergence related to any wave passage cannot be determined. Satellite infrared radiometer (IR) data were also examined for 4-day activity. However, comparisons between IR cold cloud tops (<235°K) and the radar convective activity index indicate that IR data are not a reliable indicator of convection in the east Pacific (S. Yuter, personal communication). Only cloud systems >100 km and longer than 24 hrs in duration were consistently detected as IR cold cloudiness. Nevertheless, these data reveal non-propagating variability in IR temperatures on the scale of 4-5 days. The lack of propagation may be related to the failure of IR to detect all stages of the cloud systems and the use of daily averaged data, currently the highest time resolution available for the preliminary data set. Continued work in this area will include a closer look at the IR temperature data, using warmer cloud top temperatures and higher time resolution, as well as analysis of surface mooring data and NCEP and ECMWF model analyses.

5.13 Relationships between the Atlantic and Indo-Pacific El Niņo: Predictability of African Climate (M. Jury, University of Zululand)
Links between the oceans and the atmospheric circulation over Africa prior to and during historical El Niņo events were revealed through empirical studies using NCEP reanalysis composites and numerical studies using GCM simulations. Anti-phase relationships of tropical SST on either side of Africa were outlined. Warming of the tropical eastern Pacific increases upper level westerly winds downstream over tropical Africa. Cooling occurs in the eastern Atlantic as surface easterlies drive equatorial upwelling prior to an Indo-Pacific El Ni¤o event. The sub-tropical jet decelerates over southern Africa, creating a high pressure cell which blocks the supply of moisture during austral summer. Warmer sea temperatures in the western Indian Ocean attract convection away from southern Africa.

It is concluded that the atmospheric circulation generated by warm El Niņo conditions in the Indo-Pacific Oceans opposes that which develops over the Atlantic Ocean during a warm event there. Coupling of the ENSO circulation over Africa is dependent on the response of the Atlantic Walker Cell and underlying ocean. The PIRATA array is ideally placed to assist our understanding of the uptake of ENSO signals at seasonal lead times. PIRATA has already proved its worth in long-range predictions for Africa. During a December 1997 forecast meeting in Windhoek it was pointed out that the El Niņo situation was unusual for Southern Africa with warming in the tropical eastern Atlantic Ocean reducing the potential for drought. In hindsight, this was indeed the case. Further dynamical analysis of ocean-atmosphere interactions is proposed as part of the CLIVAR Africa project, and this could ensure continued involvement by African scientists in TIP activities.

5.14 Upper Layer Hydrology and Circulation Variability in the Western Equatorial Atlantic (B. Bourles, IRD/ORSTOM, K. Pailler, University of Brest, and Y. Gouriou, IRD/ORSTOM)
The western Tropical Atlantic is an area of crucial interest with regard to the thermohaline circulation and associated mass, heat, and salt transports. There, the North Brazil Current (NBC) and the North Brazil Undercurrent (NBUC) transport warm upper ocean waters toward the northern hemisphere, contributing to balance the southward flow of cold North Atlantic Deep Water, and closing the meridional overturning cell of the global thermohaline circulation. The NBC and NBUC feed surface and subsurface eastward flows at different depths and different latitudes. Namely, from south to north, the NBUC feeds the South Equatorial Undercurrent, whereas the NBC feeds the Equatorial Undercurrent, the North Equatorial Undercurrent and the North Equatorial Countercurrent (NECC). The quantification of mean and seasonal transports and water mass contents of these different currents is made very difficult due to a large spatial and time variability encountered in this region, and to eddies that detach from the NBC retroflection from boreal summer to winter. Four surveys, carried out in the western Tropical Atlantic, in January-March 1993, January-March 1994, September-October 1995 and April-May 1996 as part of the World Ocean Circulation Experiment Hydrographic Program, allowed to improve our knowledge of some main aspects of the circulation. Off the continental shelf, while the NBC retroflection is total from June to January, the continuity of the NBC along the American continent toward the Caribbean Sea is confirmed in boreal spring in the upper layer. The southeastward flowing current, observed around 3øN, 45øW and supplied by the NBC retroflection (but also by a North Equatorial Current recirculation) feeds, in the upper layer, the EUC and the NECC, and in the subthermocline layer, the EUC and the Northern Subsurface Countercurrent. Over the continental shelf, estimates of the transport off French Guiana indicate an annual mean coastal flow as high as 3.9ņ1.2 Sv from the coastline to the 200 m isobath (located 200 km offshore). There is no clear-cut seasonal variability of this coastal flow, which is strongly modulated by the offshore mesoscale eddies shed from the NBC retroflection loop.

The western Tropical Atlantic is also a region where different water masses are present. The waters formed within the subtropical region of both hemispheres exhibit salinity values up to 37 psu just above the thermocline. At the surface, the Amazon discharge is responsible for the presence of large fresh (S<34 psu) water lenses of about 30 m thickness, extending eastward as far as 30°W in boreal fall, when entrained by the NECC. Such different water masses superimposition implies significant vertical salinity gradients, largely superior to those observed in the western Pacific Ocean, that induce strong haloclines, and thus marked pycnoclines, yielding to the presence of "barrier layers." It is noticeable that fresh surface waters are generally associated to positive sea surface temperature anomalies, that may be the consequence of barrier layer effects. Furthermore, the determination of the mixed layer depth, by applying the commonly used criteria, indicates values of 3-5 m within the Amazon water lenses.

5.15 The Barrier Layer in the Atlantic Ocean (S. Masson, LODYC/University of Paris)
Many papers highlight the importance of the barrier layer in the vertical structure of the western Pacific ocean. The barrier layer is defined as a salinity stratified layer separating the warm surface layer from the thermocline. More recently, a barrier layer has been observed in the west Atlantic. However, this barrier layer does not seem to be created by a maximum of precipitation like in Pacific ocean. An ocean general circulation model forced by the 15-year ECMWF reanalysis fluxes (1979-1993) is therefore used to investigate the barrier layer formation mechanisms and to evaluate its impact on the vertical structure of Atlantic Ocean. Each year, this simulation generates a 40 m thick barrier layer between July and September offshore of the mouth of the Amazon. The seasonal variation of the barrier layer is mainly caused by the current dynamics. In surface layer, the North Brazilian Current (NBC) and the North Equatorial Counter Current system brings offshore fresh water of Amazon, while in subsurface, salty water from the south Atlantic is advected by the North Brazilian Undercurrent and the North Equatorial Undercurrent system. Our results do not show that input of fresh water by precipitation or by river runoff affect significantly the seasonal variation of the barrier layer.

In this study, interannual variations of the barrier layer are also investigated. The results of the simulation show a minimum barrier layer thickness in 1983 and 1987. In these two years, a strong NBC seems to advect the Amazon water along the coast, limiting the decrease of sea surface salinity offshore. Presence of a robust barrier layer in the simulations encourages us to investigate the effect of the hyaline stratification on vertical mixing. By running an experiment in which the mixed layer is computed only as a function of temperature, we establish the increase of the NBC retroflection by trapping the current in the shallow pycnoclines that result from barrier layer formation.

5.16 Formation and Spreading of Arabian Sea High-Salinity Water Mass (S. Prasanna Kumar, NIO)
The formation and seasonal spreading of Arabian Sea high-salinity water mass (ASHSW) were studied based on the monthly mean climatology of temperature and salinity in the Arabian Sea, north of the equator and west of 80°E, on a 2° x 2° grid. The ASHSW forms in the northern Arabian Sea during winter and spreads southwards along 24 sigma-t surface against the prevailing weak zonal currents. The eastern extent of the core is limited by the strong northward coastal current flowing along the west coast of India. During the southwest monsoon, the northern part of the core shoals under the influence of the Findlater jet, while the southern extent deepens. Throughout the year, the southward extent of the ASHSW is inhibited by the equatorial currents. The atmospheric forcing that leads to the formation of ASHSW was delineated using the monthly mean climatology of heat and fresh water fluxes. Monsoon winds dominate all the flux fields during summer (June-September) while latent heat release during the relative calm of the winter (November-February) monsoon, driven by cool, dry continental air from the north, results in an increased density of the surface layer. Thus, excess evaporation over precipitation, and turbulent heat loss exceeding the radiative heat gain, cool the surface waters of the northern Arabian Sea during winter and drive convective formation of ASHSW.

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