Measurements of aerosol bulk composition, optical depth, size distribution and the incoming solar radiation flux were carried out over the coastal waters of India, the Arabian sea and the tropical Indian Ocean during a cruise conducted in January 1996. Aerosol concentrations were relatively high throughout much of the cruise, even when the ship was at considerable distances from land. In this paper, we link the observed spatial variations and meridional gradients in the measurements to monsoonal and interhemispheric transport across the ITCZ using a high resolution global reanalysis that highlights the winter monsoon. We show that the northeast monsoonal low level flow can transport sulfates, mineral dust and other aerosols from the Indian sub-continent to the ITCZ within 6 to 7 days. These transports result in an increase in the aerosol optical depth (AOD) at the equator by as much as 0.2 and decrease the solar radiative forcing at the sea surface by about 10 to 20 W.m-2. The high concentrations of continental aerosols are a result of 3 factors: Strong (about 6 to 10 m/s) near-surface northerly flow; a shallow boundary layer of about 400 to 800 m thick, which traps the pollutants; subsidence associated with the north east monsoon, which suppresses rainfall over most of the Arabian sea and thus minimizes wet removal processes. In addition dust can be transported in the middle troposphere from the Arabian desert to the cruise region 4000 km away with a transit time of 2-3 days. There is strong evidence in interhemispheric transports effected by eddies that wrap around the ITCZ. These eddies bring clean southern hemisphere air to about 10°N in the Indian Ocean and carry polluted continental air into the southern hemisphere. In this manner substantial amounts of aerosols and other pollutants can be routinely transported to the southern- hemisphere Indian Ocean during the northeast monsoon. Thus, in order to understand the connection between continental emissions and impacts over the Indian Ocean, it is necessary to focus on the role of the northeast monsoon in the large- scale atmospheric circulation over this region.
One of the largest sources of uncertainty in validating model predictions of climate change is the role of aerosols in the radiation budget (IPCC, 1995). Due to their short residence times, aerosols with varying optical properties are not uniformly mixed around the globe and consequently, their chemical and physical characteristics, including radiative properties, are subject to significant regional variations (Kiehl and Briegleb, 1994). The transport of aerosols from source regions on the continents to the remote oceans could play a significant role in the global radiative forcing. The primary objective of this study is to understand the extent to which continental aerosols, both natural and anthropogenic, can be transported over clean oceans areas hundreds and thousands of kilometers away from sources and to characterize the meteorological processes responsible for this transport.
The focus of the study is the Arabian sea which is surrounded by arid and semi arid regions producing wind blown dust particles into the atmosphere in addition to the anthropogenically-produced sulfate and carbonaceous particles. We know very little about the transport of these aerosols or their effects on radiative forcing over the Arabian Sea and the larger Indian ocean. The ideal time to examine this aspect of the aerosol-climate problem is during the winter monsoon when the prevailing low level winds are north-easterly, blowing from the Indian sub-continent towards the Arabian sea and the tropical Indian Ocean. Thus conditions are ideal during winter for the study of the transport of continental materials over the ocean surface, the formation of new particles during transit and the consequent radiative forcing of the aerosol products.
Our study is based on aerosol and radiation data collected from a research vessel in the Arabian sea and the tropical Indian ocean. For characterizing transports, we used meteorological fields obtained through a high resolution reanalysis described in Krishnamurti et al. (1991). The unique aspects of this reanalysis are twofold: i) It is based on a physical initialization which is critical for the tropical monsoonal flows; and ii) The reanalyzed fields are computed on a horizontal grid of 70 km x 70 km. Such high resolution is extremely important for distinguishing small-scale features such coastal flows and the structure of the ITCZ, all of which are fundamental for assessing aerosol transport.
The cruise was a preliminary component of a comprehensive international field campaign, the Indian Ocean Experiment (INDOEX) (Ramanathan et al., 1995, 1996) which will take place in early 1999 with the objective of studying the aerosol-chemical-microphysical-radiative interactions over the southern Arabian Sea and the equatorial Indian Ocean. A series of pre-INDOEX cruises on ships-of-opportunity are being conducted before the main field phase. The first of these was on the R/V Malcom Baldrige (Rhoads et al., 1997) in March-April 1995; the protocol included vertical profiles of ozone and water vapor, and extensive measurements of aerosols and gases. There were very large temporal and spatial variations in all properties which could be associated with changes in air-mass characteristics; air masses from the Arabian Sea showed dramatically higher concentrations of aerosol and gas species that are typically associated with polluted continental sources (Rhoads et al., 1997).
Our present study focuses on the second pre-INDOEX cruise which was conducted during 5 January - 4 February 1996 aboard the Indian research vessel ORV Sagar Kanya during which research groups from India and USA participated. Measurements included aerosol mass concentration, size distribution, and the concentration of trace gases. In addition there was a very extensive series of radiation measurements, including AOD and spectral-to-broad-band solar fluxes at the sea surface. Jayaraman et al, (1997) describe the results of the aerosol measurements and direct radiative forcing. In this present paper we attempt to link the oceanic aerosol forcing described in Jayaraman et al with additional speciated aerosol concentration data (described herein) and with an analysis of the meteorological processes that control transport from the continents.
Table 1 gives a list of observations and instruments
used in this study including those presented in Jayaraman et
Cruise History: Figure 1 shows the ship's track. The research vessel left Goa, India, on 4th January 1996, sailed in the Arabian Sea and the Indian Ocean down to 5° south and returned to Bombay on 4th February. The cruise took place during the northeast monsoon when clear-to-broken low cloud conditions usually prevail north of about 4°N and when the ITCZ is located at the equator or south of it. Both during the initial and final phases of the cruise, observers aboard the ship reported that the sky was nearly cloud-free north of about 4°N. During the period 20-31 January, however, the sky was cloudy, and deep convective clouds were seen over the equator; thus it was not possible to make radiation measurements during this period. These onboard visual observations are consistent with the sky conditions that we inferred from polar orbiting NOAA satellite data, described next.
Satellite Observations: The cloud cover derived from the AVHRR imagery (shown in Jayaraman et al., 1997) using spatial coherence analyses (Coakley and Baldwin, 1984) indicated that the area-mean cloud cover between the start of the cruise and 8°N ranged between 10 and 25%, with the cloud tops well within the boundary layer. Subsequently the Sagar Kanya sailed into the ITCZ, south of the equator. In this portion of the cruise the infrared brightness temperatures (IRBT) were below 240 K and the rainfall greater than 8 mm/day. This range of IRBT's is typical of upper-troposphere clouds generated by deep convection. The ship sailed north??? out of the ITCZ into relatively undisturbed conditions and then returned to the ITCZ during the later phase of the cruise. At the end of the final leg, the Sagar Kanya reentered a region of predominantly clear skies off the western coast of India.
Aerosol Sampling Procedures: Daily bulk concentrations were measured by drawing air through Whatman-41 filters (20 x 25 cm) at a flow rate of about 0.8m3/min. To minimize contamination from the ship itself, the sampler was placed above the bridge, well forward on the ship, and the pump was electronically controlled so that it was activated only when the winds came from a 270 degree sector centered on the bow and when the velocity exceeded 2 m/s. Filters were changed once a day in the morning. A procedural blank filter sample was taken for every four exposed filters by manipulating an unexposed filter through the sampling protocol without actually drawing air through it. In the marine bounder layer (MBL), the aerosol collection efficiency of Whatman-41 filters is essentially 100% for nss SO4= (Pszenny et al., 1993) and greater than 95% for NO3- and 00% for mineral; dust (Savoie, 1984).
The exposed bulk filters were individually sealed in plastic bags and returned to Miami for chemical analysis. In Miami, a quarter of each bulk filter was extracted with 20 ml of 18 M cm Milli-Q water in three separate aliquots of 10, 5 and 5 ml. Sample solutions were measured for Na+ with a standard deviation of ± 2% by flame atomic absorption and Cl-, NO3-, SO4= and methanesulfonate acid (MSA) within ± 5% by suppressed ion chromatography (Savoie, et al., 1989a) and NH4+ within 10% by automated colorimeter. Non-sea-salt (nss SO4=) is calculated as total SO4= minus Na+ concentration times 0.2517 (i.e., the SO4=/Na+ mass ratio in bulk sea water). The bulk filters were also analyzed for mineral dust by ashing the extracted filters at 500&176;C for several hours and weighing the residue. During the extraction process, some soil components (e.g., gypsum) are dissolved and, during the heating process, volatile materials (e.g., bound water, halides, carbonates) in the dust can be vaporized; to correct for these losses, we derived the dust concentration from the ash weights by multiplying with a factor of 1.3.
Because the filters collect HNO3 vapor with high efficiency, we consider our measured NO3- concentrations to represent total inorganic NO3-, that is, aerosol plus gaseous HNO3 (Savoie et al., 1989a). However, the concentration of gaseous HNO3 in the near-surface MBVL is typically around 20% or less of the total NO3- (Savoie and Prospero, 1982). The concentration of NH4+ reported here should be regarded as the total of aerosol NH4+ plus any gas-phase NH3 that might react with un-neutralized acid species on the filter (e.g., nss-SO4= and NO3-).
Aerosol microphysical properties: The AOD measurements discussed herein were made using a manually operated hand- held sun-photometer at five wavelength bands selected by interference filters centered at 399 nm, 497 nm, 667 nm, 848 nm and 1051 nm and having bandwidths (full width at half maximum) 19 nm, 13 nm, 13 nm, 14 nm and 25 nm respectively. Measurements were also made with an automated sun-photometer (Space Physics Laboratory, Trivandrum) whose results were consistent with those used in our study. The filter's transmission characteristics were periodically calibrated in the laboratory using a spectrophotometer; the effective central wavelength of the filters (transmission weighted by photodiode response and the solar spectral intensity) is used to convert the measured radiation intensity into AOD. The photometer is manually aimed at the Sun and the peak voltage is recorded during clear sky conditions and for solar zenith angles up to 70°. The total field of view of the photometer is relatively large, 8°, to facilitate the pointing of the instrument toward the sun from the ship deck.
The total optical depth, δ is calculated from the measured voltage, V and the air mass factor, 1/µ where µ = cos &dunno; and &dunno; is the solar zenith angle at the time of measurement. The instrument constant V0, the 'no atmosphere' condition, is obtained by Langley plots made periodically at Mount Abu, a hill station about 1.7 km above mean sea level in northern India (25° N). The V0 values are corrected for the mean sun-earth distance for the day.
The AOD, δa, is obtained from δ after subtracting the optical depths due to Rayleigh scattering and absorption by ozone and water vapor. Rayleigh scattering is calculated assuming an average air column density value of 2.16 x 1025 molecules/cm2; the annual variation in the air column density is less than 2% (Sasi and Sengupta, 1986) and is not considered in the present study. Ozone absorption is computed from Dobson ozone measurements made at Ahmedabad (23°00'N, 72°40'E) for over 30 years (Angreji, 1989); computed values are 0.01 and 0.017 for the 497 and 667 nm channels (weighted for the entire bandwidth) respectively. No corrections were made for the seasonal variation in the column concentration of ozone, about 4%. Water vapor absorption is computed from a constant model water vapor density value of 17g/m2 applicable for the Arabian and Indian Oceans for the months of January and February (Sarkar et al., 1982); computed values are 0.035 and 0.018 for the 667 and 1051 channels respectively. The small NO2 absorption at 399 and 497 nm is ignored. The cumulative effect of these assumptions in the retrieved AOD is expected to be less than 15% for typical AOD values.
Aerosol Size Distribution: A quartz crystal microbalance cascade impactor (PC-2, California Measurements Inc., USA) was used for the measurements of mass concentration and the size distribution of particles. The ten-stage impactor operates as a flow rate of 240 ml/min with 50% cut off at 0.025, 0.05, 0.1, 0.2, 0.4, 0.8, 1.6, 3.2, 6.25 and 12.5 µm diameter at ambient temperature and relative humidity (Jayaraman et al., 1997). Aerosol number size distributions were derived from the impactor mass-size data; these could be well fitted by the Junge's power law curve of the form, dn/d(log r) = K * rv , in the radius range 0.1 to 10 µm. Figure 2 shows a time series from January 5 to February 4, 1996 for daily average aerosol size distributions. A high 'v' value along with a high 'K' is an indication of the presence of an increased number of submicron particles relative to supramicron particles.
Radiation Measurements: Direct solar radiation measurements were made using calibrated Epopley normal incidence pyroheliometers. We had two independent estimates for the surface global solar flux for λ < 800 nm. We deployed a Biospsherical Instruments Inc. (San Diego, California) model GUV-531 multichannel solar ultraviolet/visible radiometer system, hereinafter referred to as the "photodiode radiometer." The channel of interest here is the so-called photosynthetically active radiation (PAR) channel, which covers the wavelength range 400-700 nm. Lastly, a pair of Eppley PSP pyranometers were deployed, one for measurements of global solar flux in the 280 to 2800 nm and the other in the 780 to 2800 nm wavelength regions. The radiometric instruments as well as the data reduction techniques are described in greater detain in Jayaraman et al. (1997).
The reanalysis of the meteorological fields used in this study is based on physical analysis procedures developed at FSU (Krishnamurti et al. 1991). Physical initialization was performed using a very high resolution, T-170, global spectral model (space resolution of roughly 70 km at equator). The observed rainfall used during physical initialization was based on surface and satellite rainfall as described in Gairola and Krishnamurti (1992). The physical initialization involves rainfall and OLR assimilation using several reverse algorithms:
This process restructures the humidity profiles along the vertical and spins up the convective heating, divergence and the related fields consistent with the observed rain rates. The diabatic heating and divergence fields evolve during the physical initialization consistent with the improved rain rates. The surface fluxes also become well defined with robust air-sea coupling. Therefore, we feel that our reanalysis is dynamically and thermodynamically much more consistent than the original ECMWF analysis. As an example, the analyzed fields for January 7, 1996 and February 2, 1996 are shown in Figs. 3 and 4; these are representative of the upper and lower level streamline field of a very active phase of the winter monsoon. Fig. 3a shows the 1000 mb flowfield along with the AVHRR IR radiances in Fig. 3b. Very low values of channel 4 radiances, suggest cold and thick upper tropospheric clouds, typical of the ITCZ. Thus, if the analysis is accurate, low level convergence regions should correspond with low IR radiances.
The strong northerly flows at the 1000 mb over the Arabian sea and Bay of Bengal (Fig. 3a and 4a), are typical of the NE monsoon. We note a very rapid veering of these flows by 850 mb where the flows are northeasterlies over the Arabian sea to almost due easterlies over the Bay of Bengal and the south-eastern Arabian Sea. Returning to the surface flow (1000 mb) changes abruptly to southwesterlies over the Arabian peninsula. At the 200 mb level, southwesterly flow prevails south of 10°N, veering to westerlies north of 10°N. The implications of the above flow patterns to the aerosol transport are:
The positions of the low level convergence regions correspond roughly with the cold clouds in the AVHRR image (Figs. 3b and 4b). This agreement gives us confidence in the analyzed fields. In addition, monthly mean rainfall analyses during the cruise is illustrated in figure 5. The distribution and magnitude of rainfall are very similar to the ITCZ location inferred from the AVHRR brightness temperatures shown in Jayaraman et al. (1997). It is important to note an important characteristic of the ITCZ that is revealed by the AVHRR brightness temperatures, analyzed precipitation field(see the yellow region in Fig. 5) and the low level flow pattern (Figs. 3a and 4a): it tilts in a south westward direction, from about the equator (around 75°E to 90°E) to about 5&176#;S to 15°S (around 40°E to 60°E).
The aerosol concentrations for the principal species (nss-sulfate, nitrate, ammonium and mineral dust - collectively referred to as "SNAD") are shown in Fig. 6 plotted along the path of the vessel. The highest concentrations were obtained toward the end of the cruise when the ship was close to the wet coast of India. However, relatively high concentrations were observed during most of the cruise, even when the ship was near the equator, at a considerable distance from India and other land masses. Indeed, almost all samples collected during the cruise yielded concentrations of NO3- and nss SO4= that are substantially greater than oceanic "background" values about 0.1 µg/m3 for NO3- and 0.3-0.7 µg/m3 for nss SO4= (Savoie et al., 1989b).
Our data suggest that the aerosol concentrations are largely driven by transport from continental sources. The contribution of SO4= from the oxidation of ocean-derived dimethylsulfide (DMS) is believed to be very small based on the very low concentrations of aerosol methanesulfonate (MSA) that we measured. Fig. 7 shows the concentration of MSA along with that of nss SO4=. Using MSA, we can estimate the quantity of SO4= derived from the DMS. Previous studies have shown that in the low and mid-latitudes of remote ocean regions, the ratio of nss SO4= to MSA is relatively constant, about 12-15 (Savoie et al., 1994). Using this ration, we convert the MSA values into an equivalent concentration of SO4= as shown in Fig. 7. It is clear that the oceanic component of SO4= is a very minor fraction of the total concentration; only in one case (sample JD 18) did ocean-derived nss SO4= constitute a substantial fraction of the total.
The relative concentrations of NO3-, nss SO4= and NH4+ did not vary much throughout the cruise except for the portions close to the coast of India on the return leg (JD 31, 32, 33). The ratios of NO3- to nss SO4= (Fig. 8a) and NH4+ to the sum of nss SO4= and NO3- (Fig. 8b) fall into two groups, with the samples for JD 31, 32, and 33 standing out from the remainder of the group, a factor that is emphasized in Fig. 8c, which shows the ratio of nss-SO4= to dust. The composition of the samples from JD 31-33 are dominated by mineral dust which comprises about half of the total measured species mass in the samples, including sea salt aerosol. The NO3- concentration in samples JD 31-33 is also unusually high as reflected in the ratio of NO3- to nss-SO4= (expressed in equivalents); it is about 0.3 except for JD 31-33 where it is over twice as great. Based on the ratio of NH4+ to the sum of the acid species nss-SO4= and NO3-, the aerosols are somewhat acidic with ratios (measured in equivalents) in the range of 0.6 to 0.8; Jd 33, which has a ratio of 1.1, stands out as an exception. However, given that dust is a major constituent in most samples and that neutralizing species such as CaCO3 are common constituents in dust, we might expect that the aerosol samples are considerably less acid than suggested in Fig. 8b.
The mean concentrations measured during the cruise were (in units of µg/m3): NO3-, 1.68, nss-SO4=, 3.12; MSA, 0.023; dust, 3.52; NH4+, 1.31; Na+, 1.90 (and sea salt, expressed as 3.256*Na, 6.19). The mean aerosol concentration for all species for the entire cruise is 15.84 µg/m3. These results are consistent with the limited aerosol data that are available for this region. Measurements made during the spring of 1979 during the Global Weather Experiment (Savoie et al., 1987) show that the concentrations of aerosol nss-SO4= and NO3- are relatively high in the Arabian Sea and northwestern Indian Ocean (nss-SO4=, 2.7 µg/m3; 1.01 µg/m3); in contrast, in winds from the southern hemisphere, concentrations drop to very low values (nss-SO4=, 0.50 µg/m3; NO3-, 0.16 µg/m3). Savoie et al. (1987) attributed the high concentrations of nss-SO4= and NO3- north of the ITCZ to the transport of pollutants out of India and the Middle East and possibly Europe. Savoie et al. also found strong gradients in dust concentrations. In northerly winds, the dust mean was 7.59 µg/m3; in contrast, southern hemisphere winds yielded an average of 0.27 µg/m3 (Savoie et al., 1987). Indeed, dust concentrations over the Arabian Sea and the NW Indian Ocean close to Africa are comparable to those measured along the west coast of Africa and the Mediterranean (Savoie et al., 1987; Prodi et al., 1983). More recently, in 1995 during the spring cruise of RV Malcom Baldrige, Rhoads et al., (1997) found that in the southern and central Indian Ocean south of the ITCZ, NO3- aerosol concentrations were typically in the range of 0.1-0.2 µg/m3. North of the ITCZ, NO3- concentrations were sharply higher, typically ranging from 0.5 to 2 µg/m3; with values as high as 3.5 µg/m3, nss-SO4= typically ranged from 1 to 4 µg/m3 with values as high as 9 µg/m3. Mineral dust concentrations in southern-hemisphere India Ocean air masses were below the detection limit (about 0.1 µg/m3); in contrast, the mean for Arabian Sea air was 6.2 µg/m3. The concentration distributions and the seasonality observed on these cruises are generally consistent with the aerosol transports shown in AVHRR (Husar et al., 1997), with the absorbing aerosol (dust) transports indicated in Herman et al. (1997) and with the monsoon circulation and the inferred dust distribution (Ackerman and Cox, 1982, 1989).
Concurrent complementary aerosol and radiation measurements were made on the same cruise as reported by Jayaraman et al. (1997). These are briefly summarized here.
The AOD in the visible wavelength region was in the range of 0.2 to 0.5 over the Arabian Sea and 0.1 and below over the equatorial Indian Ocean. Total aerosol mass concentrations decreased from a high of about 80 µg/m3 near the coast to a low of few tenths µg/m3 over the more distant ocean regions; similarly, the sub micron size (< 0.1 µm) particles showed more than an order of magnitude decrease in the number concentration. The large increase in the small particle concentrations near the coast was also consistent with the corresponding large increase in the Angstrom exponent, α, which increased from 0.2 over the Indian Ocean to about 1.4 near the coast.
The radiative forcing from the aerosol was obtained for the direct solar flux and for the global (direct + diffuse) solar flux separately in the UV, visible and near IR spectral regions. The regression of AOD against the flux measurement shows that for an increase of 0.1 in AOD the direct visible (< 780 nm ) solar flux decreases by about 42 W.m-2 and the global flux in the visible region decreases about 14 W.m-2 (with an uncertainty of 10 w.m-2). For the same extinction AOD, the radiative forcing (direct + diffuse) of the coastal aerosols is larger than the open-ocean aerosol forcing by a factor of 2 or larger. In summary, the data presented here and by Jayaraman et al. (1997) reveal a strong latitudinal gradient in the aerosol mass, number concentration, AOD and radiative forcing, all of which decrease from the Arabian Sea to the equatorial Indian Ocean.
In this section, we examine in detail the speciated aerosol chemistry measurements presented in Section 4.1 with AOD data (Fig. 9). Nss-Sulfate is derived from biogenic (oceanic) and anthrpogenic sources (Hameed and Dignon, 1992). Ammonium is derived primarily from continental sources with some contribution from the oceans. Nitrates are from anthropogenic sources as well as from lightning; the latter might be especially important in the ITCZ region. It should be noted that AOD data are available for only a few days, primarily because of cold interference. The following are the important features:
Two aspects of computation are noted first:
We compute 7-day back trajectories launched from the ship position. In Fig. 10 (a,b,c) we illustrate the trajectories originating from 990, 900 and 850 mb for the cruise dates of January 12, January 15, January 19, January 22 and February 2, 1996. We focus primarily on the lower levels, because the bulk of the aerosol radiative forcing at the surface is expected to take place in the lowest 1 to 2 kilometers. The following criteria were applied in selecting the 5 days shown in the figure: we selected only those days for which data were available for both the AODs and the aerosol sampling and from these we used only those days when the aerosol AOD and the sulfate concentrations reached near- maximum (Jan 12, 15, 22; Feb 2) or near-minimum values (Jan 19).
We see a number of features in these illustrations, Fig. 10 (a,b,c). Air parcels arrive offshore of the southwest coast of India from the south of the equator and from India at 990 mbs. Trajectories indicate Arabian air incursion offshore of southwest India at 900 and 850 mbs. Trajectories overlying the Bay of Bengal also make it offshore of the south western India at 900 and 850 mbs. The nature of the computed trajectories suggest that mineral aerosols from the desert region of Arabia as well as from the semi-arid regions of India could make their way into the offshore region of southwest India, see Fig. 10 (d and e). These two illustrations show a swath of backward trajectories constructed from boundary layer between 990 and 850 mb. A preponderance of Arabian air trajectories do arrive over this region, however some continental air from India must also be conveyed to this region.
Above the boundary layer (900 mb and 850 mb levels), there is a hybrid structure. In the equatorial Indian ocean, the transport is generally from the northeast to southwest. Furthermore, there is transport downwards from as high as 500 mb (see the Jan 22 trajectory). The picture near the coastal Arabian sea (Feb. 2) is strikingly different. Air originates from about 400 to 500 mb in Saudi Arabia and descends over the Indian coast, possibly transporting mineral dust. The air travels eastwards and descends covering about 3000 km in less than 3 days. These are situations of cold outbreaks over northern India when the northeast monsoon is very shallow; the thermal wind driving these cold breaks turns the wind to westerlies (Figs 3d and 4d). For the most part, the relevant trajectories from northeast India that make it to the Indian ocean (and to the ITCZ) are those that originate in the lowest 1.5 kilometers.
The daily average global (direct + diffuse) solar flux in the 400 to 900 nm region is shown in Fig. 11. The minima in the solar flux occurs on January 18th and January 29th, which indicates very thick clouds. The surface flow analyses suggests that the clouds on these 2 days over the ship were associated with the ITCZ, i.e., precipitation systems. To illustrate the fundamental importance of transport in the aerosol radiative-forcing issue, we will consider 4 cases:
The low level convergence zones (and hence the ITCZ) are generally tilted from northwest to southeast direction (eg., see Fig. 3a, 4a, 12). In other words, in the eastern Indian ocean (>75°E) the ITCZ is closer to the equator, while in the western Indian ocean (<65°E), it is south of 15°S. As a result, as the ship sailed eastward (from day Jan 13 onwards), it should have encountered more precipitating clouds. This is indeed the case, as can be seen in Fig. 5 (the yellow regions) and also in the AVHRR images too(Jayaraman et al, 1997). This Northwest to southeast tilt has a remarkable impact on transport and aerosol distribution.
East of 80°E, the southern hemisphere air can penetrate as far as 10°N into the Arabian Sea (see for example, Jan 25 stream line, Fig. 15). At the same time, polluted and aerosol rich air, from the northern hemisphere can penetrate deep into the southern Indian ocean, as far as 20°S on the western Indian Ocean (eg., Fig. 15).
An important aspect is the fast time scales in which the ITCZ changes direction and intensity. A comparison of the low level convergence zones in Fig. 12, 14 and 15 attests to such changes. Because of the rapid change in the ITCZ and the steep northwest-southeast slope of the ITCZ, we conclude that during the north-east monsoon period there are significant inter-hemispheric transports taking place in this region.
Figure 9 shows that visible AODs can reach as high as 0.2 (12, 18 and 22 January) in the northern and southern hemisphere equatorial ocean (5°N to 5°S). We attribute these high values to strong northerly winds from the Indian sub-continent. The increase was accompanied by increase in the sulfate concentration to about 1.5 to 5 µg/m3 from the background value of about 0.5 µg/m3; similarly, mineral dust concentrations increased from essentially zero values to (Fig. 16) to 15-20 µg/m3. From Jayaraman et al (1997) we infer that the instantaneous radiative forcing at the sea surface can decrease by about 20 W.m-2 for an AOD of 0.2; diurnally averaged, the value can be as high as 10W.m-2.
Near the coastal ocean, the AODs increased by about 0.3 to 0.4, while the sulfates increased comparably. The 850 mb back trajectory suggests that part of the increase may be due to transport of mineral dust, as indeed supported by the mineral dust data (Figs. 6 and 16). According to the Jayaraman et al (1997), the coastal AODs of 0.3 to 0.4 should decrease the diurnally averaged solar insolation by about 20 to 30 W.m-2.
During the northeast monsoon, the aerosol concentrations measured over a large region of the Arabian Sea and the tropical Indian Ocean were much higher than one would expect, especially for the more distant southern hemisphere ocean regions. Meteorological studies show that high aerosol concentrations could be linked to transport from the India subcontinent and also from sources in the Middle East and North Africa. Our trajectory studies, especially Fig. 10 (d and e), confirms the possibility for the transport of Saharan mineral aerosols over these long distances. Although heavier aerosols may settle down (via dry deposition) these still remain a strong possibility for the lighter aerosols of Arabian (and also possible from the semi-arid regions of India and Pakistan) to make its way to the region offshore from southern India. The optical depth data sets, presented here, provide a strong case for their possibility.
The variations in aerosol concentration could be linked to the variability of the various radiation measurements that were being made concurrently aboard ship. On this basis we could infer that even relatively modest AOD values (0.2) could result in a decrease in the instantaneous radiative forcing at the sea surface by about 20 W.m-2. Such a large reduction in surface insolation has important climatological implications. Collectively, taking the aerosol and the radiation measurements and the computed four dimensional trajectories we are able to show that: a large gradient of the aerosols is indeed present downwind from the coast of southern India as we enter the Sagar Kanya Cruise area. Between the equator and 4°S we see values of sulfate concentrations as low as 0.5 (=5 gm/m3) to as high values as 3.9 (39 gm/m3) near the coast around 76°E. This confirms the presence of large concentrations of sulfates quite far away from the source regions and the presence of large gradients near the coast. However, before any firm conclusions can be made, it will be necessary to have a better understanding of the role that these aerosols play in both direct and indirect radiative forcing.
The aerosols are clearly impacted by congenital anthropogenic species as reflected in the high concentrations of NO3-, nss SO4=, NH4+. Because these species (especially nss SO4= and NH4+) are generally found in the radiatively-important submicron aerosol size fraction, we expect that the radiative properties of the aerosol will be largely controlled by these species. Nonetheless, mineral dust was a substantial component in most of the aerosol samples. Despite the fact that mineral dust is predominantly found in the supramicron size fraction, dust can play an important role in the radiative properties of the atmosphere (Li et al., 1996) and in the radiative forcing of climate (Tegen et al, 1996; Sokolik and Toon, 1996). Indeed, the aerosol in the Indian Ocean appears to be unusual in that dust and pollutants are usually mixed in relatively balanced proportions - that is, one component does not consistently dominate the other. For example, in many industrialized nations (e.g., the United States), mineral dust is a relatively minor component (Perry et al, in press); in contrast, in areas impacted by North African aerosols, dust overwhelms all other aerosol components (Li et al, 1996). Thus the winter monsoon Indian Ocean aerosol contains a unique mix of aerosol components that could have very unusual radiative properties. Intensive field campaigns such as those planned for INDOEX are necessary to characterize these aerosols and their radiative effects.
Although there is very little data on aerosol properties over the India Ocean, the data obtained during the cruise of the ORV Sagar Kanya are consistent with earlier measurements, some of which were made recently (Rhoads et al., 1997) and some in the late 1970's (Savoie et al., 1987; Prodi et al., 1983). Thus, the transport of continental aerosol to the equatorial Indian Ocean appears to be a persistent feature that is linked with the winter monsoon. Over the longer term, we might expect aerosol concentrations in this region to increase in concert with the rapid economic development that is taking place in this region, especially on the Indian subcontinent. To more accurately assess the current radiate forcing in this region and to characterize trends, we will need long-term measurements of aerosol and radiation at the surface.
This paper was supported under the INDOEX program of the University of California at San Diego. The U.S. author and co-authors thank the National Science Foundation, USA for funding this study through the Center for Clouds, Chemistry and Climate, La Jolla, CA. This is INDOEX Publication No. 7.