The impact of cumulus congestus clouds on mid
Transcription
The impact of cumulus congestus clouds on mid
METHODS INTRODUCTION Ozone (O3) is rapidly destroyed in the remote tropical marine boundary layer [6, 13]. This ozone depleted marine boundary layer air is injected into the free troposphere by convection, where it is chemically produced at a rate of 1 - 2 ppbv per day [5]. This rate of production gives rise to a chemical replacement timescale which is comparable with the overturning timescale for the Hadley circulation. Ozone is therefore a useful tracer for diagnosing convective motions in the tropics. Ozone measurements have been used to demonstrate the existence of strong convective outflow in the upper troposphere from deep convection [3, 4, 9, 12]. At present, however, the evidence for the existence of preferred convective detrainment near the melting level due to congestus (towering) clouds (Figure 1) arises mainly from measurements of cloud top heights [1, 17], mass divergence [10, 11, 15], and relative humidity [7]. Here, we present additional evidence for the existence of mid-level cumulus congestus outflow using O3 measurements. We also use the O3 simulation in a chemical transport model (GEOS-Chem) to examine the representation of convective outflow in a widely-used assimilated meteorological dataset (GEOS-4 and GEOS-5). Negative mid-tropospheric ozone anomalies (>8 ppbv) are temporally confined within 10-hour belt about peak rainfall. The divergence anomaly patterns indicate that the negative midlevel ozone anomaly preceding peak rainfall can be attributed to outflow from cumulus congestus clouds. We also examined the ozone and divergence anomaly patterns about high rain events in the GEOS-4 and GEOS-5 meteorology in the GEOSChem model. In addition, we examined the divergence anomaly pattern about high rainfall events of a higher resolution GEOS-5 YOTC meteorological dataset [16] (0.25x0.33 deg.) at 12 locations in the tropical Pacific. Toni Mitovski, Dalhousie University, Halifax, Canada Email: mitovski@dal.ca Figure 1. The boundary layer air is detrained near the melting level (congestus) and near the tropopause (deep convection). Figure 2. Area of interest. Data availability temporal resolution horizontal resolution TRMM 3B42 1998-2010 3-hrs 2.0° SHADOZ 1998-2010 bi-weekly 2 stations 691 IGRA 1998-2010 12-hrs 2 arrays >10,000 GEOS-4 & GEOS-5 2004-2006 2D (3-hrs) 3D (6-hrs) 2.0°x2.5° 2009 2D (1-hr) 3D (3-hrs) 0.25°x0.33° GEOS-5 YOTC Figure 3. Rain frequency distribution for various datasets Figure 4. TRMM 3B42 rainfall over Samoa for Oct. 2008. We used all rain events above a rain threshold of 1.5 mm/h (red line). We stored only those SHADOZ soundings that had occurred within 24 hrs about the rainfall events. RESULTS a) Table 1. Data and models used in this research. Poster Design & Printing by Genigraphics® - 800.790.4001 The composite anomaly patterns at both Fiji and Samoa were constructed using the following procedure: High rainfall events were defined as those which exceeded a threshold of 1.5 mm/hr; We then searched for SHADOZ soundings that had occurred within 24 hours of each rain event (Figure 4). For the chosen threshold of 1.5 mm/hr, there were approximately 300 soundings available from both Fiji and Samoa; At both Fiji and Samoa, we defined seasonal mean ozone profiles (DJF, MAM, JJA, SON) using the 12 years available (1998 – 2010). The appropriate seasonal mean was then subtracted from each of the 300 ozonesondes within 24 hours of a rain event to generate an instantaneous deviation of the ozone mixing ratio from the seasonal climatology; Using the difference between the ozonesonde launch time and the time of each rainfall event, the ozone deviations were grouped into 3 hour time bins. The anomaly patterns for Fiji and Samoa were similar to each other and were therefore combined into one shown in Figure 5(a). Divergence anomaly patterns (Figure 6(a)) were constructed using simultaneous wind measurements from two triangular arrays (Figure 2) of radiosondes and the same procedure as described before with exception that here, we used an array averaged TRMM rainfall. There were 805 divergence profiles within 24 hours of a rain event from Array 1, and 1339 profiles within 24 hours of a rain event from Array 2. DATA The data and models used in this research are summarized in Table 1. We used data from 2 SHADOZ locations (Fiji and Samoa) and from 2 IGRA arrays to construct ozone and divergence anomaly patterns about high rain events. Figure 2 shows the SHADOZ and the IGRA locations. DISCUSSION The selection of a rain event threshold for Fiji and Samoa requires making some compromise between the number of rain events and their intensity. We wanted the rain event threshold to be sufficiently large that the rain events would be associated with deep convection, and give rise to significant deviations in ozone mixing ratios from background. On the other hand, the rainfall event threshold had to be sufficiently small that a statistically representative number of ozonesonde profiles would be available to construct the ozone anomaly patterns. Figure 3 shows the frequency distribution of the rainfall using a variety of data. Due to more frequent light precipitation in the models than in the TRMM, we used a smaller rain threshold of 1.0 mm/h, rather than 1.5 mm/h. c) b) a) b) d) c) d) number of soundings Figure 5. Ozone anomalies about peak rainfall (t=0) calculated using: a) SHADOZ, and GEOS Chem with b) GEOS-4 and d) GEOS-5 meteorology. Panel c) shows the strength of the signal and the significance (within the boxes) of the ozone anomalies in panel a). The rain variability about t=0 is plotted under the panels. Figure 6. Divergence anomalies about peak rainfall (time=0) calculated using: a) radiosonde arrays, b) GEOS-4, c) GEOS 5 (YOTC), d) GEOS-5 meteorology. The rain variability about t=0 is plotted under the panels. In SHADOZ (Figure 5(a)), negative ozone anomalies start to develop at mid-levels (4-8 km) about 16 hours prior to maximum rainfall. The mid-level ozone anomaly intensifies as peak rainfall approaches. At peak rainfall (t = 0), the ozone anomaly extends from 4 km to 15 km. The divergence pattern (Figure 6(a)) exhibit convergence near the surface prior to peak rainfall, an upper level divergence near 13 km associated with deep convection, and an antisymmetric divergence dipole near 6 km. The divergence dipole consists of a congestus divergence roughly 8 hours prior to peak rainfall, and a stratiform convergence 8 hours after peak rainfall. With GEOS-4 meteorology (Figure 5(b)), convection gives rise to two broad negative ozone anomalies, centered at 6 km and at 15 km. The anomalies are more persistent and are about 5-fold weaker than the observations, extending from more than 24h prior to peak rainfall, to more than 24h after peak rainfall. A broad upper tropospheric divergence is about 3-fold weaker than in the observations (Figure 6 (b)). With GEOS-5 meteorology, the ozone (Figure 5(d)) and divergence (Figure 6(d)) anomaly patterns are almost identical as with GEOS-4. However, the ozone anomalies and the upper level divergence with GEOS-5 are stronger than with GEOS-4, presumably due to stronger rain at t=0. In GEOS-5 YOTC (Table 1), overall structure of the YOTC divergence anomaly pattern (Figure 6(c)) is quite similar to the IGRA divergence anomaly pattern. However, there is a vertical offset between the congestus and stratiform divergence features that is not observed, and both features occur too close to peak rainfall. CONCLUSIONS 1. The negative mid-level ozone anomalies that develop prior to peak rainfall observed in the SHADOZ dataset are likely to be a result of the vertical transport of ozone depleted boundary layer air within congestus clouds, followed by detrainment (divergence) at mid-levels. 2. Two negative ozone anomaly features in GEOS Chem are much broader than observed, likely due to lower rainfall variability (about t=0) in GEOS-4 and GEOS-5. Quantitatively, the anomalies are comparable to the observations in GEOS-5, and are 5-fold weaker in GEOS-4. 3. In GEOS-4 and GEOS-5 meteorology, including GEOS-5 (YOTC), there is no evidence of a congestus outflow mode that precedes deep outflow, as occurs in the observations. REFERENCES 1. Dessler, A. E., S. P. Palm, and J. D. Spinhirne (2006), Tropical cloud-top height distributions revealed by the Ice, Cloud, and Land Elevation Satellite (ICESat)/ Geoscience Laser Altimeter System (GLAS), J. Geophys. Res., 111, D12215, doi:10.1029/2005JD006705. 2. 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