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<br />APRIL 1990 DESHLER, REYNOLDS AND HUGGINS 303 <br /> TABLE 2. Seedline penetrations on 18 December 1986 by the cloud physics aircraft. <br /> Penetration Age of Mean Mean Mean <br /> Advection time seedline Dispersion 2D.C 2D-P FSSP LWC <br />Seedline (degJm S-l) (min:sec) (min) (m S-l) (L-1) (L-1) (cm-3) (g m-3) <br />P3 196/17.3 1803:00 0 2 <I <I 0.01 <br /> 1807:20 5 <I 0 15 0.0 <br /> 1810:55 8 5.6 8 1 99 0.04 <br /> 1815:12 12 7.5 16 3 62 0.08 <br /> 1819:20 16 6.6 16 3 51 0.12 <br /> 1822:55 20 5.3 17 2 47 0.10 <br /> 1826:05 23 6.5 19 3 58 0.14 <br /> 1831:10 28 5.4 20 2 168 0.28 <br /> 1833:50 31 4.4 23 2 61 0,12 <br /> 1836:30 34 <I <I 14 0.0 <br />SI 208/17,3 1923:55 43 1.4 42 9 4 0.03 <br /> 1927:00 46 2.0 47 11 71 0,05 <br />S2 208/15.5 1859:44 9.5 1.3 13 0 47 0.03 <br /> 1900:25 9 1.7 5 <I 59 0.08 <br /> 1909:24 19 0.9 32 I 26 0.01 <br /> 1913:28 22 1.0 45 <I 38 0.02 <br /> 1921:25 30 0.8 49 4 15 0.01 <br /> 1929:45 39 0.8 37 6 42 0.03 <br />S3 208/15,5 1856: 10 0 4 <I 87 0.20 <br /> 1902:05 4 3 <I 67 0.14 <br /> 1907:54 12 1.5 15 <I 67 0.07 <br /> 1914:47 19 0.4 15 <I 118 0,20 <br /> 1919:50 24 0.8 57 4 37 0.06 <br /> 1931:25 35 0.9 30 7 16 0,01 <br /> <br />tion, measurements by the CSIRO and JW (not shown) <br />liquid water probes are comparable indicating that <br />there were no cloud drops> 40 JLm, assuming the large <br />drops are the major cause of differences between the <br />probes. <br />The growth of ice crystals in the seedline can be seen <br />both in the images and in the gray scale plots of ICC, <br />Fig. 8. The images observed at S2 + 30 and S2 + 39 <br />suggest that aggregation was taking place, accounting <br /> <br />I.E.09 <br /> <br /> <br />;-- I.Et08 <br />Ie <br /> <br />z I.E.07 <br />Q <br />I- <br />~ I.E.06 <br />I- <br />z <br />w <br /><.> I.E.O!l <br />z <br />o <br /><.> <br /> <br />I.E.04 <br /> <br />I.E.03 <br />.001 <br /> <br />.01 <br /> <br />.1 <br /> <br />1.00 <br /> <br />DIAME TER (mm) <br /> <br />FIG. 10. Particle spectra from the 2D.C and 2D-P during <br />penetrations ofS2 at 9,5,23,31, and 40 min. <br /> <br />for some of the larger particles indicated on Fig. 8; <br />however, the predominant particles were small rimed <br />crystals. Notice that cloud droplet concentrations di- <br />minished with time in S2; although at 39 min when <br />the aircraft had descended 300 m below the treatment <br />level there was substantial liquid water on the edges of <br />S2, suggesting that particles were falling into higher <br />liquid-water regions. Composite particle spectra from <br />the 10 to 39 min penetrations of S2 are shown in Fig. <br />10. The spectra indicate that small particles continued <br />to nucleate for 23 min before they diminished, while <br />the concentration oflarger particles was still increasing <br />at 39 min, 300 m below the seedline. <br /> <br />10. <br /> <br />(ii) Radar measurements <br /> <br />To search for seeding effects two techniques were <br />used to analyze the radar data. The simplest approach <br />was to advect seedlines across PPI elevation scans. To <br />do this an advection incorporating a wind field chang- <br />ing with height had to be used. The OTM provided <br />this capability; although it advects crystals to the surface <br />whereas echo advection would be faster since it is not <br />affected by the slower winds at the surface. To account <br />for the intermediate advection, between that measured <br />by aircraft and that calculated by the OTM, an average <br />of the two was used. The result, 14.6 m S-I from 2020, <br />was used to advect seedlines on the PPI plots. Radar <br />reflectivity patterns orienting themselves with seedlines <br />could then be considered evidence of seeding effects. <br />