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<br />1.5 <br /> <br /> <br />s <br />g 1.2 <br /> <br />.~ 0.9 <br />10 <br />a. <br />:~ 0.6 <br />o <br />>- <br />~ 0.3 <br />c: <br />w <br /> <br />0.0 <br />o <br /> <br />30 <br /> <br />60 <br /> <br />90 <br /> <br />120 <br /> <br />150 <br /> <br />Simulation Time (min) <br /> <br />1.5 <br /> <br />I <br />I <br />I <br />I <br />I <br />I <br />I <br />I <br />I <br />I <br />I <br />I <br />I <br />I <br />I <br />I <br />I <br />I <br />I <br /> <br />~ <br />-01.2 <br /> <br /> <br />:::. <br /> <br />180 <br /> <br />c: <br />,g 0.9 <br />Cll <br />a. <br />:~0.6 <br />o <br />>- <br />~0.3 - <br />c: <br />W <br />0.0 <br />o <br /> <br />5 <br /> <br />10 15 <br />Charge (C) <br /> <br />20 <br /> <br />25 <br /> <br />vM.Ult.lC,. e.IMflE"" AT TtlC- .I.INlI~H <br />HOCflNCJIITIIIIHOH '",I <br /> <br />vM.UCt.CE. ...........lIT fllll- 41,N11111 <br />!<<AI CGHCItITUTlOH ~"'J <br /> <br />VAL.IJII,QI. ..1Mn..NATTlHE. 41..111111 <br />TOULfLOllJ,IU IClIIIGl <br /> <br /> <br /> <br /> <br />r. <br /> <br />Figure 9 - Energy dissipation (1010 J) vs. time (top left), energy dissipation vs. charge transfer (top right), <br />total cloud ~ 0.1 g/kg (bottom left), NO mixing ratio ~ 1 ppbv (middle), N02 mixing ratio ~ 0.5 ppbv (bottom <br />right) at 90 min for 10 July 1996 STERAO simulation. <br /> <br />SE cloud in significant concentrations. In contrast <br />the NO mixing ratio is decaying following the <br />cessation of lightning activity in the other two cells. <br />This is even more evident in the N02 plot. <br />Interestingly, there is a plume of N02 to the <br />surface similar to that seen in the simpler 3D run <br />shown in Fig. 8. <br />In general the model did a reasonable job of <br />predicting the NOx mixing ratios in a qualitative <br />sense, but over-predicted the absolute values by <br />about an order of magnitude. Zhang (2002) <br />determined that there are several modifications <br />that can be made to the model to bring the results' <br />in harmony with the observations without <br />compromising the physics. Some of the more <br />important modifications include addition of <br />radiative transfer effects within the model cloud, <br />using the breakeven field for lightning initiation <br />rather than the breakdown field (Marshall et al., <br />1995; MacGorman et al., 2001), and adding a <br />pressure (altitude) dependence to the NO <br />production rate for lightning (Wang et al., 1998). <br />These modifications are currently pending. <br />As can be seen, much progress has been <br />made in the 30+ years since Dr. Orville and his <br />students and colleagues pioneered the inclusion of <br />electrical effects in multidimensional, coupled <br /> <br />cloud models. Interestingly, since the initial work <br />on the influence of electric forces on cloud <br />dynamics and microphysics, little has been done <br />in this area using more recent and more <br />sophisticated models. The primary reasons for <br />this are that early studies indicated potential <br />effects to be small, there is lack of detailed <br />information on how charges and fields might <br />influence interaction coefficients (collision <br />efficiencies, etc.), and the prevalent thinking (right <br />or wrong) is that other areas related to cloud <br />electrification are more worthy of study. <br /> <br />4. WHERE ARE WE NOW? <br /> <br />Currently there are two high resolution, <br />coupled, 3D models - the SO Tech SEM and the <br />Univ. of Oklahoma/NSSL model (as used by <br />MacGorman et al., 2001 and Mansell et al., 2002), <br />being used to simulate the electrification of storms. <br />Both models have small ions, inductive and <br />noninductive processes, and a lightning scheme. <br />There are some differences between the models <br />with respect to microphysics and lightning <br />schemes, but for the most part they have similar <br />capabilities. These models are state-of-the-art <br />and are being used to address the critical issues <br /> <br />44 <br />