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<br />514 <br /> <br />JOURNAL OF CLIMATE AND APPLIED METEOROLOGY <br /> <br />VOLUME 23 <br /> <br />analysis space which is congruent to the data space <br />being investigated (Mielke and Berry, 1983; Mielke et <br />al., 1982). Then the MRPP statistic used in this study <br />is given by <br /> <br />g (ni) <br />t5=L N ~i, <br /> <br />,~1 <br /> <br />where ni ;;;. 2 is the number of objects in group Si <br />(i = 1, . . . , g), <br /> <br />g <br />N= Lni, <br />i~1 <br /> <br />( )-1 <br />ni <br />~i = 2 <br /> <br />L A/,Jtfii(WI)tfii(WJ) <br />I<J <br /> <br />is the average between-object distance for all objects <br />within group Si (i = 1, . . . , g), L is the sum over all <br />I<J <br />I and J such that 1 .,;; 1< J.,;; N, and tfii(WI) is 1 if WI <br />belongs to Si and 0 otherwise (i = 1, . . . , g; I = 1, <br />. . . , N). The underlying permutation distribution of <br />15 (the null hypothesis) assigns equal probabilities to <br />the <br /> <br />g <br />M = N!(II ni!)-l <br />i~l <br /> <br />possible allocations of the Nobjects to the g groups. <br />Since small values of 15 imply a concentration of re- <br />. sponse measurements within at least some of the g <br />groups, the null hypothesis is rejected when the ob- <br />served value of 15 is small. The exact P-value (i.e., the <br />probability under the null hypothesis of a value of 15 <br />being as or more extreme than the observed value of <br />15) is the proportion of all M values of 15 which are <br />equal to or less than the observed value of 15. Berry <br />(1982) has developed an efficient algorithm for cal- <br />culating exact P-values; it is practical for values of M <br />up to 20 000. EffiCient and accurate moment approx- <br />, imation procedures exist for calculating P-values for <br />large values of M (Mielke, 1979; Mielke et ai" 1976, <br />1981a, 1982). It should be noted that when a single <br />response variable is analyzed, then MRPP is a uni- <br />variate analysis procedure. However, the term MRPP <br />will designate both univariate and multivariate analyses <br />in this paper. <br /> <br />3. Preliminary sample size estimates <br /> <br />Because the power characteristics of permutation <br />tests, such as the MRPP, are highly dependent upon <br />both the actual distribution and the hypothesized al- <br />ternative in question,' it is important that reasonable <br />approximations be obtainable for both these entities. <br />To this end, a simulation program was designed to <br />yield power-characteristic results and sample size es- <br />timates forHIPLEX-l. The data base for this simu- <br />lation consisted of measurements on CIC5, TFPI, and <br />PIC8 collected on 35 clouds (11 of which were seeded) <br /> <br />as part of the calibration seeding trials during the sum- <br />mer of 1978 and prior to the actual experiment. Ap- <br />pendix E of the design document (Bureau of Recla- <br />mation, 1979) provides details of the data set. From <br />this data base, four sets of random samples (N = 50, <br />100, 150, and 200) were drawn with replacement. <br />For analyses involving more than a single response <br />variate (i.e., joint effects), the investigator must insure <br />that the response measurements are commensurate, <br />i.e., the sample ranges of the different response variates <br />must be equalized. Let the kth response measurement <br />for a seeded case be represented by XkjS (k = 1, . . . , <br />rand) = 1, . . . , ns); similarly, let the kth response <br />measurement for a nonseeded case be represented by <br />XkjNS (k = 1, . . . , rand) = 1, . . ., nNS)' Seeded and <br />nonseeded variates of the kth response measurement <br />are respectively denoted by <br /> <br />. YkjS = bkNS(akS + CkSXkjS)} , <br /> <br />YkjNS = bkNS(XkjNS) <br /> <br />where bkNS is a commensuration adjustment, akS is. a <br />location adjustment, and CkS is a scale adjustment for <br />the kth response measurement. In this way, the input <br />for the MRPP simulation program was generated; val- <br />ues for akS, bkNs, and CkS for CIC5, TFPI, and PIC8 <br />are given in Table 1. Response variables CIC5, TFPI, <br />and PIC8 were considered most important at the time. <br />The definitions of 1) all primary and secondary re- <br />sponse variables and 2) the final test statistics are given <br />in Table 2. Values of bkNS were based on the observed <br />ranges. Since prior information on akS and CkS did not <br />exist, these initial values were based on a concensus <br />judgment by the HIPLEX-l investigators. <br />Given the specified adjustments of Table 1, the re- <br />sults of the MRPP computer simulation, using the <br />four sets of random samples (N = 50, 100, 150, and <br />200) with ns = nNS = N12, indicated that 50-150 test <br />cases of a given class of cloud (25~ 7 5 each of seeded <br />and nonseeded clouds in a given class) would be re- <br />quired to reject the null hypothesis with a = 0.10, <br />where a is the probability of a type-I statistical error. <br />Unfortunately, because 1) the summer of 1980 was <br />extremely dry in eastern Montana, 2) HIPLEX-l was <br />pre-empted by the Cooperative Convective Precipi- <br />tation Experiment (CCOPE) in the summer of 1981, <br />and 3) the funding for HIPLEX-l was suddenly ter- <br /> <br />TABLE I. Specified changes associated with the location adjustment <br />OkS, the commensuration adjustment bkNS, and the scale adjustment <br />CkS of the three response variates CIC5, TFPI, and PICS, <br /> <br /> . Adjustment <br />Response <br />variate OkS bkNS CkS <br />CIC5 5.0 1.0 1.0 <br />TFPI 0.0 2.4 0.6 <br />PICS 0.2 16,0 1.0 <br />