<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 />
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