Genetics, Vol. 161, 381-388, May 2002, Copyright © 2002

A Neutral Model With Fluctuating Population Size and Its Effective Size

Masaru Iizukaa, Hidenori Tachidab, and Hirotsugu Matsudac
a Division of Mathematics, Kyushu Dental College, Kitakyushu 803-8580, Japan,
b Department of Biology, Graduate School of Sciences, Kyushu University, Fukuoka 810-8560, Japan
c Kyushu University, Fukuoka 812-8581, Japan

Corresponding author: Masaru Iizuka, Kyushu Dental College, 2-6-1 Manazuru, Kokurakita-ku, Kitakyushu 803-8580, Japan., iizuka{at}kyu-dent.ac.jp (E-mail)

Communicating editor: W. STEPHAN


*  ABSTRACT
*TOP
*ABSTRACT
*NEUTRAL MODEL WITH FLUCTUATING...
*TWO-VALUED MARKOV CHAIN MODEL
*DISCUSSION
*APPENDIX A
*APPENDIX B
*APPENDIX C
*LITERATURE CITED

We consider a diffusion model with neutral alleles whose population size is fluctuating randomly. For this model, the effects of fluctuation of population size on the effective size are investigated. The effective size defined by the equilibrium average heterozygosity is larger than the harmonic mean of population size but smaller than the arithmetic mean of population size. To see explicitly the effects of fluctuation of population size on the effective size, we investigate a special case where population size fluctuates between two distinct states. In some cases, the effective size is very different from the harmonic mean. For this concrete model, we also obtain the stationary distribution of the average heterozygosity. Asymptotic behavior of the effective size is obtained when the population size is large and/or autocorrelation of the fluctuation is weak or strong.


THE average heterozygosity has been one of the most frequently used measures of genetic diversity. A large amount of data have been accumulated to estimate the average heterozygosity of various species using protein electrophoresis (see, for example, NEVO 1978 Down; NEI and GRAUR 1984 Down; HAMRICK and GODT 1990 Down). Recent developments in molecular techniques such as randomly amplified polymorphic DNA (WILLIAMS et al. 1990 Down) and amplified fragment length polymorphism (VOS et al. 1995 Down) enable us to carry out estimation of the average heterozygosity at the DNA level by randomly sampling many short sequences in the genome and examining their variation. Using the methods such as those developed by CLARK and LANIGAN 1993 Down, LYNCH and MILLIGAN 1994 Down, and INNAN et al. 1999 Down, it is now possible to estimate genome-wide heterozygosity fairly easily using these techniques (e.g., MIYASHITA et al. 1999 Down).

One of the reasons that heterozygosity has been used for measuring genetic diversity is a simple relationship between its expectation and population genetic parameters under the neutrality assumption (KIMURA 1968 Down). For example, if we assume the infinite allele model in a haploid population of constant size N, the expected heterozygosity is expressed as , where u is the mutation rate (KIMURA and CROW 1964 Down). Since H is a monotone increasing function of Nu, one can obtain information on Nu from estimates of H.

The size of the population is, however, hardly constant and it may fluctuate from generation to generation. In such cases, it is necessary to understand how fluctuation of population size would affect genetic diversity and summary statistics such as H. For this end, the effects of fluctuation of population size on the effective size of population Ne must be clarified and a representation for Ne must be obtained. By this representation, the expected heterozygosity may be expressed as and it shows how the fluctuation of population size affects H.

Fluctuation of population size is not independent from generation to generation in general as in the case of stochastic selection (GILLESPIE 1972 Down; TAKAHATA et al. 1975 Down; GILLESPIE and GUESS 1978 Down; IIZUKA and MATSUDA 1982 Down; SENO and SHIGA 1984 Down; IIZUKA 1987 Down). In other words, the fluctuation of population size is most likely autocorrelated. In the literature, the effective size is said to be equal to the harmonic mean of the population size when population sizes are not constant (WRIGHT 1938 Down; CROW 1954 Down; NEI et al. 1975 Down; GILLESPIE 1998 Down). IIZUKA 2001 Down showed, however, that the effective size is not equal to the harmonic mean unless the fluctuation of population size is uncorrelated for the Wright-Fisher model with fluctuating population size. To obtain this result however, no mutation is assumed and the population size is fluctuating between two distinct states. These assumptions are restrictive. It is important to include the effect of mutation to investigate the influence of fluctuation of population size on genetic diversity of population. Further, two-state models may be very special and some of their conclusions do not hold for the general case. It is necessary to see whether or not the effective size is different from the harmonic mean for the general pattern of the fluctuation of population size.

In this article, we consider the diffusion model with neutral K (2 <= K <= {infty}) alleles whose population size is fluctuating randomly, incorporating the effect of mutation. First, we consider a general case with respect to the fluctuation of population size and we show that the effective size defined by the equilibrium average heterozygosity is larger than the harmonic mean of population size but smaller than the arithmetic mean of population size. Then we consider a special case of a two-valued Markov chain as a model of the fluctuation of population size. This simplification enables us to obtain explicit formulas for the stationary distribution of the average heterozygosity and the effective size. We can see quantitatively how the effective size is different from the harmonic mean using the latter formula.


*  NEUTRAL MODEL WITH FLUCTUATING POPULATION SIZE
*TOP
*ABSTRACT
*NEUTRAL MODEL WITH FLUCTUATING...
*TWO-VALUED MARKOV CHAIN MODEL
*DISCUSSION
*APPENDIX A
*APPENDIX B
*APPENDIX C
*LITERATURE CITED

Before we introduce the fluctuation of population size, we summarize some of the known results on the constant population model (CROW and KIMURA 1970 Down; EWENS 1979 Down). We consider a neutral locus with K alleles A1, A2, ... , AK in a randomly mating haploid population of constant size N. The mutation rate from Ai to all the other alleles is u per generation. Mutation occurs from Ai to Aj with the rate u/(K - 1) per generation (i, j = 1, 2, ... , K, j != i). Under the diffusion approximation (diffusion model), let xi(t) be the gene frequency of Ai at time t. We denote by [·] the operation taking the expectation with respect to the random sampling drift. Then the average heterozygosity

(1)

at time t satisfies the differential equation

(2)

(see Appendix A), which has the solution

(3)

and

(4)

where we put

(5)

Note that the case of K = {infty} is the infinite allele model (KIMURA and CROW 1964 Down). Note also that and . By this formula, the population size N can be expressed as

(6)

A large amount of ecological data suggest that numbers of individuals in natural populations fluctuate considerably in each epoch and from generation to generation (ELTON and NICHOLSON 1942 Down; ANDREWARTHA and BIRCH 1954 Down; ODUM 1959 Down). The variations in population size are influenced by such factors as climate, the abundance of available resources, fluctuation in prey-predator balance, and competition with other species using the same habitat (NICHOLSON 1957 Down). In addition to those short-term changes demonstrated by ecological data, long-term changes of population size have been inferred from past climate and fossil data. It is well known that there were at least seven glacial and interglacial cycles with a period of ~100,000 years in the last 700,000 years. Organismal populations were thought to have responded to such climate shifts by changing their habitats (WEBB and BARTLEIN 1992 Down). For example, many plant and animal species retreated to a few refugia in the southern parts of Europe during the last glacial period (BENNETT 1997 Down; HEWITT 2000 Down). Although these climate changes have strong cyclic components, biotic responses have many stochastic elements due to existence of physical barriers and species interaction. Thus, many species are thought to have experienced long-term stochastic changes of population size. Causes for long-term changes are not restricted to glacial cycles. Longer-term climate changes such as those in the last 3 million years (WEBB and BARTLEIN 1992 Down) and mountain building are among those. Thus, it is important to investigate fluctuation of population size in a general setting.

Now we consider the cases when population size fluctuates and let N(t) be the size of a haploid population at time t. In this article, we assume that {N(t)}-{infty}<t<{infty} is a stationary stochastic process that does not depend on gene frequencies {(x1(t), x2(t), ... , xK-1(t))}t>=0. In other words, the stochastic process that governs the change in population size is independent of the genetic structure of the population. We consider a diffusion model whose population size at time t is N(t) (for the precise meaning of this model, see Appendix A). This model is referred to as the neutral diffusion model with fluctuating population size and the case of K = {infty} is referred to as the infinite allele model with fluctuating population size. For this model, the average heterozygosity H(t) satisfies

(7)

(see Appendix A). The solution of this differential equation is

(8)

Note that {H(t)}t>=0 is a stochastic process induced by {N(t)}-{infty}<t<{infty}.

Let

(9)

and

(10)

be the arithmetic mean and the harmonic mean of N(t), respectively. Here E[·] is the operation taking the expectation with respect to the probability law of N(t). On the other hand, the effective size of population Ne can be defined as

(11)

by (6). Then we have

(12)

(see Appendix B). The effective size of the population is larger than the harmonic mean but smaller than the arithmetic mean by (12). Note that this result holds for any fluctuation of N(t) as far as 1/N(t) is integrable and H(t) is described by (7). This result is general in this sense but we cannot see how much Ne is larger than Nh or how much it is smaller than Na. For this end, we must consider a concrete example of the fluctuation of N(t), which is discussed in the next section. As we noted before, the effective size is said to be equal to the harmonic mean of the population size when population sizes are not constant in the literature (WRIGHT 1938 Down; CROW 1954 Down; NEI et al. 1975 Down; GILLESPIE 1998 Down). Our result shows, however, that this is not true for the neutral model with fluctuating population size. The fact that the effective size is not always the same as the harmonic mean was pointed out by IIZUKA 2001 Down for the Wright-Fisher model with fluctuating population size.


*  TWO-VALUED MARKOV CHAIN MODEL
*TOP
*ABSTRACT
*NEUTRAL MODEL WITH FLUCTUATING...
*TWO-VALUED MARKOV CHAIN MODEL
*DISCUSSION
*APPENDIX A
*APPENDIX B
*APPENDIX C
*LITERATURE CITED

To see how the effective size of population Ne depends on the probability law of {N(t)}-{infty}<t<{infty} and to what extent Ne is different from Nh and Na, we consider a special case of a continuous time two-valued Markov chain for {N(t)}-{infty}<t<{infty}. Let {N(t)}-{infty}<t<{infty} be a Markov chain on {N1, N2} such that

(13)

({Delta}t {downarrow} 0), where N1 < N2. Here, {gamma}i is the jump rate from the state Ni to Nj (j != i) and lim{Delta}t{downarrow}0 (o({Delta}t)/{Delta}t) = 0. Note that the stationary probabilities for N(t) = N1 and N(t) = N2 are

(15)


(16)

respectively, where we put

(17)

Note that r = 1/2 for the symmetric case of {gamma}1 = {gamma}2. The autocorrelation of {N(t)}-{infty}<t<{infty} can be defined by

(18)

where Var[N(0)] and Cov[N(0), N(t)] are the variance of N(0) and the covariance of N(0) and N(t), respectively. Since

(19)

where

(20)

we have

(21)

and N(t1) and N(t2) are positively autocorrelated (t1 != t2).

Let p(h, Ni) and p(h) be the stationary probability density functions of (H(t), N(t)) and H(t), respectively (i = 1, 2). Applying the results of MATSUDA and ISHII 1981 Down, we have

(22)


(23)

and

(24)

(H1 < h < H2), where

(25)


(26)

and

(27)

is the beta function (p, q > 0; see Appendix C). The stationary probability density function p(h) of the average heterozygosity is presented in Fig 1 for the case of K = {infty}, 2N1u = 0.1 (H1 = 0.09), and 2N2u = 1 (H2 = 0.5). The solid line, the dotted line, and the dashed line represent the cases of {alpha}1 = {alpha}2 = 0.5, {alpha}1 = {alpha}2 = 1, and {alpha}1 = {alpha}2 = 2, respectively. The stationary probability density function p(h) is bell shaped if {alpha}1, {alpha}2 > 1 (the jump rates {gamma}1 and {gamma}2 are large) and it is U shaped if 0 < {alpha}1, {alpha}2 < 1 (the jump rates {gamma}1 and {gamma}2 are small). Note that the equilibrium heterozygosity H({infty}) is a random variable due to the stochastic fluctuation of population size and the distribution function of H({infty}) is

(28)



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Figure 1. The stationary probability density function p(h) of the average heterozygosity for the case of , and . The solid line, the dotted line, and the dashed line represent the cases of , and , respectively.

(H1 < h < H2). Then we have

(29)

and

(30)

where

(31)

As noted above, the variance is due to the stochastic fluctuation of population size. Thus, the variance quantifies the extent of variation expected among average heterozygosities of independent populations whose sizes obey the same probability law. The variance should not be mixed up with that among the average heterozygosities of respective loci in one species, because those loci are considered to have experienced the same population history. The conditional stationary probability density function of H(t) given N(t) = N1 is

(32)

and that given N(t) = N2 is

(33)

Then the conditional expectation of H({infty}) given the population size being N1 is

(34)

and that given the population size being N2 is

(35)

Note that E[H({infty})|Ni] is the expectation of the equilibrium average heterozygosity knowing that the population size at the observation time is Ni. It is easy to see

(36)

as we expect. On the other hand, the conditional stationary probabilities of N(t) = N1 and N(t) = N2 given H(t) = h are

(37)

and

(38)

respectively. Note that p(Ni|h) is the stationary probability that the population size is Ni knowing that the average heterozygosity is h.

Now we have an explicit expression for Ne. By (11) and (29), we have

(39)

since

(40)

Note that Ne depends on the mutation rate u. By (39), Ne is an increasing function of the measure of autocorrelation {tau} (a decreasing function of {gamma}) if we fix the value of r (note that Nh does not depend on {gamma} if we fix the value of r). To see how much Ne > Nh, we consider the ratio of the effective size to the harmonic mean

(41)

where

(42)

and

(43)

The dependence of log10(Ne/Nh) on log10(N2/N1) is presented in Fig 2 for the case of {gamma}1 = {gamma}2, K = {infty}, and {theta}2 = 1. The solid line, the dotted line, and the dashed line represent the cases of {Gamma}2 = 0.1, {Gamma}2 = 1, and {Gamma}2 = 10, respectively. The ratio Ne/Nh can be very large if N1 << N2 and the jump rate {gamma} is not large. For example, if and . On the other hand, if and . Note that Ne/Nh and log10(Ne/Nh) are decreasing functions of the scaled mutation rate {theta}2 and the values of log10(Ne/Nh) for {theta}2 < 1 are larger than those in Fig 2 if we fix log10(N2/N1) and {Gamma}2.



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Figure 2. The dependence of log10 (Ne/Nh) on log10 (N2/N1) in the two-valued Markov chain model for the case of , and . The solid line, the dotted line, and the dashed line represent the cases of , and , respectively.

Noting that

(44)

we can express Ne in terms of Na and Nh,

(45)

where

(46)

and

(47)

(0 < RK < 1). Note that we have obtained explicit expressions for Ne [i.e., (39) and (45)] by introducing the two-valued Markov chain model.

The size of population N(t) may be very large in natural populations. Further, the autocorrelation of {N(t)}-{infty}<t<{infty} may be very weak or strong. In such cases, we can consider the asymptotic behavior of Ne. For this end, we parameterize N1, N2, Ne, Nh, Na, {gamma}1, {gamma}2, {gamma}, V, u, and RK by {epsilon} ({epsilon} -> 0) such as N{epsilon}1, N{epsilon}2, N{epsilon}e, N{epsilon}h, N{epsilon}a, {gamma}{epsilon}1, {gamma}{epsilon}2, {gamma}{epsilon}, V{epsilon}, u{epsilon}, and R{epsilon}K. Here, we assume that and do not depend on {epsilon} for simplicity. Note that N{epsilon}a/N{epsilon}h does not depend on {epsilon} in this case. For simplicity, we assume that the limits

(48)

and

(49)

exist (0 <= {Gamma}, {theta} <= {infty}). By

(50)

and (45), it is easy to see that

(51)

if {Gamma} = {infty} or {theta} = {infty},

(52)

if {Gamma} = 0 and {theta} = 0. The cases that {Gamma} = {infty}, 0 < {Gamma} < {infty}, and {Gamma} = 0 are referred to as weak autocorrelation, moderate autocorrelation, and strong autocorrelation limits, respectively. In the same way, the cases that {theta} = 0, 0 < {theta} < {infty}, and {theta} = {infty} are referred to as weak mutation, moderate mutation, and strong mutation limits, respectively. By (51) and (52), the effective size is asymptotically equal to the harmonic mean in the case of weak autocorrelation or strong mutation and the effective size is asymptotically equal to the arithmetic mean in the case of strong autocorrelation and weak mutation. Note that, in the case that r and b do not depend on {epsilon}, weak, moderate, and strong autocorrelation limits correspond to lim{epsilon}->0 , and lim{epsilon}->0 , respectively.

The Wright-Fisher model with fluctuating population size is investigated by IIZUKA 2001 Down. Let N(k) be the size of haploid population in generation k, where {N(k)}k=0,±1,±2,... is a two-valued Markov chain. This model is defined as the Wright-Fisher model with no mutation and no selection whose population size in generation k is N(k). For this model, the effective size N*e can be defined by

(53)

The effective size N*e is smaller than the harmonic mean if the change in population size is negatively autocorrelated, it is larger than the harmonic mean if the change is positively autocorrelated, and it is equal to the harmonic mean if the change is uncorrelated. These results are consistent with those for the diffusion model in this section. Note that the change in population size is positively autocorrelated in our formulation through the diffusion model in this section. In other words, the introduction of the fluctuation of population size after the diffusion approximation implies that this fluctuation cannot be uncorrelated or negatively autocorrelated. There are some properties on asymptotic behavior of the Wright-Fisher model with fluctuating population size that are consistent with those of the diffusion model in this section. For example, the effective size is asymptotically equal to the harmonic mean in the case of weak autocorrelation for both models (see IIZUKA 2001 Down).

The Wright-Fisher model with fluctuating population size is more fundamental than the diffusion model with fluctuating population size since the stochastic effect of fluctuation of population size is introduced after the diffusion approximation for the latter model. It seems not to be easy, however, to incorporate the effect of mutation into the Wright-Fisher model with fluctuating population size. It is easy to incorporate the effect of mutation into the diffusion model with fluctuating population size since the differential equation for H(t) is linear. Furthermore, we can consider a very general pattern of fluctuation of population size for the diffusion model with fluctuating population size as we have shown in this article.


*  DISCUSSION
*TOP
*ABSTRACT
*NEUTRAL MODEL WITH FLUCTUATING...
*TWO-VALUED MARKOV CHAIN MODEL
*DISCUSSION
*APPENDIX A
*APPENDIX B
*APPENDIX C
*LITERATURE CITED

Here, we discuss some biological relevance of our results. Suppose that we are interested in effects of selection on genetic variation in a species. Effects of weak selection depend on population size (OHTA 1973 Down, OHTA 1992 Down). Thus, it is important to obtain information on population size although this is usually very difficult by nongenetic means (see BASSET et al. 2001 Down for the problems that have to be dealt with by researchers when trying to estimate effective size using demographic parameters). One of the easiest things we can do is to estimate the effective size defined here by measuring the average heterozygosity at neutral loci such as those of pseudogenes. Then, we can guess what variation pattern would be expected for alleles with a selection coefficient s. In fact, effects of selection depend not only on the effective size but also on the details of how population size changes (see OHTA 1997A Down, OHTA 1998 Down). For example, the behavior of TAJIMA's (1989) D as a function of the intensity of selection is very different if the change rate of population size differs with the effective size being kept constant (TACHIDA 2000 Down). Nevertheless, we can use (39) to know what parameter combinations lead to the effective population size under the assumption of the two-state model and then examine effects of selection on the basis of this information. Although the two-state model is unrealistic and we need to extend theoretical studies for more general cases, at least we can obtain a rough idea as to how selection affects genetic variation in the species by measuring the effective population size. For the inference of the mechanism of molecular evolution under fluctuating population size, see also ARAKI and TACHIDA 1997 Down and OHTA 1997B Down.

TACHIDA 1985 Down developed a method to calculate the probabilities that two neutral genes taken at random from a population have certain allelic states, which is called the joint frequencies of alleles (see also GRIFFITHS 1981 Down). Using (29), we can extend this method to the case where population size is fluctuating. Let q(k) be the probability that two neutral genes taken at random from a population have k mutations since they diverged from their most recent common ancestor. Then the probability generating function of q(k)

(54)

is expressed as

(55)

where E[H({infty})]u->u(1-z) is the value of E[H({infty})] with the total mutation rate u being replaced by u(1 - z). Then we can obtain the joint frequencies of alleles by (6) of TACHIDA 1985 Down. We denote the effective size by Ne(u) as a function of mutation rate u. It is easy to see that the expectation of k is

(56)

since

(57)

and

(58)

where is the value of and is the value of dE[H({infty})]/du when u = 0. The same method may be applied to microsatellite allele frequencies. For example, (11a) of SLATKIN 1995 Down may be extended for the case where population size is fluctuating as follows. By (56) and (7) of SLATKIN 1995 Down, the right-hand side of (11a) of SLATKIN 1995 Down can be expressed as 2Ne(0)µ{sigma}2m, where µ and {sigma}2m are the parameters describing the mutation scheme for microsatellite alleles.


*  ACKNOWLEDGMENTS

We thank A. Shimizu for noting the result of DUDLEY 1989 Down on a modification of Jensen's inequality and two anonymous reviewers for valuable comments. M.I. was partially supported by a grant-in-aid (no. 12640139) from the Ministry of Education, Culture, Sports, Science and Technology of Japan. H.T. was supported in part by a grant from Program for Promotion of Basic Research Activities for Innovative Biosciences (PROBRAIN) and a grant from Uehara Memorial Foundation.

Manuscript received August 13, 2001; Accepted for publication February 11, 2002.


*  APPENDIX A
*TOP
*ABSTRACT
*NEUTRAL MODEL WITH FLUCTUATING...
*TWO-VALUED MARKOV CHAIN MODEL
*DISCUSSION
*APPENDIX A
*APPENDIX B
*APPENDIX C
*LITERATURE CITED

Let f(x1(t), x2(t), ... , xK-1(t)) be an arbitrary function of gene frequencies in the neutral diffusion model. We denote by [·] the operation taking the expectation with respect to the random sampling drift. By the general theory of diffusion processes (see EWENS 1979 Down, pp. 136–137, or KARLIN and TAYLOR 1981 Down, pp. 213–216), the expectation of f(x1(t), x2(t), ... , xK-1(t)) satisfies

(A1)

where

(A2)


Substituting

(A3)

for f(x1, x2, ... , xK-1) in (A1), we have

(A4)

Noting that

(A5)

we have (2) by (A1).

The neutral diffusion model with fluctuating population size is defined as a diffusion model with a random parameter by replacing N in (A2) with the stationary stochastic process N(t). In other words, this model is defined as a diffusion process in random environments. We have (7) in the same way as we have (2).


*  APPENDIX B
*TOP
*ABSTRACT
*NEUTRAL MODEL WITH FLUCTUATING...
*TWO-VALUED MARKOV CHAIN MODEL
*DISCUSSION
*APPENDIX A
*APPENDIX B
*APPENDIX C
*LITERATURE CITED

For a function f(x) with

(B1)

for any x, y, and t (x != y, 0 < t < 1), and for a random variable X, we have

(B2)

unless almost surely (see DUDLEY 1989 Down, problem 14 in p. 276). Note that this result is a modification of Jensen's inequality (see FELLER 1971 Down, pp. 153–154). By applying (B2) for , we have

(B3)

and

(B4)

By (B4) and the definition of Ne in (11), we have

(B5)

By using the inequality (B2) again for , we have

(B6)

and

(B7)

Then we have

(B8)

by (B7) and (11).


*  APPENDIX C
*TOP
*ABSTRACT
*NEUTRAL MODEL WITH FLUCTUATING...
*TWO-VALUED MARKOV CHAIN MODEL
*DISCUSSION
*APPENDIX A
*APPENDIX B
*APPENDIX C
*LITERATURE CITED

For the two-valued Markov chain model, (7) can be expressed as

(C1)

if , where

(C2)

We can regard (C1) as an ordinary differential equation, one of whose parameters stochastically changes. Note that H1 <= H(t) <= H2 if H1 <= H(0) <= H2.

By (2.17) of MATSUDA and ISHII 1981 Down, the stationary probability density function p(h, Ni) of (H(t), N(t)) is given by

(C3)

(H1 < h < H2), where C is the normalization constant. By this formula, we have (22) and (23).


*  LITERATURE CITED
*TOP
*ABSTRACT
*NEUTRAL MODEL WITH FLUCTUATING...
*TWO-VALUED MARKOV CHAIN MODEL
*DISCUSSION
*APPENDIX A
*APPENDIX B
*APPENDIX C
*LITERATURE CITED

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