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Testing for Asymmetrical Gene Flow in a Drosophila melanogaster Body-Size Cline
W. Jason Kenningtona, Julia Gockela, and Linda Partridgeaa Department of Biology, University College London, London WC1E 2BT, United Kingdom
Corresponding author: Linda Partridge, University College London, Darwin Bldg., Gower St., London WC1E 2BT, United Kingdom., l.partridge{at}ucl.ac.uk (E-mail)
| ABSTRACT |
|---|
Asymmetrical gene flow is an important, but rarely examined genetic parameter. Here, we develop a new method for detecting departures from symmetrical migration between two populations using microsatellite data that are based on the difference in the proportion of private alleles. Application of this approach to data collected from wild-caught Drosophila melanogaster along a latitudinal body-size cline in eastern Australia revealed that asymmetrical gene flow could be detected, but was uncommon, nonlocalized, and occurred in both directions. We also show that, in contrast to the findings of a previous study, there is good evidence to suggest that the cline experiences significant levels of gene flow between populations.
ASYMMETRY in the movement of individuals and genes between populations affects both the ability of populations to adapt locally (e.g., ![]()
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In studies where asymmetrical gene flow has been reported, it has been inferred either from differences in the level of linkage disequilibrium within populations (e.g., ![]()
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Here, we describe a test for detecting deviations from symmetrical gene flow between two populations, using microsatellite data that are based on differences in the proportion of private alleles. The utility of this method is demonstrated by assessing the extent of asymmetrical gene flow in a Drosophila melanogaster latitudinal body-size cline on the east coast of Australia (![]()
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| MATERIALS AND METHODS |
|---|
Fly collections:
Wild D. melanogaster were collected from rotting fruits or baited traps at 16 different latitudes from a 3000-km north-south transect along the east coast of Australia during January and February 2000 (Fig 1). This transect includes sites 200 km farther north than the lowest-latitude site collected by ![]()
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Microsatellite genotyping:
DNA extraction from individual flies, PCR protocols, and allele scoring followed methods outlined in ![]()
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Data analysis:
Measures of genetic variation, such as expected heterozygosity and the variance in repeat number, were calculated for each site using the MICROSAT v1.4 software package (![]()
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values, an unbiased estimate of FST (![]()
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The significance of pairwise
values, hereafter referred to as pairwise FST, was tested by permuting genotypes rather than alleles among samples, as this is the preferred method when Hardy-Weinberg is rejected within samples (![]()
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Spatial patterns of variation at each locus were summarized by II values, a spatial autocorrelation statistic designed specifically for DNA data (![]()
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Tests for asymmetrical migration between adjacent populations:
We based our test of asymmetrical migration on the idea that asymmetry in gene flow between two populations will lead to asymmetry in the proportion of private alleles (number of unique alleles/total number of alleles). To explore this further, we carried out forward simulations that were based on a model that portrays two populations capable of exchanging migrants each generation. Individuals were haploid and the number of individuals within each population was held constant. Populations were founded with no genetic variation. Generations were nonoverlapping and had the following steps: mutation, Wright-Fisher sampling, and migration. The mutation process followed a strict stepwise model and allele size was unconstrained.
We ran a variety of models with different numbers of loci, levels of asymmetrical migration, and numbers of migrants. Each model ran for 2000 generations and each was repeated 1000 times. We found that, with equal population sizes, most distributions of the difference in proportion of private alleles (
PPA) between populations were significantly different from zero [i.e., zero was outside the 95% confidence limits (CL)] when migration was unidirectional and the number of loci was at least 10 (data not shown). However, with more modest levels of asymmetry (<4:1), the differences between populations became less, and the distributions were not significantly different from zero. Even so, in all cases of asymmetrical migration, the mean of the distribution was negative, indicating that the proportion of private alleles was higher, on average, in the population receiving more migrants. The CL were sensitive to both the number of loci and the number of migrants each generation, increasing in range as both these parameters decreased.
On the basis of these results, we developed a test to detect asymmetrical migration between two populations by calculating the CL for a null model that assumed symmetrical migration. From earlier simulations we had found that the magnitude of the CL was dependent on the product of the population size (N) and mutation rate (µ), but not on N and µ independently. It was also apparent that the CL stabilized relatively soon after populations were initiated, long before they had reached mutation-drift equilibrium (Fig 2). Since the variance in repeat number is an estimator of Nµ (![]()
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PPA fell outside the 95% CL.
|
To calculate
PPA between adjacent sites we split the sites into two groups, A and B sites (the northern- and southernmost sites at each latitude, respectively). This ensured that there was an independent set of site comparisons for each pair of adjacent latitudes. In this way we could assess whether any deviations from symmetrical migration observed along the cline were systematic or not. In cases where there was a difference in the number of microsites sampled in a site comparison (i.e., one vs. two or vice versa), then only one microsite from each site was used. To further reduce any potential bias due to differences in sample size, we resampled the minimum number of alleles at each locus with replacement for each site comparison 100 times. The proportion of private alleles in each locus was calculated by dividing the total number of private alleles by the total number of alleles.
| RESULTS AND DISCUSSION |
|---|
Variation within sites:
Expected heterozygosity and variance in repeat number, both averaged over loci, ranged from 0.59 to 0.70 and 5.9 to 10.9, respectively. On average, these estimates were 1.3 (expected heterozygosity) and 2.8 (repeat variance) times higher than those reported in a recent microsatellite survey of isofemale lines from eastern Australia (![]()
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The higher levels of variability observed in low-latitude sites might reflect larger effective population sizes or be a consequence of colonization history. In agreement with the second hypothesis, ![]()
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Population structure:
Pairwise population differentiation tests revealed that there was no significant genetic differentiation between microsites at any one site (i.e., over distances of 0.0050.4 km) or between sites within latitudes after microsite data within each site had been pooled (i.e., over distances of 2.850.4 km, data not shown). This was confirmed with AMOVA, which revealed no significant genetic structure between microsites within sites or between sites within latitudes when microsites were pooled (variance components were negative and 0.28% of the total variance, respectively). However, there was a low, but significant level of population substructuring between latitudes (variance component = 2.19%; P < 0.001).
As expected, the level of population differentiation increased with the geographic distance between sites (Mantel test, P < 0.001). Interestingly, and in contrast to ![]()
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The apparent absence of an effect of geographic distance on genetic differentiation on the Australian mainland led ![]()
A second difference from the results of ![]()
Autocorrelation coefficients for 500-km distance classes are given in Table 2. In most cases II values did not exceed 0.1. This reflects the small interpopulational differences along the cline and the high variability within sites. Despite this, most loci showed significant departures from randomness. Overall, a common pattern was shown by most loci whereby II values were positive and significant at distance classes up to 500 km and near zero and nonsignificant at intermediate distance classes. Thereafter, two main patterns emerged. The first was that II values became increasingly more negative and significant with greater distance (e.g., AC005555, AC004759, DMU14395, DMU25686, AC008193, and DMU1951). This pattern is identical to the one observed for clines in allele frequencies both in simulation (![]()
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The loci with the most pronounced clinal autocorrelation profiles were DMU25686, AC008193, and DMU1951. These loci occur within the common cosmopolitan inversion In(3R)Payne, which is known to vary clinally with latitude on several continents and is hence thought to be under selection (![]()
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Clinal autocorrelation profiles at other loci might also be associated with chromosomal inversions under selection. For example, the locus AC005555 is located within the inversion In(2L)t and DMU14395 is located within the inversion In(3L)Payne. As with In(3R)Payne, these inversions vary latitudinally on several continents and are thought to be under clinal selection (![]()
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Because parallel patterns of geographic variation at a number of loci are taken as evidence that factors affecting the entire genome are responsible (![]()
Tests of asymmetrical migration:
Pairwise comparisons of the proportion of private alleles within adjacent populations along the cline are given in Table 3. Taking into account differences in the variance in repeat number between sites, there were only nine instances (out of the 30 possible comparisons) where
PPA deviated significantly from a null model of symmetric migration at a level of five individuals (10 gametes) per generation. When the level of symmetric migration was reduced to one individual per generation, there were only three instances where the null model was rejected. Overall, pairwise comparisons that deviated significantly from null models tended to be spread randomly along the cline and were represented equally by positive and negative differences. These results suggest that asymmetrical migration, although detectable, was not a common feature of the cline. They also suggest that asymmetrical migration was not localized or predominately in one direction.
|
To test the robustness of our results, we applied the MIGRATE 1.6.9 program (![]()
| CONCLUSIONS |
|---|
As with previous studies, our survey of genetic variation in D. melanogaster revealed low, but statistically significant, differentiation among most populations. However, we found no evidence to support AGIS and SCHLÖTTERER's (2001) view that gene flow among populations was low or that Tasmanian populations were genetically distinct from mainland populations. Instead, our results indicate that gene flow has been sufficient to maintain higher than expected genetic homogeneity between sites up to 500 km apart and has possibly caused fluctuations in underlying clinal patterns at distances >1500 km. Our data therefore support the more traditionally held view that migration between populations in D. melanogaster is extensive (![]()
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On the basis of the test we developed to detect significant departures from symmetric migration, it would seem that asymmetrical gene flow between adjacent populations is relatively uncommon on the Australian continent. While it is true that the incidence of significant departures is likely to have been greater if the tests were based on more loci, the significant departures detected so far suggest that there is no consistent pattern in direction or location of asymmetry. Our results, therefore, are inconsistent with a systematic pattern of asymmetrical gene flow along the east coast of Australia and provide no support for the idea that the deviations from linearity in the body-size cline were caused by a regular influx of migrants from populations in warmer climates. Higher amounts of gene flow among low-latitude populations are also unlikely to have caused nonlinearity in the cline because isolation by distance was equally strong in the northern and southern halves of the cline.
| ACKNOWLEDGMENTS |
|---|
We thank D. Goldstein, L. Chikhi, and an anonymous referee for helpful discussions and/or comments on an earlier version of this manuscript. This work was funded by the Natural Environment Research Council.
Manuscript received February 3, 2003; Accepted for publication June 17, 2003.
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