Abstract
The global distribution of biodiversity is shaped by a complex interplay of
evolutionary history and ecological processes. While biogeographic patterns are well
defined for animals and plants, the global distributions of protists remain unclear. A key
question is whether protists follow the same broad biogeographic principles as
macroscopic life. To address this, we compiled 88 marine COI metabarcoding studies
performing population‑genetic analyses across ocean basins. Our results reveal that most
protist phyla exhibit pronounced genetic structure among oceans, a pattern exceeding that
reported for Archaeplastida and Metazoa. This likely reflects recent, and potentially
human-mediated, introductions , influencing protist dispersal and contemporary
community assembly. By demonstrating that protist distributions are not historically
cosmopolitan, our study supports the existence of common eukaryotic biogeographic
patterns that transcend organismal size.
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Main Text:
Unicellular eukaryotes (protists), which represent most of the diversity of eukaryotes
from which multicellular groups evolved, have classically been viewed as fundamentally
different from multicellular plants and animals with regard to their biogeographic patterns
(1). Early theories postulated that protists have cosmopolitan distributions and virtually
unlimited dispersal capacity, giving rise to the famous concept “everything is everywhere,
but the environment selects” (2). This view, however, was based largely on limited
morphological data. The advent of large -scale molecular techniques, such as
metabarcoding, now permits better characterization of protist distributions (3).
Some recent marine metabarcoding studies have begun to reveal that protists exhibit
biogeographic patterns more similar to those of multicellular eukaryotes than previously
assumed (4–6). Nevertheless, these investigations have predominantly focused on
presence-absence matrices, beta diversity patterns, and relative abundances inferred from
read depth. A critical knowledge gap persists regarding population-level genetic diversity
and the historical biogeographic processes shaping these distributions (7). This gap
hinders our ability to determine whether the biogeographic principles observed in
multicellular animals and plants are truly universal across all eukaryotes , or if smaller
taxa follow distinct rules in marine environments. To resolve this metabarcoding offers a
promising approach (11), as the large amount of molecular and geographic data from
different organisms enables the integration of geographical and population genetic
theories within a unified biogeographic framework (8–10). However, its effectiveness
depends on meeting certain conditions: i) the use of molecular markers with intraspecific
resolution (for example , the mitochondrial cytochrome oxidase subunit I gene, COI,
which has proven invaluable in animal biogeography (12)); ii) the availability of a
comprehensive global database for such markers that includes data from both protists and
multicellular eukaryotes (13); iii) the use of standardized taxonomic units that mitigate
the inherent biases of metabarcoding (14); and iv) the integration of population genetic
Methods
and theory into metabarcoding analyses.
Construction of a database with informative OTUs to test biogeographic patterns
To investigate global eukaryotic biogeographic patterns at the population level, a critical
first step is the creation of a comprehensive metabarcoding database amenable to
population-genetic analyses. So, we here compiled data from 88 independent
metabarcoding studies into an environmental -COI (eKOI metabarcoding) database,
comprising 976,865 amplicon -sequence variants (ASVs) with no abundance filter ( Fig.
S1) [see supplementary data (15)]; and 302,809,791 reads from 4,102 samples collected
at 957 unique sites that span all oceans (Fig. 1a). We then taxonomically annotated them
at phylum level, clustering them into 51,558 operational taxonomic units (OTUs).
To ensure robust population -genetic analyses and minimize potential artifacts, we
stringently filtered the data to retain only informative OTUs, defined as those i)
containing at least four sequences from a minimum of two distinct locations , and ii)
containing at least one pair of sequences that differ by ≥ 1% (uncorrected p‑distance).
This rigorous filtering resulted in a final dataset of 5,970 informative OTUs, comprising
276,303 ASVs and 101,898,078 reads distributed across 41 phyla (Fig. 1b, 2a). Crucially,
inter-phylum comparisons of nucleotide diversity (π) and Tajima’s D revealed minimal
significant differences (0.001% and 6.9% of pairwise comparisons, respectively; Fig. S2;
Supplementary Data), confirming broadly comparable molecular-evolutionary pressures
across phyla. Consequently, this constructed eKOI metabarcoding resource provides
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standardized taxonomic units, thereby establishing a solid foundation for rigorous,
population-level investigations of marine biogeographic hypotheses.
Protists have larger geographic ranges than animals and plants
A long -standing debate in eukaryote biogeography concerns whether protists possess
larger geographic ranges than macro -organisms (1). Testing this hypothesis has been
hindered by the sheer volume of molecular and geographic species-level data required at
a global scale (16). Our eKOI database allows for a direct assessment of this question.
We analyzed the distributional patterns of all eukaryotic phyla by comparing the range
size of every informative OTU within each eukaryotic phylum, quantifying i) the mean
pairwise geographic distance among sampling sites , and ii) the maximum distance
between any two sites. The results show that while Metazoa and Archaeplastida show
mean inter-sample distances around 1,000 km, most protist phyla average over 5,000 km,
with some individual OTUs exceeding 10,000 km ( Fig. S3). This demonstrates that
protists, at the OTU level defined by COI, possess considerably larger geographic ranges
than plants and animals.
Molecular and geographic expansions in protists
To understand why protists exhibit these distinctive geographic distances patterns,
additional data, particularly molecular data, are essential, since they enable the detection
of within-OTU genetic patterns linked to geographic range (9). Therefore, we compared
genetic versus geographic distances within each informative OTU to test whether the
observed spatial patterns were non -random and consistent across different phyla. Our
analyses using both linear and nonlinear regressions revealed that most OTUs displayed
significant non -random spatial patterns. Specifically, when compared to null models,
81.5% of OTUs in the linear models and 92.6% in the nonlinear models had R² values
that were statistically significant (p < 0.05; Supplementary Data). Furthermore, linear and
nonlinear models (Fig. S4), as well as Mantel tests (Fig. S5), consistently showed positive
relationships between genetic and geographic distances across all eukaryotic phyla
examined. In other words, genetic divergence tended to increase with greater geographic
separation. The rate of genetic divergence per unit distance, quantified by the slope of the
linear regression and by the parameter “a” of the nonlinear (exponential) model, was
largely uniform across phyla. Significant differences among phyla in these rates were
rare, occurring in only 5.7% of pairwise comparisons for the linear slopes and 3.6% for
the nonlinear “a” parameters. Moreover, the geographic extent of an OTU (mean inter -
sample distance) was only very weakly co rrelated with its genetic divergence rate,
explaining merely 3.4% of the variance in slope and 4.0% in the “a” parameter. Together,
these results indicate that geographic distance alone does not strongly limit genetic
differentiation in protists, even across vast oceanic distances. We propose that the primary
explanation for this weak isolation-by-distance pattern is the recent introduction and rapid
geographic expansion of many protist species (17, 18). Such rapid expansion over short
evolutionary timescales would limit the accumulation of substantial genetic divergence,
thus maintaining high genetic homogeneity across geographically distant populations.
Nevertheless, this interpretation should be treated with caution, as multiple introductions
can sometimes reduce genetic founder effects (19), yet molecular diversity often remains
lower compared to that observed in the centers of origin.
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Metazoa exhibit higher richness of haplotypes among eukaryotes
To follow up on those rapid geographic expansions, we then inquired how and when
current species distributions were established. To achieve this, we performed explicit
population‑genetic analyses to determine how molecular diversity is structured within
each informative OTU. Our approach involved examining the genetic structure of these
OTUs across different oceanic regions, treating each region as a distinct population. This
allows for inferences regarding both contemporary and historical processes shaping
current species distributions. To ensure unbiased analysis, population -level units within
each OTU were defined irrespective of sequencing depth variations. We observed that
haplotype richness per informative OTU had only a weak correlation with sequencin g
depth (R² = 18.2%), therefore being a robust metric for inferring population -genetic
patterns in metabarcoding studies. Using the haplotypes identified within each OTU, we
constructed haplotype networks for each informative OTU, without imposing a strict ly
bifurcating tree topology (20). This network -based approach allowed us to infer intra -
OTU genealogies while avoiding the assumption of purely bifurcating relationships
inherent to traditional phylogenies, which may not accurately capture genetic structure at
the population level (21).
As a first step, we characterized haplotype diversity distributions across major phyla
using three complementary metrics: haplotype diversity (Hd) (22), branch diversity (Bd),
and a combined haplotype -branch diversity index (H bd) (23). These metrics were
calculated based on the number of ASVs (unique haplotypes), the total read abundance
per haplotype, and log -transformed read counts. B d and H bd values showed relative
consistency across metazoan phyla, with few significant inter -phylum differences ( Fig.
S6). In contrast, H d exhibited greater variation across phyla, primarily driven by
comparisons involving Metazoa, which consistently displayed near -maximal Hd values.
This indicates a significantly higher richness of unique haplotypes and, consequently,
greater intra-OTU genetic diversity within metazoan OTUs compared to those of other
eukaryotic phyla.
Genetic Structuring Among Oceanic Regions suggest recent OTU introduction
events in protist phyla
Following the characterization of within -phylum haplotype diversity, we next assessed
genetic structuring across oceanic regions. For each informative OTU, we analysed
haplotype frequency and distribution patterns across sampled oceans. We quantified
population-level differentiation using four standard metrics of population genetic
structure: total genetic diversity (H t), within -ocean genetic diversity (H s), the fixation
index (Fst) (a measure of among-ocean differentiation) (24), and the effective number of
migrants (Nm) (an indirect estimate of gene flow) (25). These metrics revealed significant
differences among phyla in their degree of genetic structuring, with 20% of inter -phyla
comparisons showing a significant difference in H t, 9.7% in H s, 21.9% in F st, and 9.3%
in Nm (Fig. S7). The most pronounced disparities were observed in comparisons involving
Metazoa and Archaeplastida versus other phyla. Specifically, Metazoa and
Archaeplastida showed higher H s values, reflecting greater average haplotypic diversity
within individual oceans. This inter -oceanic divers ity was coupled with very low F st
values in both clades (often approaching zero and never exceeding 0.5), signifying
minimal genetic differentiation among oceanic regions. So, Metazoa and Archaeplastida
haplotypes tend to be geographically restricted. In contrast, protist phyla exhibited much
stronger genetic structuring, with consistently lower Hs and high F st values (≥ 0.5). This
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pattern indicates that although lineages in those phyla occur across multiple oceans, their
populations remain genetically isolated between regions. We propose that this strong
structure in protists may reflect recent geographic expansions or introductions rather than
long-term historical isolation.
To address the limitations of H s, in capturing haplotype distribution across oceans, we
developed the Population-level Haplotype Diversity (PHd) metric, which integrates intra-
oceanic diversity and the evenness of haplotype distribution across oceans [see
supplementary materials and methods (15)]. PHd penalizes uneven distributions, and the
difference between PHd and Hs (PHd - Hs) indicates the degree to which an OTUs genetic
diversity is structured between oceans. PH d analysis revealed significant inter -phylum
differences, 20.6% of comparisons, largely mirroring H s and F st trends. Metazoa,
Archaeplastida, and Ochrophyta showed near -zero PH d values and negative PH d - Hs
differences, suggesting concentrated haplotypic diversity in limited oceanic regions (Fig
2a and b). However, some metazoan group s such as Arthropoda (PH d - Hs = 0),
Gastrotricha (-0.17), Placozoa (0.09), and Rotifera (-0.21), exhibited more even haplotype
distributions. Protist phyla generally showed slightly higher PH d values and PH d - Hs
differences close to zero, indicating moderate population genetic structuration with
traceable dominant oceans. Overall, PH d analysis supports the hypothesis of recent
geographic expansions or introductions shaping genetic patterns in these marine
eukaryotes.
Further analysis using the PH d metric to identify dominant source oceans, harboring the
majority of that OTU’s haplotypic diversity, and introduced (recipient) oceans revealed
clear differences among taxonomic groups. Metazoa, Archaeplastida, and Ochrophyta
showed minimal evidence of multi-ocean distributions (Fig. 2C, S8). In contrast, certain
metazoan and protist phyla frequently displayed one or more introduced oceans per OTU,
indicating recent inter -ocean colonization. For example, Arthropoda, Gastrotri cha,
Porifera, Rotifera, and Xenacoelomorpha, often had broader distributions, averaging
around one introduced ocean per OTU (Fig. S8). Similarly, protists frequently displayed
one or more introduced oceans per OTU, indicating a strong signature of recent inter -
ocean introduction, with low haplotypic diversity, in these phyla. However, caution is
required when characterizing species as native or introduced, as the evolutionary history
of some species remains unclear with the current data (i.e, cryptogenic species) (26). To
minimize misclassifications, we only considered OTUs with clear patterns of intra -OTU
diversity across oceans [see supplementary materials and methods (15)].
To validate the capacity of our approach to identify genuine introduction events, we
examined specific OTUs within the phylum Chordata, where introduction histories are
often well -documented (27). Our analysis successfully highlighted several OTUs
corresponding to species known for human -mediated introductions or widespread
dispersal, such as Acipenser gueldenstaedtii, Botryllus schlosseri, Salmo trutta, Siganus
rivulatus, and Styela plicata [see supplementary data (15)]. This reinforced the reliability
of our approach in identifying recent introductions from metabarcoding data.
Furthermore, the inferred geographic scope of these colonization events differed
markedly between groups. In Metazoa and Archaeplastida, most inferred source -sink
connections occurred between geographically adjacent oceans and within the same
hemisphere, suggesting predominantly regional spread (Fig. S9). In contrast, protist phyla
OTUs often showed long -distance dispersal between non -adjacent oceans and different
hemispheres, implying that recent introductions of these microorganisms frequently span
distant oceanic regions, far exceeding the regional spread seen in larger eukaryotes (28).
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Finally, by aggregating dominant and introduced ocean assignments across all phyla, we
uncovered broad biogeographic trends that align with known global patterns of species
introductions [see supplementary materials and methods (15)]. The highest numbers of
introduced informative OTUs were detected in Northern Hemisphere oceans, particularly
the Atlantic and North Pacific (Fig. 3), consistent with these regions’ historically high
rates of species introductions (27, 29, 30). In contrast, the main source regions (dominant
oceans) across taxa were the Mediterranean Sea and Indian Ocean, both noted for their
high levels of endemic diversity (31, 32). Overall, these findings underscore that recent
colonization, most likely facilitated by anthropogenic activities, have left a distinct
imprint on global marine genetic diversity, with identifiable source areas and introduction
hotspots explaining the distribution patterns we observe.
Conclusion
Our global COI analysis, leveraging informative OTUs and the innovative PHd metric
for assessing population -level genetic diversity, definitively reveals fundamental
distinctions in the contemporary biogeography of marine eukaryotes. Metazoa and
Archaeplastida generally exhibit significantly restricted ranges and weaker ocean -basin
genetic structure compared to protist phyla, underscoring divergent molecular population
dynamics across major lineages.
These patterns likely reflect the profound impact of contemporary events, notably
anthropogenic dispersal (33). While global shipping is a known vector for metazoan
introductions (34), our data robustly indicate that protists and smaller metazoans
(Arthropoda, Rotifera, Gastrotricha, Placozoa) show heightened susceptibility to long -
distance dispersal, evidenced by elevated PHd values with respect other metazoan phyla.
Moreover, the lower PH d in these smaller metazoans compared to protist s phyla likely
stems from protists rapid generation times (35), or multiple introductions (19), could
facilitate the genetic homogenization in newly colonized oceans , reducing the founder
effect. Conversely, restricted distributions and weak structure in some small and
unicellular Archaeplastida suggest lower transoceanic transport survival, potentially due
to light and resource limitations, corroborated by the differential recovery of taxa in
ballast water studies. Consistent with this explanation, studies of ballast water frequently
recover resilient photosynthetic taxa such as Bacillariophyta and dinoflagellates, which
are capable of producing resistant forms (36), whereas groups like Chlorophyta appear
underrepresented (37, 38). This suggests that ballast water may be a less effective vector
for long-distance dispersal in certain Archaeplastida lineages.
Ultimately, our global study establishes a unified framework for interpreting broad
biogeographic and population genetic patterns across diverse eukaryotic phyla. The
congruent patterns of marine geographic distribution and genetic structure within each
group, strongly suggest shared historical processes, such as recent introductions, shaping
their contemporary ranges. These findings challenge the traditional view of protists as
ubiquitously dispersed entities (1), at the population genetic level, and reveal potentially
universal principles governing biogeographic dynamics and community assembly , that
transcend organismal size and complexity, particularly in the context of the
Anthropocene.
Materials and methods
eKOI metabarcoding database
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To generate the eKOI metabarcoding database we selected 88 marine metabarcoding
studies, with publicly accessible raw sequencing data, that had been generated on an
Illumina paired-end platform using the cytochrome oxidase subunit I (COI) molecular
marker, and employed the following primers: HCO
(TAAACTTCAGGGTGACCAAAAAATCA) (39), LCO
(GGTCAACAAATCATAAAGATATTGG) (39), jgHCO2198
(TAIACYTCIGGRTGICCRAARAAYCA) (40), mlCOIintF
(GGWACWGGWTGAACWGTWTAYCCYCC) (41), and mlCOIintF -XT
(GGWACWRGWTGRACWITITAYCCYCC) (42). After obtaining the raw data for
each study, we processed each dataset separately according to the protocol outlined in
(43). As a first step, primer trimming and demultiplexing were performed with Cutadapt
(version 2.8) (44), when necessary. Next, the resulting reads for each sample in each
metabarcoding study were processed independently using the DADA2 R package (45),
with minor modifications applied depending on the specific metabarcoding study.
Chimeric sequences were subsequently removed using the DADA2
removeBimeraDenovo function. After inferring the amplicon sequence variants (ASVs),
we stored them in a FASTA file using the following header format: >sequence_ID
merged_sample={ 'LOCALITY_ID1': reads, 'LOCALITY_ID2': reads, ... }. A separate
metadata file contained information associated with each locality ID (see metadata.csv
in the supplementary data). For each sample in the metadata, we then assigned the
corresponding ocean or sea. To achieve this, we downloaded shapefile datasets from the
“Global Oceans and Seas” database (version 1, accessed 05/11/2024) and “Natural Earth”
(accessed 05/11/2024). Using each locality’s latitude and longitude coordinates, we
determined and recorded the respective ocean or sea for that sample. For subsequent
biogeographic analyses, we utilised the broad ocean regions defined in the “Global
Oceans and Seas” database, which groups the world into 11 major seas and oceans. This
approach was chosen to avoid excessive subdivision of oceanic regions.
All FASTA files generated by each metabarcoding study, in the above format, were then
merged into a single file ( eKOI_metabarcoding_database.fasta in the supplementary
data) using a custom Python script (1_fastas_combine.py). This script utilises the
Biopython library (46) to identify identical ASVs across studies and combine their
locality information. Each unique ASV was assigned an identifier in the format eKOIX
(where X is a unique number for each ASV). Once the final merged FASTA file was
assembled, we checked it for c himeric sequences using the VSEARCH uchime_denovo
command (version 2.14.1) (47).
Taxonomic assignment of the ASVs was performed using the eKOI taxonomy database
(13). For this purpose, we used the script (5_taxonomic_assignation.py) develop in that
study. This script created a separate folder for each FASTA file in the working directory.
Within each folder, an Excel file was generated containing the taxonomic assignme nt
information for each ASV
(eKOI_metabarcoding_database_taxonomic_annotations.xlsx in the supplementary
data), obtained via the VSEARCH usearch_global command. ASVs with less than 84%
similarity to any reference sequence were not considered further. Finally, we generated
separate FASTA files for each taxonomic level of interest; in this case, we chose the
phylum level. The resulting ASV sequences for ea ch phylum can be downloaded from
the “Phyla_data” folder in the supplementary data as eKOI_database.fasta file per
phylum.
Sequence Data Processing and Analysis
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OTU Clustering
Once FASTA files were generated for each phylum, they were analysed independently.
First, all metadata for each ASV was extracted using the script
2_generate_abundances_unique.py. Biopython was used to extract each ASV’s ID and
match it with the metadata f ile, producing a DataFrame containing the sequence ID,
geographic coordinates, reads and ocean for each record (abundances_unique.csv in the
supplementary data per phylum). Because some ASVs were found in multiple localities,
duplicate entries were created for each locality where an ASV occurred by appending a
suffix “_dupN” (where N is the duplicate number) to the ASV’s ID, yielding a unique
identifier for each locality occurrence of that ASV. To avoid biases from multiple
sequencing replicates per locality (common in metabarcoding studies), only one ASV
entry per locality was retained (duplicate entries with identical ASV ID and coordi nates
were removed). After this filtering, a comprehensive FASTA file was compiled, including
all ASV sequences (with each locality -specific duplicate as a separate entry). This file
was aligned using MAFFT version 7.490 (48), with optimised parameters (--auto, --ep, -
-op, --maxiterate, --large) (aligned_sequences_mafft.fasta in the supplementary data per
phylum). Operational Taxonomic Units (OTUs) were then delineated from the alignment
using the script 3_generate_OTU.py. In particular, VSEARCH clustering at 97% identity
was employed to group sequences into OTUs. We set the clustering threshold at 97 %
identity (i.e., a 3 % divergence cut -off) because COI barcoding studies of Amoebozoa
(43), Cercozoa (49) and diverse animal taxa report similar values (12). Although each
lineage can display its own diversification rate, published barcoding gaps generally fall
between 2 % and 3 %, so we applied a uniform 3 % threshold across all phyla.
Representative ASV (centroids) for each OTU were saved, and a mapping of each ASV
to its OTU was generated as a .uc file ( otus.uc in the supplementary data per phylum).
The .uc file was subsequently processed to produce a tabular mapping file
(otus_mapping.txt in the supplementary data per phylum) that records the assignment of
each ASV ID to its corresponding OTU.
Molecular and geographic distance Matrix Construction and OTU Filtering
After obtaining the OTUs, the relationship between genetic and geographical distances
among ASVs was analysed using the R script
4_1_generate_molecular_and_geographic_distances.R. We used the Biostrings R
package to convert the phylum-level ASVs alignments into DNAbin objects, suitable for
distance calculations. Genetic distance matrices were computed under the K80 model
(Kimura 2 -parameter) (50), with gaps (insertions/deletions) excluded using the
pairwise.deletion method. In parallel, a matrix of geographical distances between
sampling localities was calculated from the coordinate data using the
distVincentyEllipsoid function of the geosphere R package. The genetic and geographical
distance matrices were both converted to long format and merged into a single data frame,
so that each row contained a pairwise genetic distance, the corresponding geographical
distance, an d the associated OTU (and phylum). To ensure robust analysis, we first
filtered the data to include only OTUs represented by at least four independent ASVs.
Next, we further filtered these OTUs, called the informative OTUs, to retain only those
in which at least one pair of sequences had a genetic distance ≥ 0.01 and at least one pair
had a geographical distance ≥ 1 m. The ratio of the number of total OTUs and filtered
informative OTUs per phylum can be downloaded from
ratio_total_OTUs_informative_OTUs_by_phylum.csv in the supplementary data, and
the ID of the informative OTUs in the file informative_OTUs.txt of each phylum. This
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two-step filtering removed OTUs with very few sequences or with negligible variation,
which could otherwise introduce noise. Metabarcoding studies that uses general primers
lack targeted taxonomic resolution and often retrieve fragmented sequences or sequences
from multiple species, potentially biasing interpretations (14). Filtering out OTUs with
uniformly low molecular divergence could mitigates these issues. While this approach
might also exclude some genuine low genetic diversity cases (for example, populations
that have undergone bottlenecks or are in decline), it pri marily reduces spurious OTUs
arising from methodological biases, improving the reliability of biogeographic patterns
interpretations.
The results of each analyses of each informative OTUs were compiled into the file
informative_OTUs_results.csv, in the supplementary data. In this file, each row
corresponds to a informative OTU and each column the results of the analysis or metrics,
such as: Phylum (the taxonomic phylum of that OTU), OTU (the OTU identifier, unique
within each phylum), Max_Distance (the maximum geographical distance, in metres,
between any two localities), Mean_Distance (the mean geographical distance among all
locality pairs), Std_Dev_Distance (standard deviation of geographical distances among
localities) and Count (number of pairwise ASV comparisons, genetic/geographical
distance pairs).
Within-OTU Diversity and Tajima’s D
To quantify genetic diversity within each informative OTU, we calculated the nucleotide
diversity (π). This was done using the previously generated alignments per phylum: the
nuc.div function (51) was applied with pairwise.deletion = TRUE to compute π for each
OTU using the script 9_calculate_nucleotide_diversity_by_otu.R. The resulting values
were recorded in the Nucleotide_Diversity_Pi column of
informative_OTUs_results.csv. We also calculated Tajima’s D for each informative
OTU to investigate potential signals of selection or demographic history (e.g. recent
expansion, bottleneck) using the script 10_calculate_tajimasD_by_otu.R. The tajima.test
function (51) was applied to the alignment data for each informative OTU. In theory, a
negative Tajima’s D indicates an excess of rare variants consistent with recent population
expansion or purifying selection, whereas a positive Tajima’s D suggests a deficiency of
rare variants, which may indicate a population bottleneck or balancing selection (52).
Given our filtering criteria (which ensured multiple sequences per OTU and some level
of genetic divergence), we expected Tajima’s D values to trend negative. Each OTU’s
Tajima’s D value was recorded in a Tajima_s_D column, with its associated p -values
recorded in P_Value_Normal (normal approximation) and P_Value_Beta (beta
distribution approximation) columns. Subsequently, we examined whether nucleotide
diversity and Tajima’s D varied significantly among phyla. (For Tajima’s D, this
comparison was restricted to OTUs with a Beta p -value < 0.05) We first checked the
distribution of each variable: the Shapiro -Wilk test indicated that the data were not
normally distributed. Therefore, a non -parametric Kruskal -Wallis test (using the
kruskal.test function in R) was employed to test for differences among phyla. A
significant Kruskal-Wallis p-value was taken as evidence of variation among phyla for
the given metric. In cases of significance, post-hoc pairwise comparisons were performed
using Dunn’s test (dunnTest function in R) with a Bonferroni adjustment for multiple
testing (53). The results of the pairwise comparisons for each variable were saved to
significant_group_comparisons_Dunn_test.csv (available in the Supplementary Data).
The file contains the columns Z (Z-Statistic), P_unadj (Uncorrected p-value) and P_adj
(Adjusted p-value) for every variable in the phyla pairwise comparison. Phyla with an
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insufficient number of informative OTUs were excluded from these comparative analyses
(Filasterea, Hemichordata, Nibbleridia, Prasinodermophyta and Ustilaginomycotina).
Additionally, for infer differences between and within groups, phyla were grouped into
three broad categories (Archaeplastida, Metazoa, and all other phyla) to compare the
prevalence of significant differences between and within these groups
(significant_group_comparations_Dunn_test.csv in the supplementary data). The
same statistical approach was applied in later analyses for other variables and metrics of
interest, as described below.
Read Count Filtering Impact
It is common in metabarcoding studies to discard ASVs with very low read counts (below
a certain threshold) to avoid spurious ASVs (54). To evaluate how such filtering might
affect the recovery of low -abundance haplotypes and OTUs, we characterised the
occurrence of rare haplotypes within each OTU. First, for each informative OTU, the total
number of ASVs and the total number of reads was recorded in the Num_Sequences and
Total_Reads columns, respectively in the informative_OTUs_results.csv file. In
addition, separate columns captured the number of reads contributed by each ocean
named _reads. We then evaluate the potential loss of data and in reads counts
filtering by counting the number of haplotypes with fewer than 10 reads for each
informative OTU, recorded in the haplotypes_lt10 column. We also determined how
many of these rare haplotypes were supported by at least two independent ASVs (each
with <10 reads); this number was recorded in haplotypes_recovered_multiple column.
By requiring multiple independent ASVs, we can identify rare haplotypes that are
consistently observed, thereby reducing the likelihood of counting sequencing artifacts as
true haplotypes. We also assessed whether the low -read filter could inadver tently affect
more abundant haplotypes. For each OTU, we counted the number of haplotypes with
total reads > 10 that nevertheless contained at least one constituent ASV with <10 reads.
This count was recorded in haplotypes_gt10_with_lt10_seq column. Finally, to examine
the biogeographic distribution of low -abundance ASVs, we counted how many oceans
had a total read count < 10 for each OTU. This value (the number of distinct oceans in
which the OTU is represented by fewer than 10 reads) was re corded in the global_lt10
column. Given that metabarcoding studies are typically constrained to specific
regions/oceans, any potential “tag jumping” across oceans (a form of cross -sample
contamination) can be ruled out at this stage. Overall, these metrics allowed us to
understand the extent to which stringent read filtering might exclude genuine but low -
frequency haplotypes and the veracity of ASVs with low number of reads.
Geographic and genetic distances
Linear regression and non -linear analyses were conducted for each informative OTU to
evaluate the relationship, strength and statistical significance of the correlation between
genetic and geographic distances using the R scripts
5_calculate_linear_models_by_otu.R and 6_calculate_nls_models_by_otu.R,
respectively. The pa rameters of the linear model (lm) were calculated for each
informative OTU using the dplyr R package, and the results were saved in the file
informative_OTUs_results.csv, with the Columns: Intercept_lm (intercept), Slope_lm
(slope), R2_lm (coefficient of determination), P_value _lm (p-value of the slope),
AIC_lm (Akaike Information Criterion), and BIC_lm (Bayesian Information Criterion).
Additionally, a non -linear regression analysis (nls) was performed using the model:
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“Genetic Distance” = a * log(“Geographical Distance” + 1) + b. Parameters a and b were
estimated from predefined initial values. The output included the a_nls (slope parameter),
b_nls (vertical offset parameter), RSS_nls (residual sum of squares), R2_nls (coefficient
of determination), AIC_nls (Akaike Information Criterion), and BIC_nls (Bayesian
Information Criterion). To interpret the differences in AIC and BIC between these two
models, categories were established based on the magnitude of the differences (Δ): (1) no
evidence to prefer either model (|Δ| ≤ 2), indicating similar fit; (2) moderate evidence (2
7),
indicating strong support for one model ( models_comparison_summary.csv file in
supplementary data). Based on these results we continued with the non-linear models for
the graphical representations, as it better explained the genetic and molecular distance
correlations per phylum.
Next, the linear and non-linear models were compared with null models to assess whether
the relationship between genetic and geographic distances was consistent with a
stochastic pattern. The null models were generated by simulating random distributions of
genetic and geographic distances using the Python script
7_calculate_null_models_by_otu.py, fitting linear models with the scikit -learn library
and optimising non-linear models with SciPy’s curve_fit function. For each OTU, 1,000
simulations were performed. In each simulation, the number of data points equalled the
number of pairwise comparisons (count column in informative_OTUs_results.csv file)
for that OTU. Geographical distances were sampled uniformly between 0 and the
maximum recorded distance ( max_distance column), and genetic distances were
sampled uniformly between 0 and 0.03 (the specified OTU cutoff). From these
simulations, the mean, median and standard deviation of R^2, AIC and BIC were
calculated for comparison with the observed models. Results were saved in
informative_OTUs_results.csv file with the following columns: Mean_R2_lm_null,
Median_R2_lm_null, Std_R2_lm_null, Mean_AIC_lm_null, Median_AIC_lm_null,
Std_AIC_lm_null, Mean_BIC_lm_null, Median_BIC_lm_null, and
Std_BIC_lm_null; and for non -linear models: Mean_R2_nls_null,
Median_R2_nls_null, Std_R2_nls_null, Mean_AIC_nls_null,
Median_AIC_nls_null, Std_AIC_nls_null, Mean_BIC_nls_null,
Median_BIC_nls_null, and Std_BIC_nls_null, Mean_a_nls_null,
Median_a_nls_null, Std_a_nls_null, Mean_b_nls_null, Median_b_nls_null, and
Std_b_nls_null. P -values were calculated to determine whether the observed
relationships differed significantly from random expectations, based on the coefficient of
determination, and were saved in the columns P_R2_lm_null (linear models) and
P_R2_nls_null (non-linear models).
To further examine whether a correlation exists between genetic and geographic distances
and to assess its consistency across phyla, Mantel tests were performed using the R script
8_calculate_mantel_test_by_otu.R. For each OTU, genetic and geographic dista nce
matrices were generated, and the Mantel test was conducted using the mantel function
from the vegan package (version 2.6) (55) with 999 permutations, the results were
recovered in the columns Mantel_R and P_Value_Mantel. However, the Mantel test can
be problematic due to inherent dependencies in the data (56). In this context, the
permutations used to calculate the p -value may not adequately reflect the expected null
distribution under true independence; therefore, this results should be interpreted with
caution. After completing these analyses, only OTUs with a Mantel test p -value < 0.05
were retained, and comparisons between phyla were conducted as described above.
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Biogeography Based on Haplotype Networks
Haplotype network construction and diversity metrics
Unique haplotypes were first identified from the alignment for each informative OTU
using the haplotype function (51). The number of haplotypes per informative OTU was
then recorded in a column named num_haplotypes. Next, using the haploNet function
(51), haplotype networks based on Minimum Spanning Networks (MSNs) were
constructed for each informative OTU and used in subsequent analyses. We then calculate
the Haplotype diversity (Hd), branch diversity (Bd) and their combined metric (Hbd) (23)
using R script 11_calculate_haplotype_diversity_by_otu.R. We saved the results in
columns named Hd, Bd and HBd, respectively, in the informative_OTUs_results.csv
file. Additionally, the maximum value of the squared haplotype frequencies per OTU was
recorded in a column Efh2_Hd.
The above metrics treat each ASV equally, regardless of its abundance (i.e. they are based
only on ASV presence/absence within each haplotype). To account for the relative
abundance of each ASV (as a proxy for its prevalence in the sample), we incorporated the
associated read counts. Specifically, we used two metrics (1) the total reads count for each
ASV and (2) a logarithmic transformation, (log(reads+1)), using the R script
12_calculate_weighted_haplotype_diversity_by_otu.R. By weighting sequences
according to their total read counts and a logarithmic transformation, haplotypes with
higher abundance have a greater influence on the calculated diversity metrics. Therefore,
if a sequence-based diversity metric exceeds its read-weighted counterpart, this indicates
that rarer haplotypes disproportionately influence the haplotypic diversity (i.e. diversity
is overestimated in the unweighted case). This approach is particularly useful for
communities with high variability in abundances, as it allows patterns of d ominance or
inequality to emerge. However, it may underestimate diversity in OTUs that contain many
low-abundance haplotypes. The results of these abundance -weighted calculations were
recorded in the following columns: Hd_reads and Hd_log_reads (haplotype diversity);
Bd_reads and Bd_log_reads (branch diversity); Hbd_reads and Hbd_log_reads
(combined haplotype and branch diversity); and Efh2_reads and Efh2_log_reads
(maximum squared haplotype frequencies).
Oceanic genetic structure
After calculating haplotype diversity metrics, we evaluated genetic structuring between
and within populations (each corresponding to a different ocean). Analysis of Molecular
Variance (AMOVA) was performed for each OTU using R script
13_calculate_amova_by_otu.R. OTUs were selected for AMOVA based on the following
criteria: (i) Presence in at least two different oceans; (ii) At least two populations; and
(iii) At least two distinct haplotypes within those populations. We used the popr.amova
function to perform the AMOVA. Variance components and sums of squares were
calculated for between-population and within-population comparisons. The results were
saved in the informative_OTUs_results.csv file, in columns named
Between_samples_SumSq, Within_samples_SumSq, Total_SumSq,
Between_samples_Sigma, Within_samples_Sigma and Total_Sigma. These metrics
were then compared across phyla as described above. Because the sequence length is
relatively short (approximately 313 bp), the AMOVA results should be interpreted with
caution.
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To mitigate potential biases introduced by short sequences, we evaluated genetic
structuring among oceans using the haplotype frequencies and distributions for each
informative OTU. The haplotypic diversity metrics total diversity (Ht), within-population
diversity (Hs), genetic differentiation coefficient (Fst) and gene flow (Nm) were calculated
for each OTU using script 14_calculate_Hs_fst_nm_by_otu.R. These four metrics were
stored in columns Ht, Hs, Fst, and Nm; and comparisons between phyla were conducted
as described above.
A modified haplotype diversity metric (PH d) was created to infer the distribution of
haplotypes among populations (here defined by different oceans) using script
15_calculate_PHd_and_global_ocean_dominance_by_otu.R. This new metric
incorporates the relative distribution of haplotypes across populations. By using weighted
relative haplotype frequencies, PH d quantifies the contribution of population -level
differences to the genetic diversity of each OTU. The classical haplotype diversity
formula was adapted to account for the distribution of haplotypes across populations. In
this adaptation, the relative frequency of each haplotype is redefined as its frequency in a
given population divided by its total frequency in the OTU. The modified PHd is therefore
calculated as:
𝑃𝐻𝑑 = 1 − ∑
𝑝𝑜𝑝𝑢𝑙𝑎𝑡𝑖𝑜𝑛(𝑜𝑐𝑒𝑎𝑛𝑠)
(𝑛𝑢𝑚𝑏𝑒𝑟 𝑜𝑓 ℎ𝑎𝑝𝑙𝑜𝑡𝑦𝑝𝑒𝑠 𝑖𝑛 𝑡ℎ𝑒 𝑝𝑜𝑝𝑢𝑙𝑎𝑡𝑖𝑜𝑛
𝑇𝑜𝑡𝑎𝑙 𝑛𝑢𝑚𝑏𝑒𝑟 𝑜𝑓 ℎ𝑎𝑝𝑙𝑜𝑡𝑦𝑝𝑒𝑠 𝑖𝑛 𝑡ℎ𝑒 𝑂𝑇𝑈 ) ^2
The PHd values were saved in a column named PHd. The relative haplotype frequencies
for each ocean were stored in columns named _sqfreq. These PHd metrics were
then compared across phyla using the same procedure as for the other diversity metrics.
Furthemore we compare PHd with Hs metric to helps to identify whether the populations
of an informative OTU are genetically structured or relatively homogeneous across
oceans. If PHd exceeds Hs (a positive difference), this indicates that the populations have
distinct genetic compositions and are partially isolated from one another, reflecting
significant genetic structuring and no single population dominating the haplotype
diversity. Conversely , if PH d is less than H s (a negative difference), one or a few
populations account for most of the global haplotypic diversity in the OTU, suggesting
that these populations dominate the haplotypic diversity.
For each informative OTU, we identified the ocean with the highest haplotype relative
contribution (the maximum sqfreq value) as a proxy for the putative population of source
and vice versa for recent introduction populations. However, this analysis is considered a
preliminary proxy to guide further investigation. To distinguish likely source populations
from recent introductions, we calculated ratios of relative haplotype frequencies between
oceans using script 20_introductions_vs_dominant_oceans_byOTU.R. Specifically,
within each OTU we used the ocean with the highest relative frequency as the reference
(ratio = 1), and we computed for each other ocean the ratio of the reference frequency to
that ocean’s frequency. We then examined the distribution of thes e ratios across all
informative OTUs to detect shifts toward lower values. A notable change in the
distribution occurred at a ratio of 0.25. Consequently, for each OTU we classified any
ocean with a ratio below 0.25 as a “recently introduced ocean/populati on,” since such
oceans have very low relative haplotype frequency compared to the highest haplotypic
frequency ocean. Furthermore, to identify a clear source ocean for each informative OTU,
we applied additional filtering criteria. We selected OTUs in whic h exactly one ocean
had a ratio of 1.0 (i.e. a single ocean had the maximum relative frequency) and excluded
informative OTUs where multiple oceans shared this maximum frequency, since that
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would preclude a clear source. We also excluded informative OTUs in which any other
ocean had a ratio exceeding 0.5, to avoid ambiguity. Although these thresholds are
somewhat arbitrary, they provide a more restrictive criterion that allows a more reliable
inference of the putative source ocean for the remaining informative OTUs. We create a
pie chart graph of the proportion of dominant oceans per phylum ancestral_oceans.pdf.
Furthermore, we combine the number of OTUs dominant and introduced oceans in the
file dominant_introduced_oceans.csv.
To validate this proxy for source (dominant) and introduced ocean populations, we used
phylum Chordata taxonomically annotated informative OTUs as a positive control. We
included only those informative OTUs that had at least one ocean classified as “recent ly
introduced”. For each selected informative OTU, the first amplicon sequence variant
(ASV) was compared to entries in the NCBI database using BLAST (57). We retained
those OTUs for which the BLAST hit showed ≥ 97% sequence identity to a species in the
database, ensuring that species -level identification was feasible. Taxonomic annotation
Results
for these OTUs are recorded in file introduced_chordata_otus.csv.
For each informative OTU, we inferred connectivity between different oceans from its
haplotype network to evaluate genetic dispersal and exchange. This analysis was
performed using the script 16_generate_ocean_connectivity_by_otu.R. In each haplotype
network, nodes represent haplotypes and edges represent connections between them. We
annotated each edge with the ocean of origin for each haplotype in the pair. Only
connections linking haplotypes from different oceans were retained; intra -oceanic
connections were discarded because they do not inform inter-ocean connectivity. We then
aggregated the data to count the number of connections between each pair of oceans. For
each informative OTU, we recorded the total number of oceanic haplotypic connections
in the column Total_Connections and the number of connections per ocean in columns
named _connections. Then, we classified oceanic pairs as “nearby” if they are
geographically adjacent and “distant” if they are geographically separated using the script
17_calculate_ocean_conectivity.R, the number of connections were recovered in the
columns nearby_oceans_connections and distant_oceans_connections. OTUs in
which all haplotypes occur in the same ocean therefore have only “nearby” connectivity
and no “distant” connectivity. We also characterised intra -hemispheric and inter -
hemispheric connectivity, focusing on connections between oceans in the Northe rn and
Southern Hemispheres, recovered in the columns Inter-Hemisferica and Intra-
Hemisferica.
For each phylum, we generated network graphs illustrating connections among oceans
using the script 18_oceanic_network_by_phyla.py and 19_global_oceanic_network.py.
In these graphs, each node represents an ocean and each edge represents the total number
of connections between two oceans, weighted by relative strength. We summed all
connections across OTUs for each phylum and applied a log1p transformation (the natural
logarithm of one plus this sum) to normalise the data. We then applied the Louvain
community detection algorithm to identify clusters (communities) within each network,
colouring nodes by their community membership. The networks were constructed using
the networkx library, with edge weights reflecting connection strength the network per
phylum were recovered as network_.pdf and .jpg.
Finally, we analysed correlations among the different calculated variables for each
informative OTU. We computed correlation matrices and associated p -values using
Pearson’s correlation coefficient, generating a table listing only those correlations that
were statistically significant (p < 0.05) significant_correlations.csv file.
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Acknowledgments: we express our gratitude to A. Berlinches, E. Lara, G. Bercedo and
M. Villar-DePablo and the MCG lab group for helpful discussions. Work funded
by the European Union (ERC, MISSINGRELATIVES, 101097659 ). Views and
opinions expressed are however those of the author(s) only and do not necessarily
reflect those of the European Union or the European Research Council. Neither
the European Union nor the granting authority can be held responsible for them .
We also acknowledge support to Departament de Recerca i Universitats de la
Generalitat de Catalunya (exp. 2021 SGR 00751) and support by PIE -
202120E047- Conexiones-Life, and MICIU/AEI /10.13039/501100011033 -
FSE+ (JDC2023-050439-I).
Author contributions:
Conceptualization: RGM, IRT
Methodology: RGM
Investigation: RGM
Visualization: RGM
Funding acquisition: RGM, IRT
Project administration: RGM
Supervision: EC, IRT
Database maintenance: AGM, GT, CB
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Writing – original draft: RGM, IRT
Writing – review & editing: RGM, AGM, GT, CB, EC, IRT
Competing interests: Authors declare that they have no competing interests.
Data and materials availability: All data, code, results, including eKOI metabarcoding
database, are available via Figshare (10.6084/m9.figshare.29144645). All other
data are available in the manuscript or the supplementary materials.
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Fig. 1. eKOI metabarcoding database . ( A) Map showing the locations of samples
included in the database. The size and color of the points represent the log(total reads) for
each sample. To the left of the map, a scatter plot displays the relationship between
log(ASVs) and log(reads) for the sampled localities, colored according to log(reads). (B)
rose plots representing the proportion of taxonomic annotated ASV as log(ASV) on the
inner layer and log(reads) on the outer layer in the different eukaryotic phyla used in the
analysis.
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Fig. 2. Population structure between eukaryotic phyla. (A) Boxplots representing the
PHd values for each OTU between phyla, where values close to 0 indicate low structuring
in terms of intra-OTU haplotype diversity. Red circles with crosses represent the median
Hs values for each phyla. The number near each phyla name represents the number of
OTU recovered after filtration. The numbers at the top indicate the difference between
PHd and H s. ( B) PHd values grouped between different phyla. ( C) Number of recent
introduced oceans per OTU grouped between different phyla.
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Fig. 3. Number of recently introduced and dominant informative OTUs per ocean.
(A) Boxplots showing the number of informative OTUs considered invasive in each
ocean and (B) the number of informative OTUs per ocean identified as their
dominant/sink.
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Fig. S1. Rare haplotypes (< 10 reads). Boxplot represents the proportion of haplotypes
with less than 10 total reads. The median is indicated by black diamonds, and the box
colors correspond to different taxonomic groups. Blue circles represent the median
proportion of haplotypes with more than 10 reads but composed of at least one ASV
with less than 10 reads. Red squares represent the median proportion of oceans
composed of less than 10 reads.
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Fig. S2. Nucleotide diversity metrics. (A) Boxplot representing the values of Tajima’s
D for OTUs grouped by phyla, with p -values less than 0.05. ( B) Boxplot of nucleotide
diversity values for OTUs grouped by phyla.
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Fig. S3. Geographic distances . The boxplots represents the maximum distribution
between two localities per informative OTU. The red circles represents the median of the
mean geographic distances between all the localities for each informative OTU.
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Fig. S4. Parameter “a” of the nonlinear (exponential) model . Boxplots representing
the values of parameter “a” from the non -linear models for each informative OTU,
relating genetic and geographic distances. Orange points represent null models generated
for each phyla, with squares marking the median values.
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Fig. S5. Significant Mantel test . Boxplots representing the R values from the Mantel
test, including only informative OTUs with a p-value less than 0.05.
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Fig. S6. Haplotypic diversity metrics . (A) Boxplot representing haplotype diversity
values, (B) branch diversity, and (C) haplotype-branch diversity, all based on the number
of sequences. In all three cases, the median considering the number of sequences is
represented by diamonds, the median based on total reads is represented by squares, and
the median using log(reads) is represented by circles.
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Fig. S7. Population structure. (A) Boxplot representing the Fst values, and (B) boxplot
of Hs values per informative OTU grouped by phyla. Circles represent the median of Nm
values, and squares represent the medians for Ht values.
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Fig. S8. Characterization dominant and introduced ocean per OTU. (A) Distribution
of haplotype relative frequency ratios between oceans of all informative OTUs. ( B)
number of introduced oceans per informative OTU grouped by phyla.
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Fig. S9. Ratios of haplotype oceanic connections. Bar plot representing the composition
of the ratios for the different types of ocean connections, based on the haplotypic
networks, for each phylum. The left side of the bar plot illustrates the proportion of
connections between inter- versus intra-hemispheric oceans, while the right side shows
the proportion of connections between separated versus adjacent oceans.
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