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Latitudinal and temporal variability in the community structure and ...

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K. Guil<strong>in</strong>i et al. / Progress <strong>in</strong> Oceanography 110 (2013) 80–92 87Table 6Results from ma<strong>in</strong> <strong>and</strong> pairwise one-factor multivariate <strong>and</strong> univariate PERMANOVA <strong>and</strong> PERMDISP analyses test<strong>in</strong>g for differences <strong>in</strong> nematode <strong>community</strong> composition, <strong>and</strong>nematode density, relative abundance, biomass, mean <strong>in</strong>dividual biomass, <strong>and</strong> juvenile/adult ratio (J/A), respectively, over <strong>the</strong> top 5 cm of <strong>the</strong> sediment between <strong>the</strong> sPF <strong>and</strong> sPF(2nd visit) station. Significant differences are <strong>in</strong>dicated <strong>in</strong> bold.Test Factor Nematode<strong>community</strong>NematodedensityNematode relativeabundanceNematodebiomassNematode mean<strong>in</strong>dividual biomassPERMANOVA Time df 1 1 1 1 1 1MS 2169.6 1.3 10 6b 3.4 10 12 559.2 a 7.9 10 4 0.13Pseudo-F 1.49 4.58 Denom<strong>in</strong>ator is 0 9.35 0.10 7.65Sediment depth df 4 4 4 4 4 4MS 3865.3 3781300 2439.8 1159.5 0.03 0.27Pseudo-F 3.66 b 33.61 b 53.43 b 27.48 b 3.14 a 3.57 aRe(Time) df 4 10 10 4 4 2MS 1456 287860 5.3 10 13 59.8 0.008 0.28Pseudo-F 1.38 a 2.56 a Negative 1.42 0.91 4.27 aTime x Sediment depth df 4 4 4 4 4 4MS 929.8 188480 192.0 202.0 0.002 0.054Pseudo-F 0.88 1.68 4.20 a 4.79 a 0.26 0.84Residuals df 16 40 40 16 16 8MS 1055.1 112510 45.66 42.19 0.009 0.07Total df 29 59 59 29 29 29PERMDISP Sediment depth F 0.49 0.05 0.41 8.89 a 0.007 1.97df 1 1 1 1 1 1 4df 2 8 8 8 8 8 25Pairwise test 0–1 cm: sPF, sPF (2nd visit) t 1.12 0.20 2.40 a 1.551–2 cm: sPF, sPF (2nd visit) t 0.91 2.15 1.05 0.322–3 cm: sPF, sPF (2nd visit) t 1.26 2.22 2.02 0.053–4 cm: sPF, sPF (2nd visit) t 0.92 1.28 0.13 0.164–5 cm: sPF, sPF (2nd visit) t 0.90 2.10 1.37 1.37a 0.001 < p 6 0.05.b p 6 0.001).Nematode J/ADespite <strong>the</strong> broad latitud<strong>in</strong>al range covered along <strong>the</strong> ANDEEP-SYSTCO transect (49–70° S, i.e. around 2400 km), relatively littlevariation is found between <strong>the</strong> deep-sea nematode communities<strong>in</strong> terms of generic composition. Although <strong>the</strong> MDS plot (Fig. 2)gives an <strong>in</strong>dication of a subdivision <strong>in</strong>to four communities, <strong>the</strong>low percentage of exclusive genera at each station, toge<strong>the</strong>r with<strong>the</strong> dom<strong>in</strong>ance of <strong>the</strong> same four genera between all stations <strong>and</strong>meiofauna-<strong>in</strong>herent, high small-scale <strong>variability</strong> with<strong>in</strong> <strong>the</strong> stationscreates considerable overlap between most of <strong>the</strong> stations.It is more likely that identification to species level would reveala clearer separation <strong>in</strong> subcommunities, s<strong>in</strong>ce a high degree ofspecies turnover between SO stations was found before (Vermeerenet al., 2004; Fonseca et al., 2006; Ingels et al., 2006; De Meselet al., 2006). The most remarkable <strong>community</strong> composition differenceamong <strong>the</strong> ANDEEP-SYSTCO stations is however <strong>the</strong> <strong>community</strong>at <strong>the</strong> seamount Maud Rise (MR) which differs from all but<strong>the</strong> abyssal south Polar Front (sPF) station. Similarly, <strong>the</strong> compositionof several macrofaunal groups at this station showed aclearly different composition from o<strong>the</strong>r formerly sampled stations<strong>in</strong> <strong>the</strong> deep Weddell Sea (Br<strong>and</strong>t et al., 2011). Moreover,similar to <strong>the</strong> nematode assemblages, <strong>the</strong> composition of polychaetesat this seamount showed highest aff<strong>in</strong>ity to <strong>the</strong> sPF stations(Wilmsen <strong>and</strong> Schüller, 2011). The unique hydrographyregime at <strong>the</strong> seamount MR creates conditions that result <strong>in</strong> a differentfrequency, quantity <strong>and</strong> quality of fresh food compared too<strong>the</strong>r Weddell Sea areas (Abelmann <strong>and</strong> Gersonde, 1991; Wefer<strong>and</strong> Fischer, 1991). However, s<strong>in</strong>ce MR is under <strong>in</strong>fluence fromseasonal sea-ice coverage, result<strong>in</strong>g <strong>in</strong> a lower organic carbon fluxwith a different composition compared to <strong>the</strong> Polar Front region(Wefer <strong>and</strong> Fischer, 1991), <strong>the</strong> ecological conditions that determ<strong>in</strong>e<strong>the</strong> similarity between <strong>the</strong> nematode communities of <strong>the</strong>serelatively distant areas are unknown. The fauna at o<strong>the</strong>r seamounthabitats is, however, apparently often similar to neighbor<strong>in</strong>gareas that fall with<strong>in</strong> organisms’ preferred depth ranges (Clarket al., 2010).The composition of <strong>the</strong> deep-sea nematode assemblages consideredat genus level along <strong>the</strong> ANDEEP-SYSTCO transect is comparablewith deep-sea nematode communities worldwide. Threeout of four genera that dom<strong>in</strong>ate at all ANDEEP-SYSTCO stations(Acantholaimus, Halalaimus, <strong>and</strong> Desmoscolex) are known as dom<strong>in</strong>antgenera (>2% relative abundance) at deep-sea (i.e. slope to hadalzone) areas worldwide (Vanreusel et al., 2010). Our results<strong>the</strong>refore confirm that <strong>the</strong>re is no dist<strong>in</strong>ct Antarctic nematode<strong>community</strong> at genus level (Vanhove et al., 1999, 2004; Sebastianet al., 2007). In <strong>the</strong> study of Vanhove et al. (1999) nematode (generic)structural <strong>and</strong> trophic diversity decreased from <strong>the</strong> shelfbreak <strong>and</strong> upper slope (EG(100) = 40, H 1 = 3.85–3.45) towardsdown slope (EG(100) = 30, H 1 = 2.94). In comparison, <strong>the</strong> LazarevSea (LS) station at a comparable depth as <strong>the</strong> downslope station <strong>in</strong><strong>the</strong> Eastern Weddell Sea, has a higher structural <strong>and</strong> trophic diversity(EG(100) = 39, H 1 = 3.5). The rarefaction <strong>in</strong>dex for <strong>the</strong> LSslope station also agreed well with <strong>the</strong> <strong>in</strong>dex calculated for slopesworldwide (EG(100) = 40; Vanreusel et al., 2010.) Similarly to whatwas found on a worldwide scale, <strong>the</strong> rarefaction <strong>in</strong>dex reducedwhen <strong>the</strong> less diverse abyssal communities were taken <strong>in</strong>to account(EG(100) = 34.5 versus 35.5 <strong>in</strong> Vanreusel et al. (2010)). TheLS station seemed to be <strong>the</strong> area of highest polychaete diversitytoo (Wilmsen <strong>and</strong> Schüller, 2011). Two factors that are generallybelieved to <strong>in</strong>crease diversity at slopes compared to <strong>the</strong> abyss areenhanced food <strong>in</strong>put <strong>and</strong> <strong>the</strong> reduced stability of <strong>the</strong> cont<strong>in</strong>entalslope environment due to <strong>the</strong> higher eventuality of l<strong>and</strong>slides(Wilmsen <strong>and</strong> Schüller, 2011 <strong>and</strong> references <strong>the</strong>re<strong>in</strong>).Epistratum feeders (2A) sensu Wieser (1953) dom<strong>in</strong>ated at moststations (LS, MR, sPF). Vanhove et al. (1995, 1999, 2004) <strong>and</strong> Sebastianet al. (2007) observed a dom<strong>in</strong>ance of epistratum feeders <strong>in</strong>Sou<strong>the</strong>rn Ocean slope <strong>and</strong> abyssal sediments where <strong>the</strong> highest <strong>in</strong>putof organic matter was expected based on highest nematodedensities. They expla<strong>in</strong>ed this as a functional adaptation of nematodecommunities to short-term events of fresh food supply. However,no such l<strong>in</strong>k emerges when our feed<strong>in</strong>g type compositions are

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