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Oxygen dynamics and plant-sediment interactions in isoetid ...

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Paper 4Hyphal densities of <strong>isoetid</strong> <strong>sediment</strong>s arecomparable to terrestrial soils hav<strong>in</strong>g typicallengths of hyphae between 2 <strong>and</strong> 40 m per cm -3(Smith <strong>and</strong> Read 2008). Densities were low <strong>in</strong>the upper 1 cm of the <strong>isoetid</strong> <strong>sediment</strong> probablydue to disturbance by wave exposure <strong>and</strong>bioturbation <strong>and</strong> pH-changes due tophotosynthesis of microalgae (Jasper et al. 1991;Van Aarle et al. 2002). In the root zone, hyphaldensity was high <strong>and</strong> correlated positively withroot density. With lengths of hyphae relative toroots of 700 <strong>and</strong> conservative estimates ofhyphal surface area exceed<strong>in</strong>g that of rootsurface areas by 1.7- 3.2 times <strong>in</strong> low-organic<strong>sediment</strong>s the AMF-<strong>isoetid</strong> symbiosis results <strong>in</strong>a large <strong>in</strong>crease of <strong>sediment</strong> contact for nutrientretrieval. Lengths of hyphae relative to <strong>in</strong>fectedroots were also comparable to terrestrial potexperiments with Trifolium subterraneum<strong>in</strong>oculated with Glomus fasciculatum (450-900,Abbott et al. 1984) suggest<strong>in</strong>g quantitativesimilarity to well-oxygenated nutrient-poor<strong>isoetid</strong> <strong>sediment</strong>s.In contrast to AMF root colonizationpercentages, no decrease was observed <strong>in</strong>hyphal density <strong>in</strong> <strong>sediment</strong>s follow<strong>in</strong>g organicenrichment. In fact, addition of organic mattertended to <strong>in</strong>crease hyphal density (Fig 4). Thisresult could, however, be due to sta<strong>in</strong><strong>in</strong>g of bothliv<strong>in</strong>g <strong>and</strong> dead hyphae because degradation ofdead hyphae can be slow <strong>in</strong> anaerobic<strong>sediment</strong>s.Beck-Nielsen & Madsen (2001) havereported hyphal densities from aquatic<strong>sediment</strong>s <strong>in</strong>habited by Littorella at 3-20 timeslower density than <strong>in</strong> the present <strong>in</strong>vestigation.They found hyphal densities to decrease withlower redox potential of <strong>sediment</strong>s. However,different redox potentials were found bysampl<strong>in</strong>g <strong>in</strong> <strong>sediment</strong>s differ<strong>in</strong>g <strong>in</strong> <strong>plant</strong> density<strong>and</strong>, therefore, relations could alternatively arisefrom differences <strong>in</strong> root densities which werehighly correlated to hyphal density <strong>in</strong> thepresent <strong>in</strong>vestigation. S<strong>and</strong>ers et al. (1998)reported of <strong>in</strong>creased hyphal growth <strong>in</strong>terrestrial soils under elevated CO 2 levels <strong>and</strong>similarly Andersen & Andersen (2006) found<strong>in</strong>creased AMF colonization of Littorella grownsubmerged at 10 times CO 2 air saturation <strong>in</strong> thewater. Addition of organic matter <strong>and</strong> thefollow<strong>in</strong>g <strong>in</strong>crease <strong>in</strong> CO 2 could be responsiblefor the observed tendencies of higher hyphaldensities upon organic enrichments but coupled<strong>in</strong>vestigations of hyphae growth <strong>and</strong> AMFcolonization are needed to address this questionfurther.Sediment biogeochemistryAMF colonization decreased when organicadditions deprived <strong>sediment</strong>s of O 2 <strong>and</strong> Fe 2+accumulated <strong>in</strong> the pore-water. Redox potentialswere not measured, but <strong>in</strong> <strong>sediment</strong>s at normalpH levels (≈7) thermo<strong>dynamics</strong> favor theoccurrence of Fe 2+ as the primary form below 0mV, while the presence of O 2 leads to rapid Fe 2+oxidation to Fe 3+ (half-life of m<strong>in</strong>utes; Canfieldet al. 2005). With anoxic <strong>sediment</strong>s <strong>and</strong>certa<strong>in</strong>ly low redox potentials follow<strong>in</strong>g organicenrichment the results are consistent with thoseof Beck-Nielsen & Madsen (2001) show<strong>in</strong>greduced AMF colonization <strong>in</strong> roots at redoxpotentials below 250 mV. Recent experimentsby Møller & S<strong>and</strong>-Jensen (2011) showed thatanoxia occurred <strong>in</strong> oligotrophic <strong>isoetid</strong><strong>sediment</strong>s dur<strong>in</strong>g nighttime, <strong>and</strong> anoxia evendeveloped <strong>in</strong> root <strong>and</strong> leaf aerenchyma ofLobelia late at night. This result implies thatAMF can cope with anoxia for at least some81

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