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In 1994, the sinking of the ‘Apollo Sea’ off the West coast of South Africa led to the deposition of ca. 2 500 tons of heavy
fuel oil over 150 km of coastline. The impact of the spill on rocky shore invertebrates, rock-pool fish fauna and rock lobsters
was assessed by conducting surveys shortly after the spill, and again two months later. Where possible, results of these surveys
were compared with existing data from before the sinking of the Apollo Sea. Among the fish fauna of rock-pools, changes in
total density of fishes were largely due to changes in the abundance ofClinus superciliosus and were within the range of natural variation for the species and the community as a whole. Community structure of the rock-pool
fish fauna also remained unaffected.
At three of four impacted rocky shore sites no changes could be detected in overall benthic community structure, although
the winkleNodilittorina africana was affected. At the fourth site, a boulder beach, statistical analysis showed distinct differences in community structure
between heavily and lightly contaminated areas, as well as between all areas compared with previously existing data. There
were also significant changes in the lightly oiled areas between the first and second surveys after the spill.
Oil-fouled lobster were found at one of three sites investigated. Ca. 7 % of the seabed in this particular area was polluted.
Antennae and forelegs of almost all lobsters in the vicinity of the oil were fouled. Examination of the gut-contents confirmed
that oil inhibits the ability of lobster to feed. Although there was no evidence that mortalities of lobster were caused by
the spill, growth rates may be reduced by the decreased feeding rate. Overall, the impact of the spill was strikingly less
than might have been predicted from the effects of other oil spills.
Nomenclature: Names of fish species follow Smith & Heemstra (1986). 相似文献
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Recruitment rates of stony corals to artificial substrates were monitored for 2 years at 20 sites along the coast of Eilat, northern Red Sea, to compare with those recorded at other coral reef locations and to assess variation in recruitment at several spatial scales. Coral recruitment was low compared to that observed on the Great Barrier Reef in Australia, but was similar to levels reported from other high-latitude reef locations. Pocilloporids were the most abundant coral recruits in all seasons. Recruitment was twofold higher during the first year than during the second year of study. There was considerable spatial variability, with the largest proportion of variance, apart from the error term, attributable to differences between sites, at a scale of 102 m. Spearmans ranked correlation showed consistency in spatial patterns of recruitment of pocilloporid corals between years, but not of acroporid corals. During spring, when only the brooding pocilloporid coral Stylophora pistillata reproduces at this locality, most coral recruitment occurred at central and southern sites adjacent to well-developed coral reefs. During summer, recruitment patterns varied significantly between years, with wide variation in the recruitment of broadcasting acroporid corals at northern sites located distant from coral reefs. Settlement was low at all sites during autumn and winter. This work is the first detailed analysis of coral recruitment patterns in the Red Sea, and contributes to the understanding of the spatial and temporal scales of variation in this important reef process.Communicated by O. Kinne, Oldendorf/Luhe 相似文献
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