Radiolaria : flux, ecology, and taxonomy in the Pacific and Atlantic
Radiolaria : flux, ecology, and taxonomy in the Pacific and Atlantic
Date
1991
Authors
Takahashi, Kozo
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DOI
10.1575/1912/408
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Abstract
Radiolarians setting through the oceanic water column were recovered from three
stations (western tropical Atlantic, Station E; central tropical Pacific, Station P1; and
Panama Basin, Station PB) using PARFLUX sediment traps in moored arrays at several
depths. The taxonomic diversity of the radiolarian assemblages in the sediment
traps was very high. A total of 420 taxa (including 23 new taxa) were found at the
three stations; of these 208 taxa were found at Station E. The polycystine radiolarians
generally reach the sea floor with little change in abundance or species composition,
although slight skeletal dissolution occurs during their descent through the water column.
The phaeodarian radiolarians, on the other hand, are largely dissolved within the
water column; only a few species reach the sea-floor and these dissolve rapidly at the
sediment-water interface. Most radiolarian skeletons sink as individuals through deep
water columns without being incorporated into large biogenic aggregates. Because significant
numbers of nassellarian and phaeodarian species are deep-water dwelling forms,
the diversity of radiolarians increases with increasing depth in the mesopelagic zone.
The vertical flux of the total radiolarians arriving at the trap depths (in x 103 individuals/m2/day) ranged from 16-24 at Station E, 0.6-17 at Station Pl, and 29-53
at Station PB. On the average 25% and 69% of the total radiolarian flux is transported
by Spumellaria and Nassellaria, respectively, while 5% is carried by Phaeodaria. The
supply of radiolarian silica (mg Si02/m2/day) to each trap depth ranged from 2.5-4.0
at Station E, 0.9-3.2 at Station Pl, and 5.7-10.4 at Station PB. The Radiolaria appear
to be a significantly large portion of the Si02 flux in the > 63 μm size fraction and
thus play an important role in the silica cycle. When the radiolarian fluxes at the three
stations are compared with Holocene radiolarian accumulation rates in the same areas it
became apparent that several percent or less of the fluxes are preserved in the sediment
in all cases and the rest must be dissolved on the sea-floor.