D. Boltovskoy et al., RADIOLARIAN SEDIMENTARY IMPRINT IN ATLANTIC EQUATORIAL SEDIMENTS - COMPARISON WITH THE YEARLY FLUX AT 853 M, Marine micropaleontology, 23(1), 1993, pp. 1-12
Radiolarian specific compositions in a series of 20 sediment trap samp
les covering an entire year (1.3.1989 to 16.3.1990, collected at 853 m
) were compared with bottom (0-1 cm) materials from the same site (eas
tern equatorial Atlantic: 01 degrees 47.5'N, 11 degrees 07.6'W). Data
on mean sediment accumulation rates at the site of the mooring (1.59 g
/cm(2)/kyr), mean radiolarian flux at 853 m (28,446 shells/m(2)/day),
and abundance in the 0-1 cm bottom layer (48,258 shells/g) suggest tha
t approximately 95% of the radiolarians produced are lost to the fossi
l record. Sediment trap sample-to-sample correlations (based on relati
ve abundances of 40 radiolarian species present at levels greater than
or equal to 1% in at least one sample, mean value, r=0.886) did not d
iffer significantly from correlations between each water column sample
and surface sediments (mean r=0.878). Similarities between the flux a
nd the sediments were not associated with time of year and with period
s of enhanced radiolarian output. Two taxa had lower, and nine tars ha
d higher percentage contributions in the sediments than in any one sed
iment trap sample, and a few of the abundant species had averages up t
o 7 times higher in either the water column or the sediments. These di
ssimilar percentage loadings are attributed to selective dissolution,
lateral subsurface and deep advection of shells from higher-latitude a
reas, and identification biases. As opposed to species-level inventori
es, family-level databases (including shells identified to family only
) differed significantly between the water column and the sediments. S
pumellaria (especially Spongodiscidae) were more abundant in the sedim
ents (35%) than in the water column (19%), while Nassellaria showed th
e opposite trend (64% and 80%, respectively). It is suggested that eas
e of identification of spongodiscid fragments and fragility of juvenil
e nassellarians are responsible for these differences.