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(Appendix) Radiolarian abundances in ODP Hole 171-1052A
This dataset has no description
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(Table 3) Occurrence of radiolaria in upper loer Eocene and lower middle Eoce...
Species abundance: C = common (>10%), F = few (1%-10%), R = rare (0.1%-1%), VR = very rare (0.01%-0.1%), + = traces (< 0.01% of the total assemblage). A dash indicates... -
(Table T3) Radiolarian biostratigraphy of ODP Site 199-1220
Sediment depth is given in mbsf. Species abundance estimates (specimens > 63 µm): P = present but no abundance estimated, A = abundant (>10%), C = common (>1%-10%), F =... -
(Table T2) Radiolarian biostratigraphy of ODP Site 199-1219
Sediment depth is given in mbsf. Species abundance estimates (specimens > 63 µm): P = present but no abundance estimated, A = abundant (>10%), C = common (>1%-10%), F =... -
(Table T1) Radiolarian biostratigraphy of ODP Site 199-1218
Sediment depth is given in mbsf. Species abundance estimates (specimens > 63 µm): P = present but no abundance estimated, A = abundant (>10%), C = common (>1%-10%), F =... -
(Table 3) Range chart for stratigraphically important radiolarian species in ...
Sediment depth is given in mbsf. Barren intervals below 850 m not shown. Species abundance estimates as follows: C = common, F = few, VF = very few, MR = moderately rare, R =... -
(Table 2) Range chart for stratigraphically important radiolarian species in ...
Sediment depth is given in mbsf. Species abundance estimates as follows: C = common, F = few, MR = moderately rare, R = rare, + = single specimen, - = searched for but not... -
(Table 4) Range chart for stratigraphically important radiolarian species in ...
Sediment depth is given in mbsf. Species abundance estimates as follows: C = common, F = few, VF = very few, MR = moderately rare, R = rare, + = single specimen, - = searched... -
(Table 2) Radiolaria species in nodule samples from the Clarion-Clipperton pr...
Radiolaria were studied in 19 manganese nodules raised from the bottom. The nodules occurred mainly on the surface of thin Quaternary sediments covering Tertiary deposits of... -
Radiolaria abundance of Hole 44-390A
Relative abundance: D = dominant, A = abundant, C = common, F = few, R = rare, T = trace, P = present (numerical values are abundance in percent) -
Radiolaria abundance of Hole 24-237
Relative abundance: D = dominant, A = abundant, C = common, F = few, R = rare, T = trace, P = present (numerical values are abundance in percent) -
Radiolaria abundance of Hole 15-149
Relative abundance: D = dominant, A = abundant, C = common, F = few, R = rare, T = trace, P = present (numerical values are abundance in percent) -
Radiolaria abundance of Hole 14-144
Relative abundance: D = dominant, A = abundant, C = common, F = few, R = rare, T = trace, P = present (numerical values are abundance in percent) -
Radiolaria abundance of Hole 14-140A
Relative abundance: D = dominant, A = abundant, C = common, F = few, R = rare, T = trace, P = present (numerical values are abundance in percent) -
Radiolaria abundance of Hole 23-220
Relative abundance: D = dominant, A = abundant, C = common, F = few, R = rare, T = trace, P = present (numerical values are abundance in percent) -
Radiolaria abundance of Hole 23-219
Relative abundance: D = dominant, A = abundant, C = common, F = few, R = rare, T = trace, P = present (numerical values are abundance in percent) -
Radiolaria abundance of Hole 31-291A
Relative abundance: D = dominant, A = abundant, C = common, F = few, R = rare, T = trace, P = present (numerical values are abundance in percent) -
Radiolaria abundance of Hole 31-291
Relative abundance: D = dominant, A = abundant, C = common, F = few, R = rare, T = trace, P = present (numerical values are abundance in percent) -
Radiolaria abundance of Hole 31-290A
Relative abundance: D = dominant, A = abundant, C = common, F = few, R = rare, T = trace, P = present (numerical values are abundance in percent) -
Radiolaria abundance of Hole 31-290
Relative abundance: D = dominant, A = abundant, C = common, F = few, R = rare, T = trace, P = present (numerical values are abundance in percent)
