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Northwestern Australian Margin radiolarian dataset of IODP 363 Site U1483
This dataset has no description
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Radiolarian Assemblage Counts from Northwest Pacific Surface Sediments
The Northwest Pacific Ocean is a broad ocean influenced by two major currents: the cold Oyashio Current flowing southward and the warm Kuroshio Current flowing northward. In... -
(Appendix A) Radiolarian abundances in sediment core MD96-2086
Ages are from the age model of Bertrand et al. (2002, doi:10.1016/S0025-3227(01)00216-X) based on the benthic oxygen-isotope record measured on Cibicidoides wuellerstorfi -
Radiolaria abundance of Hole 63-471
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 63-469
Relative abundance: D = dominant, A = abundant, C = common, F = few, R = rare, T = trace, P = present (numerical values are abundance in percent) -
(Table 4) Occurrences of spumellarians in Quaternary samples of ODP Site 134-...
This dataset has no description
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(Table 1) Distribution of radiolarians from ODP Hole 128-798A
Species abundance: A = abundant, C = common, F = few, R = rare, - = absent. -
(Table 17) Distribution of radiolaria in Miocene to Pleistocene sediments of ...
Species abundaces: A = abundant, C = common, F = few, R = rare, - = absent. -
(Table 4) Distribution of radiolarians in ODP Hole 126-790C
species abundance: A = abundant, C = common, F = few, R = rare, - = absent -
Counts of radiolarians at Hole C9001C
The Northwest Pacific Ocean is characterized by a strong mixing of water masses, due to the interplay of three distinct currents, i.e., the Kuroshio, the Tsugaru, and the... -
Radiolaria abundance of Hole 56-436
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 56-435
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 57-441
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 57-440B
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 57-440A
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 57-440
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 86-580
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 86-579A
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 86-579
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 86-578
Relative abundance: D = dominant, A = abundant, C = common, F = few, R = rare, T = trace, P = present (numerical values are abundance in percent)
