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Range table from radiolarians in ODP Hole 167-1016A
This dataset has no description
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Range table from radiolarians in ODP Hole 167-1011B
This dataset has no description
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Range table from radiolarians in ODP Hole 146-892D
This dataset has no description
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Range table from radiolarians in ODP Hole 146-892A
This dataset has no description
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Range table from radiolarians in ODP Hole 146-889A
This dataset has no description
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Range table from radiolarians in ODP Hole 145-887C
This dataset has no description
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Range table from radiolarians in ODP Hole 145-886C
This dataset has no description
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Range table from radiolarians in ODP Hole 145-885A
This dataset has no description
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Range table from radiolarians in ODP Hole 145-884C
This dataset has no description
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Range table from radiolarians in ODP Hole 145-884B
This dataset has no description
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Range table from radiolarians in ODP Hole 145-883C
This dataset has no description
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Range table from radiolarians in ODP Hole 145-883B
This dataset has no description
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Range table from radiolarians in ODP Hole 145-882B
This dataset has no description
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Range table from radiolarians in ODP Hole 145-882A
This dataset has no description
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Range table from radiolarians in ODP Hole 145-881D
This dataset has no description
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Range table from radiolarians in ODP Hole 145-881C
This dataset has no description
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Radiolaria abundance of Hole 94-610
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 94-608
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 81-555
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 81-554A
Relative abundance: D = dominant, A = abundant, C = common, F = few, R = rare, T = trace, P = present (numerical values are abundance in percent)