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	"Rhttps://data.globalchange.gov/gcmd_keyword/1efdd374-40a1-4118-a1da-61c647017ec9" -> "L1efdd374-40a1-4118-a1da-61c647017ec9" [ label="dcterms:identifier" ];
	"Rhttps://data.globalchange.gov/gcmd_keyword/1efdd374-40a1-4118-a1da-61c647017ec9" -> "LALUMINUM-26 ANALYSIS|Datatype: xsd:string" [ label="rdfs:label" ];
	"Rhttps://data.globalchange.gov/gcmd_keyword/1efdd374-40a1-4118-a1da-61c647017ec9" -> "LALUMINUM-26, is a radioactive isotope of the chemical element aluminium, decaying by either of the modes beta-plus or electron capture, both resulting in the stable nuclide magnesium-26. The half-life of 26Al is 7.17×105years. This is far too short for the isotope to survive to the present, but a small amount of the nuclide is produced by collisions of argon atoms with cosmic ray protons.\n The analysis of AL26 is part of the process to determine exposure ages.|Datatype: xsd:string" [ label="dcterms:description" ];
	"Rhttps://data.globalchange.gov/gcmd_keyword/1efdd374-40a1-4118-a1da-61c647017ec9" -> "Rdbpedia:Index_term" [ label="http://www.w3.org/1999/02/22-rdf-syntax-ns#type" ];

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	"LALUMINUM-26 ANALYSIS|Datatype: xsd:string" [ label="ALUMINUM-26 ANALYSIS|Datatype: xsd:string", shape = record ];
	"LALUMINUM-26, is a radioactive isotope of the chemical element aluminium, decaying by either of the modes beta-plus or electron capture, both resulting in the stable nuclide magnesium-26. The half-life of 26Al is 7.17×105years. This is far too short for the isotope to survive to the present, but a small amount of the nuclide is produced by collisions of argon atoms with cosmic ray protons.\n The analysis of AL26 is part of the process to determine exposure ages.|Datatype: xsd:string" [ label="ALUMINUM-26, is a radioactive isotope of the chemical element aluminium, decaying by either of the modes beta-plus or electron capture, both resulting in the stable nuclide magnesium-26. The half-life of 26Al is 7.17×105years. This is far too short for the isotope to survive to the present, but a small amount of the nuclide is produced by collisions of argon atoms with cosmic ray protons.\n The analysis of AL26 is part of the process to determine exposure ages.|Datatype: xsd:string", shape = record ];

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