IODP Expedition 374 Natural gamma radiation

• Main Authors: McKay, Robert M., De Santis, Laura, Kulhanek, Denise K., Ash, Jeanine L., Beny, François, Browne, Imogen M., Cordeiro de Sousa, Isabela M., Cortese, Giuseppe, Dodd, Justin P., Esper, Oliver M., Gales, Jenny A., Harwood, David M., Ishino, Saki, Keisling, Benjamin A., Kim, Sookwan, Kim, Sunghan, Laberg, Jan S., Leckie, R. M., Müller, Juliane, Patterson, Molly O., Romans, Brian W., Romero, Oscar E., Sangiorgi, Francesca, Seki, Osamu, Shevenell, Amelia, Singh, Shiv M., Sugisaki, Saiko T., van de Flierdt, Tina, van Peer, Tim E., Xiao, Wenshen, Xiong, Zhifang
• Other Authors: International Ocean Discovery Program
• Format: Dataset
• Language: unknown
• Published: 2019
• Subjects: International Ocean Discovery Program; IODP; JOIDES Resolution; Expedition 374; Site U1521; Site U1522; Site U1523; Site U1524; Site U1525; Ross Sea; climate and ocean change; sea level; ocean chemistry; deep biosphere; West Antarctic; ice sheet; sea ice; Antarctic Bottom Water; ice-rafted debris; Antarctic water masses; Antarctic; West Antarctic Ice Sheet; Antarc*; Ice Sheet; Sea ice
• Online Access: https://zenodo.org/record/6515791; https://doi.org/10.5281/zenodo.6515791

Natural gamma radiation (NGR) data in the ~0.1 to 3.0 MeV range were measured using eight custom-designed sodium iodide (thallium) [NaI(Tl)] detectors arranged along the core measurement axis at 20 cm intervals. The NGR system uses layers of passive shielding (lead) and active shielding (plastic scintillators and coincidence electronics) to reduce the cosmic-ray signal for low-count analysis of sediment core sections and to obtain the maximum signal-to-noise ratio. Data are reported on a total counts per second basis and the raw spectral files are available as compressed files for later analysis.