_version_ 1866902017862008832
author Fryer, P.
Wheat, C.G.
Williams, T.
Albers, E.
Bekins, B.
Debret, B.P.R.
Deng, J.
Dong, Y.
Eickenbusch, P.
Frery, E.A.
Ichiyama, Y.
Johnson, K.
Johnston, R.M.
Kevorkian, R.T.
Kurz, W.
Magalhaes, V.
Mantovanelli, S.S.
Menapace, W.
Menzies, C.D.
Michibayashi, K.
Moyer, C.L.
Mullane, K.K.
Park, J.-W.
Price, R.E.
Ryan, J.G.
Shervais, J.W.
Sissmann, O.J.
Suzuki, S.
Takai, K.
Walter, B.
Zhang, R.
author_facet Fryer, P.
Wheat, C.G.
Williams, T.
Albers, E.
Bekins, B.
Debret, B.P.R.
Deng, J.
Dong, Y.
Eickenbusch, P.
Frery, E.A.
Ichiyama, Y.
Johnson, K.
Johnston, R.M.
Kevorkian, R.T.
Kurz, W.
Magalhaes, V.
Mantovanelli, S.S.
Menapace, W.
Menzies, C.D.
Michibayashi, K.
Moyer, C.L.
Mullane, K.K.
Park, J.-W.
Price, R.E.
Ryan, J.G.
Shervais, J.W.
Sissmann, O.J.
Suzuki, S.
Takai, K.
Walter, B.
Zhang, R.
contents <p>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.</p>
format Recurso digital
id zenodo_https___doi_org_10_5281_zenodo_19614318
institution Zenodo
language
publishDate 2017
publisher Zenodo
record_format zenodo
spellingShingle IODP Expedition 366 Natural gamma radiation
Fryer, P.
Wheat, C.G.
Williams, T.
Albers, E.
Bekins, B.
Debret, B.P.R.
Deng, J.
Dong, Y.
Eickenbusch, P.
Frery, E.A.
Ichiyama, Y.
Johnson, K.
Johnston, R.M.
Kevorkian, R.T.
Kurz, W.
Magalhaes, V.
Mantovanelli, S.S.
Menapace, W.
Menzies, C.D.
Michibayashi, K.
Moyer, C.L.
Mullane, K.K.
Park, J.-W.
Price, R.E.
Ryan, J.G.
Shervais, J.W.
Sissmann, O.J.
Suzuki, S.
Takai, K.
Walter, B.
Zhang, R.
Expedition 366
Mariana
Site 1200
Site U1491
Site U1492
Site U1493
Site U1494
Site U1495
Site U1496
Site U1497
Site U1498
Leg 195
Deep biosphere
subseafloor biosphere
Earth in Motion
seismic zones
JOIDES Resolution
Pacific plate
Asut Tesoru Seamount
Conical Seamount
Fantangisna Seamount
South Chamorro Seamount
Ynazao Seamount
Blue Moon Seamount
Big Blue Seamount
Celestial Seamount
subduction
seismogenic zone
mud volcano
serpentinite
CORK
forearc
harzburgite
ultramafic rock
reef limestone
guyot
<p>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.</p>
title IODP Expedition 366 Natural gamma radiation
topic Expedition 366
Mariana
Site 1200
Site U1491
Site U1492
Site U1493
Site U1494
Site U1495
Site U1496
Site U1497
Site U1498
Leg 195
Deep biosphere
subseafloor biosphere
Earth in Motion
seismic zones
JOIDES Resolution
Pacific plate
Asut Tesoru Seamount
Conical Seamount
Fantangisna Seamount
South Chamorro Seamount
Ynazao Seamount
Blue Moon Seamount
Big Blue Seamount
Celestial Seamount
subduction
seismogenic zone
mud volcano
serpentinite
CORK
forearc
harzburgite
ultramafic rock
reef limestone
guyot
url https://doi.org/10.5281/zenodo.19614318