(Table 4) Magnetic properties of titanomagnetite in MORB younger than 100 Ma, DSDP Hole 34-320B


Autoria(s): Wang, Daming; Van der Voo, Rob; Peacor, Donald R
Cobertura

LATITUDE: -9.006700 * LONGITUDE: -83.530000 * DATE/TIME START: 1974-01-21T00:00:00 * DATE/TIME END: 1974-01-21T00:00:00 * MINIMUM DEPTH, sediment/rock: 155.72 m * MAXIMUM DEPTH, sediment/rock: 165.25 m

Data(s)

20/01/2005

Formato

text/tab-separated-values, 12 data points

Identificador

https://doi.pangaea.de/10.1594/PANGAEA.711508

doi:10.1594/PANGAEA.711508

Idioma(s)

en

Publicador

PANGAEA

Relação

doi:10.1594/PANGAEA.711520

Wang, Daming; Van der Voo, Rob; Peacor, Donald R (2005): Why is the remanent magnetic intensity of Cretaceous MORB so much higher than that of mid to late Cenozoic MORB? Geosphere, 1(3), 138-146, doi:10.1130/GES00024.1

Direitos

CC-BY: Creative Commons Attribution 3.0 Unported

Access constraints: unrestricted

Palavras-Chave #34-320B; AGE; Coercivity; Deep Sea Drilling Project; DEPTH, sediment/rock; DRILL; Drilling/drill rig; DSDP; Glomar Challenger; Hysteresis, coercivity of remanence/coercivity; Hysteresis, saturation magnetization/ saturation remanence; Hysteresis, saturation remanence; Leg34; NRM, Intensity per unit mass; ODP sample designation; Sample code/label; South Pacific/BASIN; vibrating sample magnetometer (microVSM)
Tipo

Dataset