Shoji Kojima

Dr. Shoji Kojima


Research Focus & Metrics

Academic Career Length

29Years (1998-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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20 February 2014 in Journal of South American Earth Sciences
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Journal Article
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BGBenigno Godoy
Benigno Godoy
GWGerhard Wörner
Gerhard Wörner
SKShoji Kojima
Shoji Kojima
Felipe AguileraFelipe Aguilera
Felipe Aguilera
KSKlaus Simon
Klaus Simon
GHGerald Hartmann
Gerald Hartmann

22 December 2010 in Resource Geology
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Journal Article
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BRBárbara Romero
Bárbara Romero
SKShoji Kojima
Shoji Kojima
CWChilong Wong
Chilong Wong
FBFernando Barra
Fernando Barra
WVWalter Véliz
Walter Véliz
JRJoaquin Ruiz
Joaquin Ruiz

1 March 1998 in Mineralogy and Petrology
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Journal Article
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SKShoji Kojima
Shoji Kojima
THT. Hanamuro
T. Hanamuro
KHK. Hayashi
K. Hayashi
MHM. Haruna
M. Haruna
HOH. Ohmoto
H. Ohmoto

1 March 2003 in Resource Geology
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DTDania Trista
Dania Trista
SKShoji Kojima
Shoji Kojima
Formation conditions of some vein‐type copper deposits of the Tocopilla district (Deseada, San Jose, Santa Rosa) and the Gatico district (Yohanita, Toldo‐Velarde, Argentina) in the Coastal Cordillera of northern Chile were inferred from mineral paragenesis and fluid inclusion data, and were compared with those of neighboring stratiform copper deposits. The vein‐type copper deposits are hosted in Late Jurassic dioritic to quartz‐dioritic plutons intruding extensively an andesite‐dominant volcanic pile of the Jurassic La Negra Formation. Primary mineralization is characterized by chalcopyrite + magnetite + pyrite + bornite, and supergene alteration of these minerals produced anilite, covellite, atacamite and chrysocolla. The hypogene mineral assemblage indicates relatively high sulfur fugacity and weakly oxidized conditions, distinct from the stratiform copper deposits formed under low sulfur fugacity and moderately oxidized conditions. Furthermore, the fluid inclusion data of the vein‐type deposits indicate high temperature (401–560d̀C) and high salinity (39–68 wt% NaCl equiv.) ranges in contrast to the stratiform deposits, suggesting that this type of deposits formed by magma‐associated hypersaline ore fluids.

1 July 2005 in Revista geológica de Chile
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VHVerónica Herrera
Verónica Herrera
JCJosé Cembrano
José Cembrano
VOViviana Olivares
Viviana Olivares
SKShoji Kojima
Shoji Kojima
GAGloria Arancibia
Gloria Arancibia

14 November 2018 in Minerals
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EGElias González
Elias González
SKShoji Kojima
Shoji Kojima
YIYoshihiko Ichii
Yoshihiko Ichii
TTTakayuki Tanaka
Takayuki Tanaka
YFYoshikazu Fujimoto
Yoshikazu Fujimoto
TOTakeyuki Ogata
Takeyuki Ogata
Silica-bearing magnetite was recognized in the Copiapó Nordeste prospect as the first documented occurrence in Chilean iron oxide–copper–gold (IOCG) deposits. The SiO2-rich magnetite termed silician magnetite occurs in early calcic to potassic alteration zones as orderly oscillatory layers in polyhedral magnetite and as isolated discrete grains, displaying perceptible optical differences in color and reflectance compared to normal magnetite. Micro-X-ray fluorescence and electron microprobe analyses reveal that silician magnetite has a significant SiO2 content with small amounts of other “impure” components, such as Al2O3, CaO, MgO, TiO2, and MnO. The oscillatory-zoned magnetite is generally enriched in SiO2 (up to 7.5 wt %) compared to the discrete grains. The formation of silician magnetite is explained by the exchange reactions between 2Fe (III) and Si (IV) + Fe (II), with the subordinate reactions between Fe (III) and Al (III) and between 2Fe (II) and Ca (II) + Mg (II). Silician magnetite with high concentrations of SiO2 (3.8–8.9 wt %) was similarly noted in intrusion-related magmatic–hydrothermal deposits including porphyry- and skarn-type deposits. This characteristic suggests that a hydrothermal system of relatively high-temperature and hypersaline fluids could be a substantial factor in the formation of silician magnetite with high SiO2 contents.