Jian Chen

Dr. Jian Chen

orcid

Research Focus & Metrics

Academic Career Length

14Years (2013-Present)

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

Representative Publications

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1 December 2018 in Marine and Petroleum Geology
Verified
Journal Article
Closed access
JCJian Chen
Jian Chen
DLDayong Liu
Dayong Liu
XHXiaolin Hou
Xiaolin Hou
YFYukun Fan
Yukun Fan
WJWanglu Jia
Wanglu Jia
ZXZhongyao Xiao
Zhongyao Xiao

1 October 2017 in Organic Geochemistry
Verified
Journal Article
Closed access
JCJian Chen
Jian Chen
PPPing'AN Peng
Ping'AN Peng

1 February 2016 in Applied Geochemistry
Verified
Journal Article
Closed access
JCJian Chen
Jian Chen
DLDayong Liu
Dayong Liu
PPPing'AN Peng
Ping'AN Peng
CNChen Ning
Chen Ning
HXHou Xiaolin
Hou Xiaolin
XZXiao Zhongyao
Xiao Zhongyao

11 April 2013 in Geofluids
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Journal Article
Open access
PDF file
JCJian Chen
Jian Chen
DLD. Liu
D. Liu
PPPingan Peng
Pingan Peng
CYC. Yu
C. Yu
BZB. Zhang
B. Zhang
ZXZ. Xiao
Z. Xiao
The most important petroleum exploration target in the Tarim Basin, northwest China, is the paleokarst reservoir. To understand the source and evolution of brine in this type of reservoir, a total of 37 formation‐water samples were collected from the Middle‐Lower Ordovician paleokarst reservoir in the Lunnan oilfield. The δD‐δ18O correlation and Cl/Br ratios reflect the mixture of two fluids: meteoric water and evaporated seawater. The different degree of mixture divided samples into two groups. Group 1 samples, from deep strata (5150–6667 m.b.s.l.) in the east of the field, with elevated δD (−53.5 to −38.0‰), δ18O values (0.66–5.99‰), and lower Cl/Br ratios (336–478 for Cl/Br, except LN634‐1 and LN631‐1) were formed by evaporation of seawater plus a small contribution from meteoric water. Group 2 samples, from shallow strata (5038–6067 m.b.s.l.), in the west of the field, have contrasting features (−59.6 to −48.5‰ for δD, −0.47 to 2.17‰ for δ18O, and 501 to 871 for Cl/Br), which reflect a mixture of evaporated seawater with a high proportion of meteoric water. Both of the fluid types exchanged oxygen isotope with minerals. The investigation into cation composition reveals that, before entering into the current reservoir, waters suffered albitization of plagioclase; moreover, meteoric water dissolved evaporites and seawater experienced dolomitization. A mixing trend showed by strontium isotopes (0.709801–0.711628) gave further evidence for the mixture of two fluid types. Based on the correlation of geological history with our data, two infiltration models of meteoric waters can be constructed. According to the chemical and isotopic compositions of the waters, an east fluid regime (Group 1) and a west fluid regime (Group 2) have thus been defined. Better understanding of the subsurface fluid movement patterns may be helpful for the local exploration.

1 April 2020 in Marine and Petroleum Geology
Verified
Journal Article
Closed access
JCJian Chen
Jian Chen
WJWanglu Jia
Wanglu Jia
ZXZhongyao Xiao
Zhongyao Xiao
PPPing'AN Peng
Ping'AN Peng

22 March 2021 in Geofluids
Verified
Journal Article
Open access
PDF file
JCJian Chen
Jian Chen
JXJie Xu
Jie Xu
SWSusu Wang
Susu Wang
ZSZhenyu Sun
Zhenyu Sun
ZLZhong Li
Zhong Li
PPPing’aN Peng
Ping’aN Peng
Organic acids are important agents in the alteration of deep reservoirs. It is difficult, however, to assess the impact of organic acid alteration on deep reservoirs because different dissolution processes may occur during diagenesis. This study simulated the dissolution of three different types of reservoir rocks by acetic acid in a closed system and compared the mineral and elemental composition, surface morphology, pore structure, and water chemistry variations of the initial and altered samples. The study demonstrated that both micrite and sucrosic dolostone are strongly dissolved, losing about 20%–30% of their initial rock sample weights. Observation under SEM showed that the limestone dissolved homogenously, whereas the dolostone showed honeycomb-like dissolution. Both carbonate samples showed the development of large voids, including holes and cavities of micrometer scale, but nanopores of various sizes were blocked. In contrast, lithic arkose was heterogeneously altered, losing a weight proportion of about 13% by dissolution of calcite cement. These micrometer-scale microfissures were developed, but those nanometer-scale pores just varied in a narrow range of sizes. The volume increase in all three reservoir types is mainly attributed to the dissolution of carbonate minerals. In deep reservoirs, in situ generated organic acids can enlarge existing cavities in carbonates and develop microfissures in sandstones. The microfissure porosity in sandstone is limited but can increase through other geological processes such as overpressure. More importantly, these acids can maintain the acidity of pore waters, inhibit the precipitation of dissolved minerals, and help to preserve reservoir porosity. Although temperature plays an insignificant role in laboratory simulations, it influences both the generation and destruction processes of organic acids in deep reservoirs on geologic time scales and, thus, warrants further attention. The results provide a basis for recognizing the typical patterns of organic acid dissolution on different reservoir rocks and further suggest the potential role of organic acids in the formation and preservation of secondary porosity in deeply buried reservoirs.