The mechanisms and time scale of alteration halos in vein-type tungsten deposits in southern China

2017 ◽  
Vol 89 ◽  
pp. 1019-1029 ◽  
Author(s):  
Xiangchong Liu ◽  
Huilin Xing ◽  
Dehui Zhang
Geofluids ◽  
2017 ◽  
Vol 2017 ◽  
pp. 1-11 ◽  
Author(s):  
Xiangchong Liu ◽  
Huilin Xing ◽  
Dehui Zhang

Wolframite is the main ore mineral at the vein-type tungsten deposits in the Nanling Range, which is a world-class tungsten province. It is disputed how wolframite is precipitated at these deposits and no one has yet studied the links of the mechanical processes to fluid flow and mineralization. Finite element-based numerical experiments are used to investigate the influences of a hydraulic fracturing process on fluid flow and solubility of CO2and quartz. The fluids are aqueous NaCl solutions and fluid pressure is the only variable controlling solubility of CO2and quartz in the numerical experiments. Significant fluctuations of fluid pressure and high-velocity hydrothermal pulse are found once rock is fractured by high-pressure fluids. The fluid pressure drop induced by hydraulic fracturing could cause a 9% decrease of quartz solubility. This amount of quartz deposition may not cause a significant decrease in rock permeability. The fluid pressure decrease after hydraulic fracturing also reduces solubility of CO2by 36% and increases pH. Because an increase in pH would cause a major decrease in solubility of tungsten, the fluid pressure drop accompanying a hydraulic fracturing process facilitates wolframite precipitation. Our numerical experiments provide insight into the mechanisms precipitating wolframite at the tungsten deposits in the Nanling Range as well as other metals whose solubility is strongly dependent on pH.


2017 ◽  
Vol 18 (4) ◽  
pp. 1333-1349
Author(s):  
Kunpeng Ge ◽  
Qingsong Liu ◽  
Juzhi Deng ◽  
David Nobes ◽  
Yang Wang ◽  
...  

1993 ◽  
Vol 8 (3-4) ◽  
pp. 233-246 ◽  
Author(s):  
Liu Yingjun ◽  
Ma Dongsheng
Keyword(s):  

2000 ◽  
Vol 179 ◽  
pp. 205-208
Author(s):  
Pavel Ambrož ◽  
Alfred Schroll

AbstractPrecise measurements of heliographic position of solar filaments were used for determination of the proper motion of solar filaments on the time-scale of days. The filaments have a tendency to make a shaking or waving of the external structure and to make a general movement of whole filament body, coinciding with the transport of the magnetic flux in the photosphere. The velocity scatter of individual measured points is about one order higher than the accuracy of measurements.


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