Study on sorption and diffusion of Sr in crushed and intact basalt and granite investigated in through-diffusion experiments

2015 ◽  
Vol 304 (1) ◽  
pp. 435-441 ◽  
Author(s):  
Ming-Chee Wu ◽  
Chuan-Pin Lee ◽  
Shih-Chin Tsai ◽  
Ching-Yuan Liu ◽  
Chun-Hua Pan ◽  
...  
2016 ◽  
Vol 311 (2) ◽  
pp. 1111-1116 ◽  
Author(s):  
Yu-Hung Shih ◽  
Tsuey-Lin Tsai ◽  
Liang-Cheng Chen ◽  
Te-Yen Su ◽  
Chuan-Pin Lee ◽  
...  

2016 ◽  
Vol 311 (2) ◽  
pp. 1155-1162
Author(s):  
Chuan-Pin Lee ◽  
Shih-Chin Tsai ◽  
Ming-Chee Wu ◽  
Tsuey-Lin Tsai ◽  
Yu-Lin Tu ◽  
...  

2010 ◽  
Vol 285 (3) ◽  
pp. 733-739 ◽  
Author(s):  
Tsuey-Lin Tsai ◽  
Chuan-Pin Lee ◽  
Tzung-Yi Lin ◽  
Hwa-Jou Wei ◽  
Lee-Chung Men

2014 ◽  
Vol 1665 ◽  
pp. 171-177
Author(s):  
Kotaro Ise ◽  
Tomofumi Sato ◽  
Yoshito Sasaki ◽  
Hideki Yoshikawa

ABSTRACTWe developed a simplified biofilm sorption and diffusion experiment method. The biofilms of the Bacillus cereus were incubated on cellulose acetate membrane filters (pore size 0.2 µm, diameter 47 mm) placed on thick NB broth agar medium (thickness was about 30 mm) to support sufficient biofilm growth of the Bacillus cereus. The thickness of the formed biofilms was about 1 mm. The formed biofilms were applied to through-diffusion method, which has been used to measure diffusion coefficient of crystalline and sedimentary rocks and clay minerals. The obtained copper sorption coefficient by batch experiments was about 100 ml/g (wet weight) at the case of the concentration of cupper ion was over 0.074mmol/L. And diffusion coefficients by through diffusion experiment was De=1.1 x 10-10 (m2/s). From these results, this simplified biofilm sorption and diffusion experiment may make possible to obtain these parameters with ease.


1976 ◽  
Vol 32 ◽  
pp. 109-116 ◽  
Author(s):  
S. Vauclair

This paper gives the first results of a work in progress, in collaboration with G. Michaud and G. Vauclair. It is a first attempt to compute the effects of meridional circulation and turbulence on diffusion processes in stellar envelopes. Computations have been made for a 2 Mʘstar, which lies in the Am - δ Scuti region of the HR diagram.Let us recall that in Am stars diffusion cannot occur between the two outer convection zones, contrary to what was assumed by Watson (1970, 1971) and Smith (1971), since they are linked by overshooting (Latour, 1972; Toomre et al., 1975). But diffusion may occur at the bottom of the second convection zone. According to Vauclair et al. (1974), the second convection zone, due to He II ionization, disappears after a time equal to the helium diffusion time, and then diffusion may happen at the bottom of the first convection zone, so that the arguments by Watson and Smith are preserved.


1997 ◽  
Vol 101-103 (1-2) ◽  
pp. 479-487
Author(s):  
H v. Wensierski
Keyword(s):  

Sign in / Sign up

Export Citation Format

Share Document