Aggression Replacement Therapy in Norway: Evaluation of the program and diffusion of treatment and model effects in the environment. Preliminary results

2007 ◽  
Author(s):  
Knut Gundersen
2004 ◽  
Vol 43 (3) ◽  
pp. 444-453 ◽  
Author(s):  
Stanislao Morgera ◽  
Torsten Slowinski ◽  
Christoph Melzer ◽  
Vanessa Sobottke ◽  
Ortrud Vargas-Hein ◽  
...  

2015 ◽  
Vol 30 (suppl_3) ◽  
pp. iii390-iii391
Author(s):  
Yavuz Yenicierioglu ◽  
Hakan Akdam ◽  
Belda Dursin ◽  
Alper Alp ◽  
Funda Saglam Iyiler ◽  
...  

2015 ◽  
Vol 1130 ◽  
pp. 316-320 ◽  
Author(s):  
Elaine Govender ◽  
Athanasios Kotsiopoulos ◽  
Sue T.L. Harrison

Multiple mini-column reactors, loaded with identically constructed ore samples representing grab samples of a larger heap, were used to study the behaviour of solution tracers to elucidate solution diffusion, dispersion and transport. The tracers were either introduced to the ore bed as a pulse, included during agglomeration of the ore or introduced to the system by submerging the ore bed. These methods of tracer introduction allowed for the characterisation of flow interchange in unsteady state systems. The resulting concentration-time distribution curves were analysed to allow characterisation of flow dispersion and diffusion, which facilitates exchange between the fast flowing and largely stagnant liquid phases. Preliminary results support the presence of distinct stagnant and flowing regions within the agglomerated ore bed. Agglomeration with the tracer promotes increased retention on the ore; potentially enhancing microbial transport via increased solution exchange after the initial period of attachment.


2008 ◽  
Vol 4 (S252) ◽  
pp. 253-254
Author(s):  
Laurent Piau ◽  
Robert F. Stein

AbstractThe initial surface abundances of Population II stars have been altered by the interplay between convection, rotational mixing and diffusion. In particular the shallower the outer convection zone the stronger the diffusion impact. We present preliminary results on constraining the extension of the convection zones of Population II stars thanks to 3D hydrodynamical simulations.


Sign in / Sign up

Export Citation Format

Share Document