Surface Rheology III. Stress on a Spherical Fluid Surface

1988 ◽  
Vol 32 (5) ◽  
pp. 473-484 ◽  
Author(s):  
D. A. Edwards ◽  
D. T. Wasan
Keyword(s):  
Surface Rheology ◽  
Fluid Surface ◽  
Spherical Fluid

Surface Rheology I. The Planar Fluid Surface

1988 ◽  
Vol 32 (5) ◽  
pp. 429-445 ◽  
Author(s):  
D. A. Edwards ◽  
D. T. Wasan
Keyword(s):  
Surface Rheology ◽  
Fluid Surface

scholarly journals Capillary wave turbulence on a spherical fluid surface in low gravity

2009 ◽  
Vol 86 (1) ◽  
pp. 14002 ◽  
Author(s):  
C. Falcón ◽  
E. Falcon ◽  
U. Bortolozzo ◽  
S. Fauve
Keyword(s):  
Capillary Wave ◽  
Wave Turbulence ◽  
Low Gravity ◽  
Fluid Surface ◽  
Spherical Fluid

Surface Rheology II. The Curved Fluid Surface

1988 ◽  
Vol 32 (5) ◽  
pp. 447-472 ◽  
Author(s):  
D. A. Edwards ◽  
D. T. Wasan
Keyword(s):  
Surface Rheology ◽  
Fluid Surface

Surface rheology and morphology of beer protein and iso-humulone at air-liquid surface

2020 ◽  
Vol 108 ◽  
pp. 105897
Author(s):  
Yi Lu ◽  
Bobae Choi ◽  
Tommy Nylander ◽  
Björn Bergenståhl ◽  
Lars Nilsson
Keyword(s):  
Liquid Surface ◽  
Surface Rheology

scholarly journals Hydromagnetic dynamos in rotating spherical fluid shells in dependence on the Prandtl number, density stratification and electromagnetic boundary conditions

2014 ◽  
Vol 44 (4) ◽  
pp. 293-312 ◽  
Author(s):  
Tomáš Šoltis ◽  
Ján Šimkanin
Keyword(s):  
Magnetic Field ◽  
Electrical Conductivity ◽  
Magnetic Fields ◽  
Prandtl Number ◽  
Inner Core ◽  
Polar Regions ◽  
Number Density ◽  
Magnetic Diffusion ◽  
Spherical Fluid ◽  
The Magnetic Field

Abstract We present an investigation of dynamo in a simultaneous dependence on the non-uniform stratification, electrical conductivity of the inner core and the Prandtl number. Computations are performed using the MAG dynamo code. In all the investigated cases, the generated magnetic fields are dipolar. Our results show that the dynamos, especially magnetic field structures, are independent in our investigated cases on the electrical conductivity of the inner core. This is in agreement with results obtained in previous analyses. The influence of non-uniform stratification is for our parameters weak, which is understandable because most of the shell is unstably stratified, and the stably stratified region is only a thin layer near the CMB. The teleconvection is not observed in our study. However, the influence of the Prandtl number is strong. The generated magnetic fields do not become weak in the polar regions because the magnetic field inside the tangent cylinder is always regenerated due to the weak magnetic diffusion.

Sign in / Sign up

Export Citation Format

Share Document