Flow properties of the solar wind derived from a two-fluid model with constraints from white light and in situ interplanetary observations

1995 ◽  
Vol 22 (12) ◽  
pp. 1465-1468 ◽  
Author(s):  
Shadia Rifai Habbal ◽  
Ruth Esser ◽  
Madhulika Guhathakurta ◽  
Richard R. Fisher
Keyword(s):  
Solar Wind ◽  
White Light ◽  
Fluid Model ◽  
Flow Properties ◽  
Two Fluid Model ◽  
Two Fluid

Flow properties of the solar wind obtained from white light data, Ulysses observations and a two-fluid model

1996 ◽  
Author(s):  
Shadia Rifai Habbal ◽  
Ruth Esser ◽  
Madhulika Guhathakurta ◽  
Richard Fisher
Keyword(s):  
Solar Wind ◽  
White Light ◽  
Fluid Model ◽  
Flow Properties ◽  
Two Fluid Model ◽  
Two Fluid

A TWO-FLUID MODEL OF THE SOLAR WIND

1992 ◽  
pp. 95-98
Author(s):  
Ø. Sandbæk ◽  
E. Leer ◽  
T.E. Holzer
Keyword(s):  
Solar Wind ◽  
Fluid Model ◽  
Two Fluid Model ◽  
Two Fluid

Two-Fluid Model of the Solar Wind

1966 ◽  
Vol 16 (14) ◽  
pp. 628-631 ◽  
Author(s):  
P. A. Sturrock ◽  
R. E. Hartle
Keyword(s):  
Solar Wind ◽  
Fluid Model ◽  
Two Fluid Model ◽  
Two Fluid

Two-Fluid Model of the Solar Wind

1968 ◽  
Vol 151 ◽  
pp. 1155 ◽  
Author(s):  
R. E. Hartle ◽  
P. A. Sturrock
Keyword(s):  
Solar Wind ◽  
Fluid Model ◽  
Two Fluid Model ◽  
Two Fluid

Numerical study on the bubbly flow around a hydrofoil in pitching and heaving motions

2003 ◽  
Vol 217 (7) ◽  
pp. 811-820 ◽  
Author(s):  
T Uchiyama
Keyword(s):  
Horizontal Plane ◽  
Numerical Study ◽  
Fluid Model ◽  
Bubbly Flow ◽  
The Finite Element Method ◽  
Flow Properties ◽  
Volumetric Fraction ◽  
Propulsive Performance ◽  
Two Fluid Model ◽  
Two Fluid

The air-water bubbly flow around a hydrofoil of NACA65-010, undergoing the heaving and pitching motions in the uniform flow on a horizontal plane, is simulated by an incompressible two-fluid model. The finite element method proposed in a prior paper is applied to solve the model. The Reynolds number defined by the volumetric velocity of the water is 10000 and the volumetric fraction of the air upstream of the hydrofoil, αg0, ranges from 0 to 0.06. The simulation reveals the effects of the αg0 value, the phase difference between the heaving and pitching motions, and the oscillating frequency. The propulsive performance is also discussed in relation to the time variation of the flow properties around the hydrofoil.

An eight-moment approximation two-fluid model of the solar wind

1996 ◽  
Vol 101 (A7) ◽  
pp. 15591-15603 ◽  
Author(s):  
Espen Lyngdal Olsen ◽  
Egil Leer
Keyword(s):  
Solar Wind ◽  
Fluid Model ◽  
Moment Approximation ◽  
Two Fluid Model ◽  
Two Fluid
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