scholarly journals Comparison of gyrokinetic stability code calculated critical ion temperature gradients and growth rates to DIII-D measured gradients and diffusivities

2003 ◽  
Vol 10 (11) ◽  
pp. 4419-4426 ◽  
Author(s):  
D. R. Baker ◽  
G. M. Staebler ◽  
C. C. Petty ◽  
C. M. Greenfield ◽  
T. C. Luce
2002 ◽  
Vol 9 (5) ◽  
pp. 1539-1543 ◽  
Author(s):  
O. G. Onishchenko ◽  
O. A. Pokhotelov ◽  
R. Z. Sagdeev ◽  
V. P. Pavlenko ◽  
L. Stenflo ◽  
...  

Author(s):  
Isaac Perez-Raya ◽  
Satish G. Kandlikar

Effective heat transfer techniques benefit the development of nuclear and fossil fuel powered steam generators, high power electronic devices, and industrial refrigeration systems. Boiling dissipates large heat fluxes while keeping a low and a constant surface temperature. However, studies of the fluid behavior surrounding the bubble and the heat transfer near the contact-line are scare due to difficulties of flow visualization, chaotic conditions, and small length scales. The preset study shows the simulation of bubble growth over a heated surface from conception to departure. The computation of mass transfer with interfacial temperature gradients leads to proper bubble growth rates. Models to include the interface sharpness uncover the dynamic and thermal interaction between the interface and the fluid. Results indicate that the nucleation of a bubble (in water at 1 atm with 6.2 K wall superheat) has an influence region of 2Db (where Db is the departure bubble diameter). In addition, results reveal a thin thermal film near the interface that increases the heat transfer at the contact-line region. Numerical bubble growth rates compare well with experimental data on single bubble nucleation.


2012 ◽  
Vol 19 (5) ◽  
pp. 052303 ◽  
Author(s):  
Anisa Qamar ◽  
Ata-ur-Rahman ◽  
Arshad M. Mirza

2019 ◽  
Vol 85 (5) ◽  
Author(s):  
I. J. McKinney ◽  
M. J. Pueschel ◽  
B. J. Faber ◽  
C. C. Hegna ◽  
J. N. Talmadge ◽  
...  

Ion-temperature-gradient-driven (ITG) turbulence is compared for two quasi-symmetric (QS) stellarator configurations to determine the relationship between linear growth rates and nonlinear heat fluxes. We focus on the quasi-helically symmetric (QHS) stellarator HSX and the quasi-axisymmetric (QAS) stellarator NCSX. In normalized units, HSX exhibits higher growth rates than NCSX, while heat fluxes in gyro-Bohm units are lower in HSX. These results hold for simulations made with both adiabatic and kinetic electrons. The results show that HSX has a larger number of subdominant modes than NCSX and that eigenmodes are more spatially extended in HSX. We conclude that the consideration of nonlinear physics is necessary to accurately assess the heat flux due to ITG turbulence when comparing QS stellarator equilibria.


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