Mode structure of turbulent electron temperature fluctuations in the Texas Experimental Tokamak Upgrade

1998 ◽  
Vol 5 (12) ◽  
pp. 4117-4120 ◽  
Author(s):  
B. H. Deng ◽  
D. L. Brower ◽  
G. Cima ◽  
C. W. Domier ◽  
N. C. Luhmann ◽  
...  
2013 ◽  
Vol 110 (4) ◽  
Author(s):  
J. C. Hillesheim ◽  
J. C. DeBoo ◽  
W. A. Peebles ◽  
T. A. Carter ◽  
G. Wang ◽  
...  

2016 ◽  
Vol 23 (4) ◽  
pp. 042303 ◽  
Author(s):  
C. Sung ◽  
A. E. White ◽  
D. R. Mikkelsen ◽  
M. Greenwald ◽  
C. Holland ◽  
...  

2002 ◽  
Vol 30 (1) ◽  
pp. 72-73 ◽  
Author(s):  
B.H. Deng ◽  
D.L. Brower ◽  
G. Cima ◽  
C.W. Domier ◽  
A.J.H. Donne ◽  
...  

1998 ◽  
Vol 5 (2) ◽  
pp. 450-454 ◽  
Author(s):  
C. Ren ◽  
J. D. Callen ◽  
T. A. Gianakon ◽  
C. C. Hegna ◽  
Z. Chang ◽  
...  

2008 ◽  
Vol 84 (4) ◽  
pp. 43002 ◽  
Author(s):  
J. Rosato ◽  
H. Capes ◽  
Y. Marandet ◽  
F. B. Rosmej ◽  
R. Stamm ◽  
...  

1997 ◽  
Vol 4 (4) ◽  
pp. 991-1001 ◽  
Author(s):  
A. Zeiler ◽  
J. F. Drake ◽  
D. Biskamp

1970 ◽  
Vol 48 (7) ◽  
pp. 918-921 ◽  
Author(s):  
Z. Zakrzewski ◽  
C. Beaudry ◽  
G. G. Cloutier

When temperature fluctuations are large in a plasma, the floating potential cannot be used to calculate electric fields. This note describes a method which allows the calculation of the plasma potential as a function of time from measured values of the electron temperature and the floating potential. An application of this technique to the evaluation of electric fields in a reflex discharge is briefly outlined.


1997 ◽  
Vol 180 ◽  
pp. 271-271
Author(s):  
D. L. Pollacco ◽  
S. A. Bell

Imaging and spectroscopy are presented for four planetary nebulae known to contain close binary central stars resulting from a recent phase of common envelope evolution. These objects are Abell 41, Abell 46, Abell 63 and Abell 65. Determinations of the nebula abundances show that He is significantly enhanced in all of the objects. These results are in agreement with theoretical expectations. Uncertainties in the nebular electron temperature constrain other abundances less well. The line fluxes indicate that N is unexpectedly under-abundant. This effect is probably not real and may be an artifact of electron temperature fluctuations within the nebulae.


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