On the parametric dependences of the beam-plasma-discharge at low pressures and magnetic field strengths

1981 ◽  
Vol 8 (1) ◽  
pp. 117-120 ◽  
Author(s):  
S. Cuperman ◽  
I. Roth
1978 ◽  
Vol 5 (2) ◽  
pp. 127-130 ◽  
Author(s):  
W. Bernstein ◽  
H. Leinbach ◽  
P. Kellogg ◽  
S. Monson ◽  
T. Hallinan ◽  
...  

1982 ◽  
Vol 27 (2) ◽  
pp. 363-376
Author(s):  
I. Roth ◽  
S. Cuperman

The electrostatic instability of bounded beam –plasma systems as well as its consequences on the ignition of the beam –plasma discharge (BPD) at low pressures and magnetic field strengths are investigated. For this purpose, configurations consisting of a finite radius electron-beam –plasma system whose edge is far away from a confining coaxial metallic container are considered; an ambient, partially ionized gas filling the container is also present.


1972 ◽  
Vol 28 (12) ◽  
pp. 723-726 ◽  
Author(s):  
D. Bollinger ◽  
D. Boyd ◽  
H. Liu ◽  
M. Seidl

2000 ◽  
Vol 26 (4) ◽  
pp. 366-368
Author(s):  
A. A. Ivanov ◽  
L. N. Knyazev ◽  
A. A. Luk’yanov ◽  
S. V. Murav’ev ◽  
A. A. Serov ◽  
...  

Vacuum ◽  
2009 ◽  
Vol 83 (11) ◽  
pp. 1350-1354 ◽  
Author(s):  
E.G. Shustin ◽  
N.V. Isaev ◽  
M.P. Temiryazeva ◽  
Yu.V. Fedorov

1967 ◽  
Vol 31 ◽  
pp. 381-383
Author(s):  
J. M. Greenberg

Van de Hulst (Paper 64, Table 1) has marked optical polarization as a questionable or marginal source of information concerning magnetic field strengths. Rather than arguing about this–I should rate this method asq+-, or quarrelling about the term ‘model-sensitive results’, I wish to stress the historical point that as recently as two years ago there were still some who questioned that optical polarization was definitely due to magnetically-oriented interstellar particles.


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