magnetic arch
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2020 ◽  
Vol 86 (5) ◽  
Author(s):  
A. Chami ◽  
C. Arnas

Two-dimensional spatial measurements of magnetic field and plasma parameters have been performed in conventional magnetron DC discharges during the formation of metallic nanoparticles. Correlations between the electron density and temperature distributions, and the magnetic field geometry and strength have been established. A sharp increase of the plasma potential is found on the edge of the last magnetic arch followed by a decrease towards the anode plate and edges. It is shown that the spatial variation of the plasma potential is at the origin of a potential well that can trap negatively charged nanoparticles.



2019 ◽  
Vol 1400 ◽  
pp. 077034
Author(s):  
M E Viktorov ◽  
S V Golubev ◽  
A V Vodopyanov


2019 ◽  
Vol 61 (3) ◽  
pp. 035001 ◽  
Author(s):  
M E Viktorov ◽  
S V Golubev ◽  
A V Vodopyanov


2017 ◽  
Vol 57 (8) ◽  
pp. 1028-1037 ◽  
Author(s):  
A. S. Morgachev ◽  
Yu. T. Tsap ◽  
V. V. Smirnova ◽  
G. G. Motorina ◽  
S. A. Kuznetsov


2017 ◽  
Vol 59 (7) ◽  
pp. 075001 ◽  
Author(s):  
M E Viktorov ◽  
D A Mansfeld ◽  
A V Vodopyanov ◽  
N D Kiryuhin ◽  
S V Golubev ◽  
...  






1997 ◽  
Vol 18 (9) ◽  
pp. 865-870 ◽  
Author(s):  
Feng Quingzeng
Keyword(s):  


Solar Physics ◽  
1975 ◽  
Vol 42 (1) ◽  
pp. 179-181 ◽  
Author(s):  
R. G. Stone ◽  
Joseph Fainberg
Keyword(s):  


1971 ◽  
Vol 2 (1) ◽  
pp. 60-62 ◽  
Author(s):  
R. T. Stewart ◽  
K. V. Sheridan

In this paper we discuss 80 MHz heliograph observations of the multiple source structure and polarization of a type IV solar radio outburst on 1970 November 16. At times during the event six sources were present. Three of these were highly circularly polarized in a L.H. sense and two in a R.H. sense. The sixth source was extended and had oppositely polarized edges. From the source behaviour we conclude that the radio emission came from two expanding and one stationary magnetic arch.



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