scholarly journals Method for determining electrons current extracted from plasma generator vessel used for simulation of electron beam trajectory using Simion-8 software

2018 ◽  
Author(s):  
Agus Purwadi ◽  
Suprapto ◽  
Djoko S. P. ◽  
Arum Sekar ◽  
Fuad Anwar
Keyword(s):  
Electron Beam ◽  
Plasma Generator ◽  
Beam Trajectory

37.3: A Carbon Nanotube Field Emission Display with Simple Electron Beam Trajectory Control

2007 ◽  
Vol 38 (1) ◽  
pp. 1305-1308
Author(s):  
Kenneth A. Dean ◽  
Emmett Howard ◽  
Michael R. Johnson ◽  
Bernard F. Coll ◽  
Larry Marshbanks ◽  
...  
Keyword(s):  
Electron Beam ◽  
Carbon Nanotube ◽  
Field Emission ◽  
Trajectory Control ◽  
Field Emission Display ◽  
Beam Trajectory

scholarly journals A Simulation of the Influence of the Magnetization of the Shadow Mask on the Electron Beam Trajectory.

1993 ◽  
Vol 17 (2) ◽  
pp. 545-548 ◽  
Author(s):  
H. Nasuno ◽  
A. Haga ◽  
T. Kanbayashi ◽  
K. Yamane
Keyword(s):  
Electron Beam ◽  
Shadow Mask ◽  
Beam Trajectory

scholarly journals Actively produced high-energy electron bursts within the magnetosphere: the APEX project

2002 ◽  
Vol 20 (10) ◽  
pp. 1529-1538 ◽  
Author(s):  
L. Přech ◽  
Z. Nĕmeček ◽  
J. Šafránková ◽  
A. Omar
Keyword(s):  
Electron Beam ◽  
Plasma Generator ◽  
High Energy ◽  
Energy Structure ◽  
Space Plasma Physics ◽  
Polar Orbit ◽  
Plasma Experiment ◽  
Particle Spreading ◽  
Upper Ionosphere

Abstract. The APEX project (Active Plasma Experiment) has been launched into a polar orbit in December 1991 and consists of two satellites (IK-25 and MAGION-3), with a distance between them from 200 km to 10 000 km. The mission used intensive electron beam emission, complemented by a low-energy Xenon plasma generator during the electron beam injection, for the study of dynamic processes in the magnetosphere and upper ionosphere.  The paper deals with short, intensive bursts of field-aligned electrons observed during the APEX mission on board the MAGION-3 satellite. These events are located pre-dominantly at the middle geomagnetic latitudes in the day-side magnetosphere. The time-energy structure of these electron bursts is similar to the inverted-V one, but the pitch-angle width is less than 10°. Electrons with an energy up to 700 keV are often observed during the events. We analyze the observed events, discuss the possible mechanisms of the particle spreading, and the role of the main satellite’s activity as a possible source of these events.Key words. Ionosphere (particle acceleration; particle precipitation) – Space plasma physics (active perturbation experiments)

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