scholarly journals Beam Stability Overview

2021 ◽  
Author(s):  
Carl Ekdahl
Keyword(s):  

Author(s):  
Carl Ekdahl ◽  
P. Aragon ◽  
E. Abeyta ◽  
R. Bartsch ◽  
L. Caudill ◽  
...  
Keyword(s):  


Instruments ◽  
2021 ◽  
Vol 5 (3) ◽  
pp. 29
Author(s):  
Simone Andresen

Synchrotron radiation facilities are very important in different areas of fundamental and applied science to investigate structures or processes at small scales. Magnet–girder assemblies play a key role for the performance of such accelerator machines. High structural eigenfrequencies of the magnet–girder assemblies are required to assure a sufficient particle beam stability. The objective of the present parametric study was to numerically investigate and quantify the impact of different boundary conditions and components on the magnet–girder eigenfrequencies. As case studies, two 3 m long girder designs following the specifications of the PETRA IV project at DESY (German Electron Synchrotron, Hamburg, Germany) were selected. High magnet–girder assembly eigenfrequencies were achieved by, e.g., positioning the magnets close to the upper girder surface, increasing the connection stiffness between the magnets and the girder and between the girder and the bases, and positioning the girder support points as high as possible in the shape of a large triangle. Comparing the E/ρ ratio (E: Young’s modulus, ρ: material density) of different materials was used as a first approach to evaluate different materials for application to the girder. Based on the findings, general principles are recommended to be considered in the future girder design development processes.



2016 ◽  
Vol 84 ◽  
pp. 96-100
Author(s):  
Ya.V. Getmanov ◽  
N.A. Vinokurov ◽  
O.A. Shevchenko ◽  
I.V. Davidyuk


1961 ◽  
Vol 34 (398) ◽  
pp. 129-132 ◽  
Author(s):  
D. Greene
Keyword(s):  


Author(s):  
Joseph E. Borovsky ◽  
Gian Luca Delzanno ◽  
Michael G. Henderson

Insufficiently accurate magnetic-field-line mapping between the aurora and the equatorial magnetosphere prevents us from determining the cause of many types of aurora. An important example is the longstanding question of how the magnetosphere drives low-latitude (growth-phase) auroral arcs: a large number of diverse generator mechanisms have been hypothesized but equatorial magnetospheric measurements cannot be unambiguously connected to arcs in the ionosphere, preventing the community from identifying the correct generator mechanisms. Here a mission concept is described to solve the magnetic-connection problem. From an equatorial instrumented spacecraft, a powerful energetic-electron beam is fired into the atmospheric loss cone resulting in an optical beam spot in the upper atmosphere that can be optically imaged from the ground, putting the magnetic connection of the equatorial spacecraft’s measurements into the context of the aurora. Multiple technical challenges that must be overcome for this mission concept are discussed: these include spacecraft charging, beam dynamics, beam stability, detection of the beam spot in the presence of aurora, and the safety of nearby spacecraft.





1993 ◽  
Vol 71 (11-12) ◽  
pp. 578-581
Author(s):  
D. M. Danailov ◽  
V. Miteva ◽  
U. Littmark

Auger profiles analysis is performed on thin carbon films deposited on silicon substrates (a-C:D/Si) using a 5 keV Xe+-ion beam. Stability of the interface is observed after annealing at different temperatures. The profiling is modeled by means of a Monte-Carlo dynamic computer code. A comparison is made of the mixing of the layers for profiling with different primary ions: the heavy Xe+ and the commonly-used Ar+.



1983 ◽  
Vol 30 (4) ◽  
pp. 2092-2094 ◽  
Author(s):  
P. W. Schmor ◽  
R. Baartman ◽  
J. W. Carey ◽  
D. Dohan ◽  
G. Dutto ◽  
...  
Keyword(s):  


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