A predictive model for relativistic electrons at geostationary orbit

2008 ◽  
Vol 35 (15) ◽  
Author(s):  
Wladislaw Lyatsky ◽  
George V. Khazanov
Author(s):  
Victor A. Pinto ◽  
Jacob Bortnik ◽  
Pablo S. Moya ◽  
Larry R. Lyons ◽  
David G. Sibeck ◽  
...  

1989 ◽  
Vol 16 (6) ◽  
pp. 559-562 ◽  
Author(s):  
D. N. Baker ◽  
J. B. Blake ◽  
L. B. Callis ◽  
R. D. Belian ◽  
T. E. Cayton

2021 ◽  
Author(s):  
Hua Zhang ◽  
Haoran Xu ◽  
GuangShuai Peng ◽  
Ye dong Qian ◽  
Chao Shen ◽  
...  

2019 ◽  
Author(s):  
Victor A. Pinto ◽  
Jacob Bortnik ◽  
Pablo Sebastian Moya ◽  
Larry R. Lyons ◽  
David Gary Sibeck ◽  
...  

Author(s):  
J. H. Butler ◽  
C. J. Humphreys

Electromagnetic radiation is emitted when fast (relativistic) electrons pass through crystal targets which are oriented in a preferential (channelling) direction with respect to the incident beam. In the classical sense, the electrons perform sinusoidal oscillations as they propagate through the crystal (as illustrated in Fig. 1 for the case of planar channelling). When viewed in the electron rest frame, this motion, a result of successive Bragg reflections, gives rise to familiar dipole emission. In the laboratory frame, the radiation is seen to be of a higher energy (because of the Doppler shift) and is also compressed into a narrower cone of emission (due to the relativistic “searchlight” effect). The energy and yield of this monochromatic light is a continuously increasing function of the incident beam energy and, for beam energies of 1 MeV and higher, it occurs in the x-ray and γ-ray regions of the spectrum. Consequently, much interest has been expressed in regard to the use of this phenomenon as the basis for fabricating a coherent, tunable radiation source.


2020 ◽  
Vol 125 (12) ◽  
Author(s):  
Jiang Yu ◽  
L. Y. Li ◽  
Jun Cui ◽  
J. B. Cao ◽  
Jing Wang ◽  
...  

1985 ◽  
Author(s):  
Norma Miller ◽  
Thomas G. Wheeler

Sign in / Sign up

Export Citation Format

Share Document