scholarly journals Electron radiated power in cyclotron radiation emission spectroscopy experiments

2019 ◽  
Vol 99 (5) ◽  
Author(s):  
A. Ashtari Esfahani ◽  
V. Bansal ◽  
S. Böser ◽  
N. Buzinsky ◽  
R. Cervantes ◽  
...  
2020 ◽  
Vol 22 (3) ◽  
pp. 033004
Author(s):  
A Ashtari Esfahani ◽  
S Böser ◽  
N Buzinsky ◽  
R Cervantes ◽  
C Claessens ◽  
...  

2017 ◽  
Vol 44 (5) ◽  
pp. 054004 ◽  
Author(s):  
Ali Ashtari Esfahani ◽  
David M Asner ◽  
Sebastian Böser ◽  
Raphael Cervantes ◽  
Christine Claessens ◽  
...  

2017 ◽  
Vol 888 ◽  
pp. 012074
Author(s):  
A Ashtari Esfahani ◽  
S Böser ◽  
C Claessens ◽  
L de Viveiros ◽  
P J Doe ◽  
...  

Author(s):  
S. L. MConville ◽  
K. Ronald ◽  
D. C. Speirs ◽  
A. D. R. Phelps ◽  
A. W. Cross ◽  
...  

1964 ◽  
Vol 17 (1) ◽  
pp. 63 ◽  
Author(s):  
GRA Ellis

The possibility is considered that cyclotron radiation, generated by fast bunched electrons in the Earth's outer atmosphere, may be observable outside the geomagnetic field. It is shown that the intensity and other properties of such external radiation may be deduced from the known characteristics of v.1.f. hooks. It appears likely that the radiation will occur as short bursts in the frequency range from 200 to 1000 kc/s. The total radiated power may be from 1 to 1000 W, depending on the electron energy.


Author(s):  
R. F. Egerton

An important parameter governing the sensitivity and accuracy of elemental analysis by electron energy-loss spectroscopy (EELS) or by X-ray emission spectroscopy is the signal/noise ratio of the characteristic signal.


Sign in / Sign up

Export Citation Format

Share Document