Brightness Suppression of Relativistic Radio Jets of Quasars: The Role of the Lower Electron Energy Cutoff

2004 ◽  
Vol 603 (1) ◽  
pp. L9-L12 ◽  
Author(s):  
Gopal-Krishna ◽  
Peter L. Biermann ◽  
Paul J. Wiita
2000 ◽  
Vol 195 ◽  
pp. 439-441
Author(s):  
D.-Y. Wang ◽  
Y. Ma

Relativistic electrons may be effectively accelerated by turbulent Alfvén waves in radio jets. The acceleration spectrum is a power law with the electron energy as high as γ ~ 106, but the spectrum index is ~ 1.2 in the condition of diffusion approximation, which is less than the observation value.


1986 ◽  
Vol 34 (8) ◽  
pp. 5177-5183 ◽  
Author(s):  
H. J. W. M. Hoekstra ◽  
W. Speier ◽  
R. Zeller ◽  
J. C. Fuggle

2019 ◽  
Vol 880 (2) ◽  
pp. 136 ◽  
Author(s):  
Natasha L. S. Jeffrey ◽  
Eduard P. Kontar ◽  
Lyndsay Fletcher

2004 ◽  
Vol 22 (6) ◽  
pp. 2073-2080 ◽  
Author(s):  
V. Génot ◽  
S. J. Schwartz

Abstract. A complete computation of the effect of the spacecraft potential on electron moments is presented. We adopt the perfect detector concept to estimate how measured density, velocity and temperature are affected by the constraints imposed by the detector, such as the finite lower energy cutoff and the spacecraft potential. We investigate the role of the potential in different plasma regimes usually crossed by satellites. It appears that the solar wind is the region where the moments are most compromised, as the particle temperature is low. To a lesser extent the moments calculated in the magnetosheath may also deviate from the real moments, displaying up to 40% overestimation for the density under typical detector operation. The analysis allows us to identify a range of spacecraft potential values which minimizes the variation in the estimation; it is found that it corresponds to the common value adopted by potential controlling experiments.


2014 ◽  
Vol 21 (9) ◽  
pp. 093508 ◽  
Author(s):  
Giuliano D'Ammando ◽  
Mario Capitelli ◽  
Fabrizio Esposito ◽  
Annarita Laricchiuta ◽  
Lucia D. Pietanza ◽  
...  

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