reflection probability
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2008 ◽  
Vol 15 (2) ◽  
pp. 265-273 ◽  
Author(s):  
Y. Kuramitsu ◽  
T. Hada

Abstract. Interaction between a magnetohydrodynamic~(MHD) pulse and a charged particle is discussed both numerically and theoretically. Charged particles can be accelerated efficiently in the presence of spatially correlated MHD waves, such as short large amplitude magnetic structures, by successive mirror reflection (Fermi process). In order to understand this process, we study the reflection probability of particles by the MHD pulses, focusing on the adiabaticity on the particle motion. When the particle velocity is small (adiabatic regime), the probability that the particle is reflected by the MHD pulse is essentially determined only by the pitch angle, independent from the velocity. On the other hand, in the non-adiabatic regime, the reflection probability is inversely proportional to the square root of the normalized velocity. We discuss our numerical as well as analytical results of the interaction process with various pulse amplitude, pulse shape, and the pulse winding number. The reflection probability is universally represented as a power law function independent from above pulse properties.


Open Physics ◽  
2008 ◽  
Vol 6 (1) ◽  
Author(s):  
Vladislav Olkhovsky ◽  
Vittoria Petrillo ◽  
Jacek Jakiel ◽  
Wiesław Kantor

AbstractThe particle tunneling through a 3-D rectangular potential barrier has been studied. The simplest model for multiple internal reflections has been assumed. The explicit expression for all the transmission and reflection probability amplitudes have been derived, as well as the tunneling and reflection phase times.


2000 ◽  
Vol 77 (4) ◽  
pp. 549-551
Author(s):  
J. Appenzeller ◽  
M. Jakob ◽  
H. Stahl ◽  
J. Knoch ◽  
B. Lengeler

2000 ◽  
Vol 76 (9) ◽  
pp. 1152-1154 ◽  
Author(s):  
M. Jakob ◽  
H. Stahl ◽  
J. Knoch ◽  
J. Appenzeller ◽  
B. Lengeler ◽  
...  

1999 ◽  
Vol 78 (3) ◽  
pp. 204-231 ◽  
Author(s):  
Anton Kühberger ◽  
Michael Schulte-Mecklenbeck ◽  
Josef Perner

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