Pitch-Angle Dependence of First-Order Fermi Acceleration at Shock Fronts

1966 ◽  
Vol 145 ◽  
pp. 616 ◽  
Author(s):  
J. R. Jokipii
2016 ◽  
Vol 2 ◽  
pp. 63-65 ◽  
Author(s):  
F. Fraschetti

Abstract. Recent modelling of solar energetic particles (SEPs) propagation through the heliospheric turbulence, also discussed in this workshop, has investigated the role of the pitch-angle scattering and the perpendicular transport in spreading particles in heliolongitude, as shown by multi-spacecraft measurements (STEREO A/B, ACE, SOHO, etc.) at 1 AU in various energy ranges. In some events the first-order pitch-angle anisotropy of the particles distribution is not-negligible. We calculate the average perpendicular displacement due to the gradient/curvature drift in an inhomogeneous turbulence accounting for pitch-angle dependence for two MHD turbulence models: (a) 3-D isotropic, (b) anisotropic as conjectured by Goldreich-Sridhar. We find in both cases that the drift scales as (1 − μ2)2 with the cosine of pitch-angle μ, in contrast with previous models for transport of SEPs. This result can impact the models of propagation of SEPs through the heliosphere.


2014 ◽  
Vol 119 (7) ◽  
pp. 1689-1706 ◽  
Author(s):  
Shaosui Xu ◽  
Michael W. Liemohn ◽  
David L. Mitchell ◽  
Michael D. Smith

1983 ◽  
Vol 267 ◽  
pp. 433 ◽  
Author(s):  
T. Bai ◽  
H. S. Hudson ◽  
R. M. Pelling ◽  
R. P. Lin ◽  
R. A. Schwartz ◽  
...  

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