Open AccessShock propagation in the outer heliosphere: 3. Pickup ions, MHD, cosmic rays, and energetic particles
Author(s) -
Rice W. K. M.,
Zank G. P.
Publication year - 2000
Publication title -
journal of geophysical research: space physics
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.67
H-Index - 298
eISSN - 2156-2202
pISSN - 0148-0227
DOI - 10.1029/1999ja000337
Subject(s) - heliosphere , physics , cosmic ray , shock wave , shock waves in astrophysics , shock (circulatory) , magnetohydrodynamics , astrophysics , interplanetary medium , interplanetary spaceflight , acceleration , diffusion , computational physics , solar wind , plasma , mechanics , nuclear physics , classical mechanics , medicine , thermodynamics
It has been shown previously that to study the propagation charcteristics of shock waves accurately in the outer helioshpere, the heliospheric model should contain pickup ions (PIs). The inclusion of a magnetic field was also shown to affect shock wave propagation but was found to be far less important than the effect of the PIs. To further this study, we consider here the effect of galactic cosmic rays and energetic particles on interplanetary traveling shock waves in the outer heliosphere. The energetic particles are taken to be protons and are assumed to be produced by injection and acceleration at the shock fronts. The galactic cosmic rays are found to have almost no effect on the shock waves. Depending on their injection efficiency and diffusion coefficient, the energetic protons, on the other hand, can significantly modify the shock structure.