1987
DOI: 10.1007/bf01005556
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Determination of the characteristics of interstellar turbulence from data on the diffusion coefficient of cosmic rays

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Cited by 3 publications
(4 citation statements)
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“…The main result of this paper is the expression for nonlinear damping rate (22). Results obtained differ from results [6,7] where oblique Alfvén waves were also considered. We take into account components of random field, corresponding to magnetosonic waves.…”
contrasting
confidence: 91%
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“…The main result of this paper is the expression for nonlinear damping rate (22). Results obtained differ from results [6,7] where oblique Alfvén waves were also considered. We take into account components of random field, corresponding to magnetosonic waves.…”
contrasting
confidence: 91%
“…For the opposite relation one-dimensional results [2][3][4][5] and results [6,7] are valid. The results of this papers can be readily obtained if one let B zk = 0 in Eq.…”
Section: Basic Equationsmentioning
confidence: 85%
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