Abstract
A modification of the diffusional motion of cosmic rays in a large scale turbulent field is considered. The partial dragging of particles in the arbitrarily wandering magnetic field lines may lead to the creation of a new regime of diffusion of cosmic rays in the Galaxy.
Similar content being viewed by others
References
Allan, H. R.: 1972,Astrophys. Lett. 12, 237.
Getmantsev, G. G.: 1962,Astron. Zh. 39, 607.
Gombosi, T. and Kota, J.: 1975,14th Intern. Cosmic Ray Conf., Munich. OG 9.5-19.
Heiles, C.: 1976,Ann. Rev. Astron. Astrophys. 14, 1.
Jokipii, J. R.: 1973,Astrophys. J. 183, 1029.
Jokipii, J. R. and Parker, E. N.: 1969,Astrophys. J. 155, 799.
Lingenfelter, R. E., Ramaty, R., and Fisk, L. A.: 1971Astrophys. Lett. 8, 93.
Monin, A. S. and Yaglom, A. M.: 1965,Statistical Hydromechanics, ‘Nauka’, Moscow.
Osborn, J. L.: 1975, in J. L. Osborn and A. W. Wolfendale (eds.),Origin of Cosmic Rays, Reidel, Dordrecht.
Ptuskin, V. S.: 1977,15th Intern. Cosmic Ray Conf. Plovdiv. 2, 257.
Skilling, J., McIvor, I. and Holmes, J. A.: 1974,Monthly Notices Roy. Astron. Soc.,167, 87.
Whiteoak, J. B.: 1974, in F. J. Kerr and S. C. Simonson (eds.),Galactic Radio Astronomy, IAU Symp. No. 60, p. 137.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Ptuskin, V.S. Cosmic rays in a large-scale strongly turbulent magnetic field. Astrophys Space Sci 61, 259–265 (1979). https://doi.org/10.1007/BF00640530
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00640530