z-logo
Premium
Approximate Solutions of the Equations of Motion of a Charged Particle in the Field of a Magnetic Dipole
Author(s) -
Kustaanheimo P. E.,
Tutein J.
Publication year - 1983
Publication title -
astronomische nachrichten
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.394
H-Index - 63
eISSN - 1521-3994
pISSN - 0004-6337
DOI - 10.1002/asna.2113040305
Subject(s) - physics , magnetic dipole , magnetic field , bent molecular geometry , magnetosphere particle motion , classical mechanics , dipole , differential equation , charged particle , trajectory , point particle , equations of motion , electromagnetic field , cosmic ray , quantum electrodynamics , astrophysics , quantum mechanics , ion , chemistry , organic chemistry
Three differential equations of the first order (26)—(28) which determine the trajectory are deduced. An approximate integration by means of elementary functions yields a set of formulas (in chapt. 13. Conclusions) that give a „window” in the sky inside of which the radiation point of a high energy cosmic ray (monotonely bent in the magnetic field) must lie.

This content is not available in your region!

Continue researching here.

Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom