On the synchrotron radiation in curved magnetic lines

dc.contributor.authorSobolev, Ya.M.
dc.date.accessioned2015-04-03T15:03:25Z
dc.date.available2015-04-03T15:03:25Z
dc.date.issued2005
dc.description.abstractThe general formulae that describe radiation of an ultrarelativistic electron moving along spiral trajectories with a small pitch angle in curved magnetic force lines are considered. These formulae can be identical to either synchrotron radiation or curvature radiation in certain parametric regions, but there are appreciable differences between new and old mechanisms when the velocity of Larmor’s rotation is of the order of a centrifugal drift velocity. The case when the Larmor velocity is equal exactly to the velocity of centrifugal drift was not investigated earlier. There are points with zero curvature in the particle’s trajectory, in that case. The spectral angular distribution, polarization characteristics in the neighborhood of these points have been obtained.uk_UA
dc.identifier.citationOn the synchrotron radiation in curved magnetic lines / Ya.M. Sobolev // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 51-56. — Бібліогр.: 13 назв. — англ.uk_UA
dc.identifier.issn0233-7665
dc.identifier.urihttps://nasplib.isofts.kiev.ua/handle/123456789/79602
dc.language.isoenuk_UA
dc.publisherГоловна астрономічна обсерваторія НАН Україниuk_UA
dc.relation.ispartofКинематика и физика небесных тел
dc.statuspublished earlieruk_UA
dc.subjectMS1: Decameter Radioastronomyuk_UA
dc.titleOn the synchrotron radiation in curved magnetic linesuk_UA
dc.typeArticleuk_UA

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