Nonlinear drift-Alfven waves in relativistically hot multicomponent plasmas and their relevance to the fine structure of pulsar radioemissions

Citation
Oa. Pokhotelov et al., Nonlinear drift-Alfven waves in relativistically hot multicomponent plasmas and their relevance to the fine structure of pulsar radioemissions, ASTRO SP SC, 277(3), 2001, pp. 497-505
Citations number
20
Categorie Soggetti
Space Sciences
Journal title
ASTROPHYSICS AND SPACE SCIENCE
ISSN journal
0004640X → ACNP
Volume
277
Issue
3
Year of publication
2001
Pages
497 - 505
Database
ISI
SICI code
0004-640X(2001)277:3<497:NDWIRH>2.0.ZU;2-C
Abstract
A set of equations which governs the nonlinear dynamics of drift-Alfven wav es in an inhomogeneous relativistic electron-positron plasma with a small a dmixture of heavy ions is derived. It is shown that these equations admit a stationary solution in the form of a two-scale dipolar vortex. The conditi ons for the existence of such structures are discussed. It is shown that th e presence of heavy ions in a relativistic electron-positron plasma signifi cantly reinforces the spatial localization of the solitary waves which resu lts in the appearance of exponentially localized vortex structures. It is a lso shown that the small scale micropulse structure of radio pulsar radiati on (e.g., in the case of the pulsar PSR 0905+08) can be interpreted as a si gnature of the vortex structure in the outer region of the pulsar polar mag netosphere.