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Electrostatic drift vortices in a hot rotating strongly magnetized electron-positron pulsar plasma

Technical Report:

Abstract

Electrostatic drift wave in a hot rotating and strongly magnetized electron-positron pulsar plasma is considered. Using relativistic two fluid equations a pair of coupled nonlinear equations is derived. It is shown that the wave can propagate in the form of two-dimensional dipolar vortices at ultrarelativistic temperature (T much greater than mc{sup 2}) of the plasma. The latter may affect the energy transport in the hot plasma, which can lead to a new turbulent state in the pulsar magnetosphere. (author). 16 refs.
Authors:
Publication Date:
Jul 01, 1991
Product Type:
Technical Report
Report Number:
IC-91/177
Reference Number:
SCA: 700340; PA: AIX-23:013656; SN: 92000639326
Resource Relation:
Other Information: PBD: Jul 1991
Subject:
70 PLASMA PHYSICS AND FUSION TECHNOLOGY; COLLISIONLESS PLASMA; PLASMA DRIFT; PULSARS; ELECTRONS; PLASMA FLUID EQUATIONS; POSITRONS; STELLAR MAGNETOSPHERES; TURBULENCE; VORTICES; 700340; PLASMA WAVES, OSCILLATIONS, AND INSTABILITIES
OSTI ID:
10111701
Research Organizations:
International Centre for Theoretical Physics (ICTP), Trieste (Italy)
Country of Origin:
IAEA
Language:
English
Other Identifying Numbers:
Other: ON: DE92614464; TRN: XA9130281013656
Availability:
OSTI; NTIS (US Sales Only); INIS
Submitting Site:
INIS
Size:
8 p.
Announcement Date:
Jun 30, 2005

Technical Report:

Citation Formats

Mofiz, U A. Electrostatic drift vortices in a hot rotating strongly magnetized electron-positron pulsar plasma. IAEA: N. p., 1991. Web.
Mofiz, U A. Electrostatic drift vortices in a hot rotating strongly magnetized electron-positron pulsar plasma. IAEA.
Mofiz, U A. 1991. "Electrostatic drift vortices in a hot rotating strongly magnetized electron-positron pulsar plasma." IAEA.
@misc{etde_10111701,
title = {Electrostatic drift vortices in a hot rotating strongly magnetized electron-positron pulsar plasma}
author = {Mofiz, U A}
abstractNote = {Electrostatic drift wave in a hot rotating and strongly magnetized electron-positron pulsar plasma is considered. Using relativistic two fluid equations a pair of coupled nonlinear equations is derived. It is shown that the wave can propagate in the form of two-dimensional dipolar vortices at ultrarelativistic temperature (T much greater than mc{sup 2}) of the plasma. The latter may affect the energy transport in the hot plasma, which can lead to a new turbulent state in the pulsar magnetosphere. (author). 16 refs.}
place = {IAEA}
year = {1991}
month = {Jul}
}