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.
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}
}
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}
}