Electrostatic structure of the rotational discontinuity: The elementary pulse
Creators
- 1. Physics Department, Dartmouth College, Hanover, New Hampshire 03755
Description
An analysis is presented of the rotational discontinuity in a collision-free plasma when the width of the discontinuity is comparable to the Debye length, lambda/sub D/, so that a large deviation from charge neutrality occurs. It is found that such discontinuities have positive electrostatic potentials and structures similar to those of ion-acoustic solitons. The tangential magnetic field changes direction by a small angle Δtheta across the discontinuity, where Δtheta is of the order of lambda/sub D//lambda/sub i/, lambda/sub i/ being the ion inertial length. The polarization is left handed. These elementary pulse solutions exist only in a limited range of β/sub x/e and β/sub x/i values where β/sub x/e and β/sub x/i are the ratios of electron and ion pressure to magnetic pressure, the latter based on the magnetic field component B/sub x/, normal to the layer. The possibility that rotational discontinuities with a large angle change Δtheta are composed of wave trains of elementary pulses is discussed. Applications in the solar wind, at the magnetopause, and above the auroral zones are examined briefly
Additional details
Publishing Information
- Journal Title
- Phys. Fluids
- Journal Volume
- 27
- Journal Issue
- 7
- Series
- Phys. Fluids.
- Journal Page Range
- 1640-1646
- ISSN
- 0031-9171
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 16008055
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- AURORAL ZONES; COLD PLASMA; COLLISIONLESS PLASMA; COULOMB FIELD; DEBYE LENGTH; MAGNETIZATION; MAGNETOPAUSE; NONLINEAR PROBLEMS; SOLAR WIND; STEADY-STATE CONDITIONS; USES
- Descriptors DEC
- ELECTRIC FIELDS; MAGNETIC MOMENTS; MAGNETIC PROPERTIES; PHYSICAL PROPERTIES; PLASMA; SOLAR ACTIVITY; STELLAR ACTIVITY; STELLAR WINDS