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Title: Double-hump H{sup +} velocity distribution in the polar wind

Journal Article · · Geophysical Research Letters
DOI:https://doi.org/10.1029/95GL01519· OSTI ID:123334
; ;  [1]
  1. Utah State Univ., Logan, UT (United States)

The polar wind is an ambipolar plasma outflow from the terrestrial ionosphere at high latitudes. As the ions drift upward along geomagnetic flux tubes, they move from collision-dominated to collisionless regions. A transition layer is embedded between these two regions where the ion characteristics change rapidly. A Monte Carlo simulation was used to study the steady-state flow of H{sup +} ions through a background of O{sup +} ions. The simulation domain covered the collision-dominated, transition, and collisionless regions. The model properly accounted for the divergence of magnetic field lines, the gravitational force, the electrostatic field, and H{sup +}-O{sup +} collisions. The H{sup +} velocity distribution, f(H{sup +}), was found to be very close to Maxwellian at low altitudes. As the ions drifted to higher altitudes, f(H{sup +}) formed an upward tail. In the transition layer, the upward tail evolved into a second peak with a kidney bean shape, and hence, f(H{sup +}) developed a double-humped shape. The second peak grew with altitude and eventually became dominant as the ions reached the exosphere. This behavior is due to the interplay between the electrostatic force and the velocity-dependent Coulomb collisions. Moreover, the H{sup +} heat flux, q(H{sup +}), was found to change rapidly with altitude in the transition layer form a positive maximum to a negative minimum. This remarkable feature of q(H{sup +}) is closely related to the coincident formation of the double-humped structure of f(H{sup +}). The double-hump distribution might destabilize the plasma or, at least, cause enhanced thermal fluctuations. The double-hump f(H{sup +}), and the associated wave turbulence, have several consequences with regard to our understanding of the polar wind and similar space physics problems. 13 refs., 3 figs.

OSTI ID:
123334
Journal Information:
Geophysical Research Letters, Vol. 22, Issue 14; Other Information: PBD: 15 Jul 1995
Country of Publication:
United States
Language:
English

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