skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: The effect of wave-particle interactions on the polar wind O{sup +}

Journal Article · · Geophysical Research Letters
DOI:https://doi.org/10.1029/94GL01701· OSTI ID:166285
;  [1]
  1. Utah State Univ., Logan, UT (United States)

The escape of the polar wind plasma is an important element in the ionosphere-magnetosphere coupling. Both theory and observations indicate that the wave-particle interactions (WPI) play a significant role in the dynamics of ion outflow along open geomagnetic field lines. A Monte Carlo simulation was developed in order to include the effect of the WPI in addition to the factors that are traditionally included in the {open_quote}classical{close_quote} polar wind (i.e. gravity, electrostatic field, and divergence of geomagnetic field lines). The ion distribution function (f{sub j}), as well as the profiles of its moments (density, drift velocity, temperature, etc.) were found for different levels of WPI, that is, for different values of the normalized diffusion rate in the velocity space (D{sub {perpendicular}{sub j}}). Although the model included O{sup +}, H{sup +} and electrons, the authors presented only the results related to the O{sup +} ions. They found that (1) both the density and drift velocity of O{sup +} increased with the WPI strength, and consequently, the O{sup +} escape flux was enhanced by a factor of up to 10{sup 5}; (2) The O{sup +} ions could be energized up to a few electron volts; (3) for moderate and high levels of WPI (D{sub {perpendicular}}(O{sup +})>1), the distribution function f(O{sup +}) displayed very pronounced conic features at altitudes around 3R{sub E}. Finally, the interplay between the downward body force, the upward mirror force, and the perpendicular heating resulted in the formation of the {open_quotes}pressure cooker{close_quotes} effect. This phenomena explained some interesting features of their solution, such as, the peak in the O{sup +} temperature, and the formation of {open_quotes}ears{close_quotes} and conics for f(O{sup +}) around 2.5R{sub E}. 10 refs., 2 figs.

OSTI ID:
166285
Journal Information:
Geophysical Research Letters, Vol. 21, Issue 21; Other Information: PBD: 15 Oct 1994
Country of Publication:
United States
Language:
English

Similar Records

Monte Carlo study of the transition region in the polar wind: An improved collision model
Journal Article · Fri Oct 01 00:00:00 EDT 1993 · Journal of Geophysical Research · OSTI ID:166285

Stability of the polar wind
Journal Article · Wed Apr 01 00:00:00 EST 1987 · J. Geophys. Res.; (United States) · OSTI ID:166285

Centrifugal acceleration of the polar wind
Journal Article · Mon Aug 01 00:00:00 EDT 1994 · Journal of Geophysical Research · OSTI ID:166285