Polar wind survey with the Thermal Ion Dynamics Experiment/Plasma Source Instrument suite aboard POLAR
Authors:
- Yi‐Jiun SuYSYi‐Jiun Su
- J. L. HorwitzJHJ. L. Horwitz
- T. E. MooreTMT. E. Moore
- B. L. GilesBGB. L. Giles
- M. O. ChandlerMCM. O. Chandler
- P. D. CravenPCP. D. Craven
- M. HiraharaMHM. Hirahara
- 1 December 1998
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 103 (A12) , 29305-29337
Abstract
In February 1996, the POLAR spacecraft was placed in an elliptical orbit with a 9 RE geocentric distance apogee in the northern hemisphere and 1.8 RE perigee in the southern hemisphere. The Thermal Ion Dynamics Experiment (TIDE) on POLAR has allowed sampling of the three‐dimensional ion distribution functions with excellent energy, angular, and mass resolution. The Plasma Source Instrument (PSI), when operated, allows sufficient diminution of the electric potential to observe the polar wind at very high altitudes. In this paper, we describe the results of a survey of the polar wind characteristics for H+, He+, and O+ as observed by TIDE at ∼5000 km and ∼8 RE altitudes over the polar cap during April–May 1996. At 5000 km altitude, the H+ polar wind exhibits a supersonic outflow, while O+ shows subsonic downflow, which suggests a cleft ion fountain origin for the O+ ions in the polar cap region. Dramatic decreases of the 5000 km altitude H+ and O+ ion densities and fluxes are seen as the solar zenith angle increases from 90° to 100° for the ionospheric base, which is consistent with solar illumination ionization control. However, the polar cap downward O+ flow and density decline from dayside to nightside in magnetic coordinates suggest a cleft ion fountain origin for the polar cap O+. Cleft ion fountain origin O+ density plumes could also be partially responsible for a similar day‐night asymmetry in H+, owing to the charge‐exchange reaction. At 8 RE altitude, both H+ and O+ outflows are supersonic and H+ is the highly dominant ion species. The average bulk ion field‐aligned velocities are in the typical ratio V0+ ∶ VHe+ ∶ VH+ ∼ 2 ∶ 3 ∶ 5, which may suggest a tendency toward comparable energy gains, such as via an electric potential layer.Keywords
This publication has 70 references indexed in Scilit:
- Observations of downward moving O+ in the polar topside ionosphereJournal of Geophysical Research, 1995
- The Global Geospace Science Program and its investigationsSpace Science Reviews, 1995
- The effect of wave‐particle interactions on the polar wind O+Geophysical Research Letters, 1994
- Altitude profile of the polar wind velocity and its relationship to ionospheric conditionsGeophysical Research Letters, 1993
- ‘Self‐consistent’ production of ion conics on return current region auroral field lines: A time‐dependent, semi‐kinetic modelGeophysical Research Letters, 1991
- Observations of polar ion outflowsJournal of Geophysical Research, 1991
- Effect of hot electrons on the polar windJournal of Geophysical Research, 1984
- O+ ions in the polar windJournal of Geophysical Research, 1983
- Altitude variation of ion composition in the midlatitude trough region: Evidence for upward plasma flowJournal of Geophysical Research, 1971
- Features of plasma transport in the upper atmosphereJournal of Geophysical Research, 1969